№ſ ſae §§§ **** Ķ ::::: ##### Řł §§§§::: įſigiſ 㺠*::: ¿¿.** ###### sºr; #########|- * º tº § * ##### *、:######::::::::: }}#############§§§§§); § 3:4,ſkſ;£!3;;;;;;; }$ſ;};}; Ķī£; §:ſſae; *! *(#:; ####« %¿?→·§\, ſaei####### · … ,; sa: +£########čt ##ſae#---- ,##.* Źź#ffff;ī£; ſae~~~∞ #,#ffff;{{Ž · e |-… * * • ... *** *T**, …….. ·****~~). } ț¢;Ģx §§** …“. -*<!--* ~ ######ËËĚĚĒĒĖĖĘĚĖĒģ ĒĒTĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĪĘŅŅŇŇſ# Eq E \ ,-§§H- EE| $ º \\(\\),\\§. ĒĒĖ,!Dæ! } Eſ. ENº.Þ^»G ĒĒÅÈY º E}; } ſ ==§: EFĐ<>§-ſ ·!~$=}| N،ſ (~ }-} (}})º3#### №ſſae!č SS=№M ●El ſ ·?={$2## |----· •■; : ! EĶÅ-{ EŤſ,§ 3 ĒĒffffffÈÉſ i ĒĒĶ* -->} | |-, E- £ €U ĒĒ|×}); ĒĒĒ. - H: ~~~~, , , ,## Ē§Á%ſ,%ſ|\[№ſūIIIIIIIIIIIIIIIIIIIIIIIIIIIIË}} ſiiſ IIIſTTTTTTTTTTTTTTTT:ſ №ſhillſ”.~--~~~~~); TJR. } + (2 , T 53 PHOTOGRAPHY FOR YOUNG PEOPLE rººf-ºr- ºx r--a < *- J ..+…ºrs:- - -, --, - - - - - - --- * * * * - - - - Photograph by Mr. Vivian Burnett * THE Young ARtist'' An attractive portrait, showing artistic judgment. Though the sunlight is shining through the window, there is no glare or fogging from it. PHOTOGRAPHY for YOUNG PEOPLE By T U D O R J E N K S AUTHOR OF “ELECTRICITY FoR T young PEOPLE” NEW YORK FREDERICK A. STOKES COMPANY PUBLISHERS tº- Copyright, 1908, by FREDERICK A. STOKES COMPANY September, 1908 All rights reserved Preface THE first thing to understand about photography is that we may mean by the word two very different things. As the word is used by men who have given the greater part of their lives to the study of the subject, it means a deep science and a marvellous art, to understand which completely is hardly possible even to the deepest students, the wisest philosophers, or the most painstaking workers in the laboratory. To them the whole art is full of deep questions, any one of which requires for its full understanding years of study and experiment. Photography in this sense belongs to men of science, who for our benefit solve its puzzles and tell the world what they have learned. Fortunately for most of us, photography means also something far easier, much pleasanter, and more useful. There was a time when the great land of photography was like an unexplored, pathless wilderness or forest, through which only the hardy pioneer could make his way a step at a time, gaining every advance at the cost of a dozen painful blunders. But, owing to the labours of these pioneers, at first the good paths were found, and then were by other workers widened into roads, and made so easy that even a child's feet may travel in them safely, surely, and easily. To study the science of photography is to learn how these paths were first opened and then made into W 2055 i 5 Vi PREFACE broad roads. But to travel in the highways that have been prepared for us later comers is in no way difficult, and is full of pleasures. It is believed that the reader of this book will wish to do more than merely make his way along the easy routes that have been prepared for him. It is hoped that he will wish to know at least the outline of the work that has been done to make photography a daily pleasure instead of an absorbing and difficult study. But at the same time we shall try never to forget that for most of us the attraction of photography lies in the making of good pictures, and that the history of the art and the study of its processes are chiefly valuable because they teach us to make good pictures by knowing just what to do and just why each thing is done. In this book we shall try to tell even the beginner how he may learn to use his camera, his chemicals, and his material, to the best advantage. We shall not forget that some like to work without bothering them- selves about why results come; for such we hope to give plain directions based upon the best authorities. For those who wish not only to do good work, but to be able to vary the work and to understand each step they take, we shall try to give equally plain explana- tions pointing out the reasons for what is done. We believe, however, that to any user of a camera who learns to enjoy his work, the wish to know more and more about the art and the science that gives him beautiful pictures or valuable records is sure sooner or later to come. Once the wish to study out the art and mystery of light, lens, camera, and print, is born, the student may be safely left to himself. He will need PREFACE Vii no urging to give time enough, and possibly too much time, to the fascinating work that has all the delights of an art and all the depths of a science. In choosing the three great helpers that have made our times different from the past, a recent thoughtful writer, George Iles, chose flame, electricity, and the camera. Flame was the first great servant that savage man won from nature; electricity, the second, seems rather a powerful genie than a servant; but he, too, has been reduced to bondage. Of the camera we can hardly speak in the same sense as a “servant.” It is, rather, a faithful friend and an intimate com- panion who helps us to enjoy and to understand what we see, to remember what we do not wish to forget. At first, this new friend seemed but a pretty child to amuse man's lighter hours, but as the years have brought fuller growth, the child has become man and has won the right to be thought of as a most powerful helper in all man's work. As printing makes the result of thinking immortal, so the camera has made lasting the result of seeing; as books tell us what men thought in the past, so will the camera tell the future what men saw in the past. All over the world the camera shutters are snapping; at every instant thousands of cameras are recording the forms of clouds, of waves, the beauties of land- scape, the happenings in the great drama of nature. They are noting for our children how their fathers and mothers lived, what were their surroundings, what they did. They are saving from forgetfulness types of men and women, quaint happenings, occurrences both commonplace and strange. From the life of a king to the coming of a butterfly viii _* PREFACE from its cocoon, the camera records all; nothing is too great or too small for its attention. None of us are too grand or too obscure to be left out of its dark box. By its aid we may see again the faces of those who are gone, may recall places that are changed or beyond our reach, may live again in our pleasures and See again the sights that have delighted us. From the camera come pictures moving us to laughter or to tears; records that teach the wisest or explain what is deep to the simplest. Perhaps as well as being his daily friend and companion, it may become man's most useful helper. I. II. III. IV. V. VI. VII. VIII. IX. Y. XI. XII. XIII. YIV. XV. XVI. YVII. XVIII. XIX. XX. XXI. XXII. XXIII. XXIV. Contents SOME INTRODUCTORY NOTIONS © © WHAT THE CAMERA IS . º e o GENERAL PRINCIPLES OF THE PROCESS . CHOOSING A CAMERA e © e FIRST USE OF THE CAMERA . º º LEARNING ABOUT EXPOSURES. e º FIRST STEPS IN DEVELOPING . e º MAKING A PRINT . e © º º WHAT TO PHOTOGRAPH . º © Q OUTDOOR PHOTOGRAPHY . º e PHOTOGRAPHY INDOORS . º º e FROM RULE OF THUMB TO KNOWLEDGE . ABOUT LENSES AND THEIR QUALITIES . THE CAMERA AND ITS ATTACHMENTS . PRACTICAL HINTS ON EXPOSURE . MODERN DEVELOPING © © FURTHER REMARKS ON DEVELOPING — AFTER TREATMENT OF NEGATIVES . PRINTING — METHODS AND PROCESSES LIGHT AND ITS ACTION . © o THE BEGINNINGS OF PHOTOGRAPHY FROM THE DAGUERREOTYPE TO THE DRY PLATE . e & ſº tº e A GLANCE AT MODERN PHOTOGRAPHY COLOUR WoRK AND OTHER APPLICA- TIONS OF PHOTOGRAPHY e SOME HINTS ON THE CHEMICAL SIDE APPENDIX e e tº e e e INDEX & * e o e º ix ~~~~3rº-ºr--ºf-i-º-º-ºrrºr--ºvº. (~~~~--~~~~~~)*----~~~~--~~~--~~~~, ILLUSTRATIONS “The Young Artist’” e e G Q * Ç Frontispiece Camera Accessories . ſº e • * * © © “The Man on the Box '' . O . . c ſº e “Broadway in a Snow-Storm’” . º º º © e Effective Photographs Taken With Small Cameras . © Instantaneous Photography e © e e © e A Pinhole Photograph • • e * & The Magnifying Power of a Telephoto Lens o te e Camera Accessories & e e & e § tº Photograph made with a Focal-plane Shutter, at Slow Speed The Effect of Focal Length in Photography e O & “Sunlight on Surf" . ſº © º © Q Ç © A “Firelight " Photograph & {} C G O © Monument to Daguerre . iº e e C O G A Night Scene . c © An Unusual Scene in New York Harbour A Duplicate Portrait O o © 140 150 156 160 166 192 202 236 270 PHOTOGRAPHY FOR YOUNG PEOPLE |-} ‘… '?*: < < *-*á«nåkešº-->.………_ _ Y) • *…*…:) -----------~--~~~~u (~~~~ ~~~~x~&& (~~~~*.*)?-******************************************)^*,,,,,,,,,,,=,<>)•••••••••• --~~~~ ~~~~--~~~~ ~~~~~ ~~~~ ~~~--~~~~--~--~~~~~--~~~~ ~~~~ ~~~~ ~~~~~--~~~~~------…-- ~- - - ---- ------- -- t Photography for Young People CHAPTER I SOME INTRODUCTORY NOTIONS Photography and its value in general – As a pleasure and as a useful helper — What can be done with simple apparatus — What the amateur should know — What part of the work he should do. IN a number of that bright little magazine for ama- teur photographers, the Photo-Miniature, an opin- ion is quoted from John Richard Green, the English historian, to the effect that photography was “the greatest boon conferred on the poorer classes” by re- cent inventions. This opinion was called out by a talk he had with a friend who was praising schools, museums, and other things tending to make the poor man's lot happier. But Green points out that by making it cheap to own portraits of one's family, the happiness of the poor, who by the need of making their living are often sep- arated from one another, has been increased more than any one can tell. As Green said, the little row of por- traits over the fireplace still keeps alive in the home the memory of “the boy who has gone to Canada, the girl out at service,” the little one who died, the old grandfather who still remains in his country home. The writer who quotes this opinion says also that these words carry the more weight since Green had been for years a hard-working clergyman in a poor l 2 PHOTOGRAPHY FOR YOUNG PEOPLE district of London, and knew intimately the life of the poor. This is the side of photography of which we all know something, and of late years the little home pictures have become so common that they serve as records of more than mere portraiture. At first they Were, of course, stiff and dignified pictures of members of one's family; but now there is no side of family life, no daily happening, however trivial, no cause for tears or laughter, that may not have its lasting record in one's pictorial diary. While it has gained greatly in Value as a profession or a business, and has widened enormously as an art and science, it has likewise become a most fascinating pursuit, amusement, and pastime. - According to the use we each make of it is the time we can afford the camera. If it is to be no more than a means of fun, we shall choose in all ways the easiest methods, shall not trouble ourselves to learn more than to press a button, and shall care little about the expense or the waste coming from the numerous failures we shall be sure to have, being satisfied by an Occasional pleasing or amusing picture, the result of some rare good luck. .” But no young person who is wise and foreseeing should be content with mere dabbling in the art. There is too great a chance that any one of us may find that the work of the camera will play a most important part in his future. There is hardly a busi- ness or profession in which photography does not have an important place, even if photography were not often a means of money-making in itself. - As a means of education, too, picture-making with SOME INTRODUCTORY NOTIONS 3 the camera may nowadays be compared not unfavour- ably with drawing itself, and a great authority on education, the French architect, Viollet-le-Duc, de- clared drawing to be the true basis of all practical edu- cation. He who uses the camera soon comes to look with a new eye upon everything. If he is already a draughtsman, he will find that the taking of photo- graphs has increased his power of composition, or put- ting together of pictures; his knowledge of light and shade, his familiarity with outline, his knowledge of form ; and particularly with the attitudes, gestures, and motions, of living things. Indeed, it may be doubted whether the artist in his long study of a single subject acquires such a training as comes to the photographer who can study in the same length of time twenty subjects. For if the camera is used with thought, as it must be by those who become interested in its work, it induces the photographer to study a hundred possibilities of pic- ture-making for every photograph he takes. It will teach him perspective, it will acquaint him with the beauties of landscape, and, indeed, should make him an artist, with the one exception that it does not yet train directly the colour-sense except as it gives keen- ness of eyesight and inclines the mind to notice the beauties of natural appearances. But even colour pho- tography is sure to be accomplished. More and more every year are men and women find- ing their work in different fields of science ; and there is no scientific work which does not depend more or less upon the use of the camera. To the student of nature it has become indispensable, and has made him able to do mechanically the picturing of the living 4 THOTOGRAPHY FOR YOUNG PEOPLE animal or plant in a way that was once most imper- fectly done by laborious use of the pen and pencil, even when these were wielded by genius. In botany, geology, forestry, in surveying, in exploring, in medi- cine, in astronomy, the camera is playing an increasing part as years go on. George Iles, in his “Flame, Electricity, and the Camera,” has called the camera the “handmaiden of literature,” and has, in the book mentioned, shown Something of the thousand and one services ren- dered by photography in every field of human work. In all these fields our boys and girls will find their life-work, and that work will be the easier if they have already acquired cleverness in the use of their cameras and ability to understand its results. It is not at all improbable that before many years a knowl- edge of photography will become a branch of educa- tion considered an essential to every boy and girl who means to enter the battle of life well equipped to at- tain success. But even were all this not so, even if we could con- sider the magic “dark box” as nothing more impor- tant than a pleasant companion, the reader is assured that the time spent in learning how to use it and to understand what it can do is well spent merely as an education in science and in learning how to see and to observe understandingly. Just as the college student studies many branches simply because they prepare him to acquire other things more readily, so the ama- teur photographer — using the word “amateur’ in its right sense, as meaning one who practices photography for pleasure — will learn from it how to understand SOME INTRODUCTORY NOTIONS 5 better the world around him and to enjoy more what- ever brings pleasure to the eye. We believe, however, that no mere words can give as clear an idea of what photography is and of what it brings to him who practices it, as will come from even a mere beginner's first use of the art itself. With the use of the camera and the pleasure of pic- ture-making will come the curiosity as to hows and whys and the desire for skill in accomplishment that will lead the amateur to read more widely and to practice with more freedom the rules that are laid down for his help. For this reason we shall not ask you to begin with the history of how photography came to be, nor with long explanations pointing out just the laws according to which experts are guided in giving us our rules of working. We shall, instead, suppose that you either have, or mean to have, a camera, and that you will, as Soon as you have knowledge enough, begin at Once the taking of pictures and the making of prints. We shall, therefore, begin by telling you a little of how photography is done, and then proceed by advis- ing you how to choose a camera, or to make the best use of those not too complicated for the beginner. Fortunately, most of us cannot afford to confuse our- selves by doing elementary work with the compli- cated machines needed by the advanced photographer. We begin with the simpler work, try to do that well, and thus learn to walk before we run. Fortunately also, there is very little that cannot be done even with the simpler forms of apparatus. The more complicated cameras and the more difficult proc- esses are seldom needed. A recent photographic 6 PHOTOGRAPHY FOR YOUNG PEOPLE annual gives us the marvel of a humming-bird pictured in the air apparently with motionless wings. We see in similar journals, or in the periodical press, examples of other triumphs of skill — objects taken in rapid motion, photographs taken on a large scale, flashlight jungle pictures, views showing feats of mountain climbing that must have been secured at the risk of the photographer's neck — but we shall come to all these soon enough. A really good photographer is one who will secure results that are beautiful, valuable, or interesting, even if he has no better apparatus than a pasteboard box with a pinhole lens, or a cheap camera that con- sists of little more than this with the addition of a tiny lens. So do not let the fact that you cannot own an expensive camera and cannot afford hours of study to acquire new processes, discourage you in seeking to become entitled to the name of a skillful photog- rapher. The very best work that brings about a good photograph is done within the human skull, and so it will ever continue to be. The camera and its plates, the prepared papers and the necessary chemicals are to-day made ready for our use, and are of such excellence that no one can fairly complain of his apparatus. If there is a failure to secure good pictures the chances are that the trouble is with yourself — either lack of care, lack of skill, or lack of knowledge. You may for a small amount to-day procure a better camera, better materials — better everything — than the early photographers could command without the exercise of their highest skill and the most painstaking care. In fact, the modern photographer who fails to make SOME INTRODUCTORY NOTIONS 7 good pictures should be ashamed to bring to nothing by his carelessness the elaborate and excellent work of the manufacturers who furnish him with his apparatus. The reader of this book is asked to believe, at the beginning, that in spite of all he may be told by dealers interested in making him spend money, he can- not take good photographs unless he understands the reasons for what he does. By accident any one may now and then get a good picture, especially if he has a great part of the work done for him; but any one who uses a camera will find it an expensive and irritating instrument unless he learns how to use it, and why he does things. But one can learn easily, and then the camera will be a delight, an educator, and a most valuable companion all one's life. The study of photography is full of interest and pleasure. Even a little knowledge will not only greatly increase your ability to take good pictures but will also teach you to enjoy the work of others — to know how to appreciate the thousands of pictures reproduced in books, papers, and magazines, or made by amateurs. We need not know all the science of the subject, but we may easily know the hows and whys of the camera, the plate, the developing and fixing chemicals, and the most usual printing methods. All this depends first on knowing something about light — for the photograph is the child of light, and obeys the laws of its parent. Next we must become acquainted with the machine that is used for taking pictures, so that we know the 8 PHOTOGRAPHY FOR YOUNG PEOPLE purpose of each of its parts and can understand how it is to be made ready for picture-making under different circumstances. And here, nowadays, many will stop, at least for a while. They will be satisfied to make the exposures, and will turn over all the rest of the work to others. We desire to say that there can hardly be a greater mistake for the young photographer than to be con- tent to learn only the use of the camera without learning also to do every bit of the work that can be done by the amateur. There are certain things which it is better to buy ready-made. For example, the preparing of plates and films is so delicate a piece of work, and is so much better done by the great firms who sell the best-known brands, that there can be no good reason for trying to make one's own emulsion and to prepare one's own plates or films, except as a matter of study. But as to the developing and printing, it is not too much to say that no one can be a good photographer or can know what may be done with the camera unless he learns to develop his own negatives and to print from them by at least the usual proc- €SS6S. Perhaps not every reader knows that of late years there has been a complete change in the whole art of taking photographs. There was a time when the amateur who meant to go into photography found himself obliged to set apart a special room, to stock it with a great array of chemicals, to provide all sorts of apparatus, and to devote a large part of his time to picture-making. Some writers on the subject regret that these days have passed away, believing that when amateurs were forced to do every step of the SOME INTRODUCTORY NOTIONS 9 work they became interested and acquainted with all the facts, and so were likely to make discoveries and improvements. But the subject to-day is far too big to be covered by any one amateur, and in order to study a part of the subject thoroughly, or to learn enough to make good pictures, does not require either special dark rooms, many chemicals, or a large part of your time. It is necessary, however, even for one who has no purpose beyond the making of pictures that will please himself and his friends, to understand what takes the picture, meaning by this the action of the light and the use of the camera. He must also know at least the commoner ways of developing and the most usual methods of printing. In fact, there is, even in this simple outline, plenty of opportunity to study out the best ways and to become skillful in them; for although the directions given by those who sell cameras and materials are made as simple as can be, and need only to be followed in order to get excellent results, yet the amateur will soon find that there are cases arising con- stantly that require him to think for himself and to make slight changes in what he is directed to do. CHAPTER II WHAT THE CAMERA. IS. Derivation of “photography ’” — The nature of light — What light is used in photography — The rays of the spectrum and their powers — Which rays are used in photography — The purpose of the camera — The simplest form of camera — Explanation of the pin- hole camera — The bending of light rays — How a prism acts — A lens like a number of prisms put together — The purpose of the lens in the camera. THE names that we use for things nearly always, if we understand how they came to be given, show us what those things were in their simple form. The word photograph comes, as you probably know, from two simple Greek words, 40s and Yodºety. The first comes from a verb that means “show,” and thus signi- fies “the thing that shows other things”; that is, light. The second word comes from a verb that is of great use in making compounds. It is often spoken of as meaning “write,” but really, in Greek, the verb had a wider meaning and was more in meaning like our word “mark.” It could be used of any action that left a trace, a mark, a cut, or a print. So the compound word, “ photograph,” really means to mark by light, or what has been marked by light. In order, then, to understand exactly what pho- tography is, we shall need, first, to know something of the nature of light. Of course the great source from which we get most of our light is the sun, and in early days photographs were sometimes thought of as “sun-pictures”; but it is a wrong way to think of 10 WHAT THE CAMERA. IS 11 the subject to look upon the sun as if it were the only source of the light used in photography. Any kind of light, whether coming from the sun, from the moon, from the stars, from the action of chemicals on One another, from electric action, or from even more un- usual sources. •rch as the action of radium and other light-giving substances or living creatures that are phosphorescent, may be used in making photographs, and has been so used by scientific men in studying nature. Neither is it right to think of photographs always as pictures. To speak correctly we must include under the name “photograph * any visible effect of light upon substances. It may be well to show that this is not merely a fussy way of talking. For blunders will be made, if we think of photographs as being caused only by the direct or indirect light of the sun. In handling mod- ern dry-plates any one who thought that they would not be affected except by the sun or by daylight, would be careless about exposing them too long to the light of his ruby lantern, or might not understand that a roll of film could be marked in branching lines when unrolling it too rapidly had made it give out electric sparks. - These two instances are given to show that it is best from the beginning to understand that a clear idea of photography teaches us that it has to do with any source of light. So, in trying to understand the nature of light, we must get an idea of light in general, at the same time remembering that to us on this earth the most important light, of course, is that which comes from the sun. 12 PHOTOGRAPEIY FOR YOUNG PEOPLE The reader must not get an idea, however, that the sun, or any other source of light acts directly on the plates within the camera, as it does on the paper with which we print from the negative afterward. The rays that enter the camera through its lens are those received from the objects that we photograph — not reflected from them unchanged, as from a mirror or polished surface, but partly absorbed, and partly modified in many ways, according to the colours and the dark or light places in the objects. When we say that we see dark and light in a scene, we mean that we receive in our eyes light-waves in greater or less amount; and when we say that we see different colours, we mean that certain parts of the scene con- duct to our eyes only red rays or yellow rays, absorb- ing all the other kinds. Just as every separate shade or colour affects our eyes differently from every other, so it affects the plates, making a different impression on different parts of it. You can understand this better when you see the beautiful image the lens throws on the ground glass ; and it may interest you to know that the eyes are in fact little cameras, each with a perfect lens and a sensitive surface back of it, on which the images are thrown. We expect in a later part of this book to give a rather full explanation of what light is supposed to be, and of how it acts to make changes in the plate that en- able us to develop a negative. At present we shall tell only the few things that must be known by every practical worker to keep him from making mistakes and to guide him in the use of his camera and its fit- tings, as well as the after work of getting a finished negative and from it a finished print. WEHAT THE CAMERA. IS 13 These few facts have first to do with the kind of light that makes photographs. It will be explained later that in the ordinary light of day there are differ- ent sorts of light rays, each having a different effect; but, just now, it is enough for us to remember that the light rays which make a photograph are not altogether the same as the rays by which we see. But perhaps it would be plainer to say that part of the light rays are best for seeing, while others are best for taking photographs. When light is broken up by means of the prism into the different coloured rays which go to make white light, we shall find, broadly speaking, that there are three portions differing in colour — the red, the yellow, and the blue. Of these, those rays that are found toward the red end of the spectrum have very little power on the ordinary photo- graphic plate; those around the yellow part, while slightly photographic, are at their best in helping us to see. Toward and beyond the blue end of the spec- trum we find the most active rays used for photography. This will show at once that the eye cannot surely tell us whether a subject for the camera is going to affect the plate in the same degree that it affects the eye. This is well known even to beginners with the camera who have tried to photograph flowers, for ex- ample, and have discovered that, so far as the photo- graphic plate is concerned, it makes little difference whether a flower be blue or white, or, on the other hand, whether it be red or nearly black. The blue — together with purple and violet–affects the plate nearly as much as the white; whereas the weak and the red and the yellow rays all fail to produce much, if any, effect through the camera. 14 PHOTOGRAPHY FOR YOUNG PEOPLE By this state of things it is brought about that we must, in photography, always bear in mind that we are trying to use, not the rays that we see, but the rays that act most through the camera. In many cases, of course, this will not make a very great differ- ence, but now and then the knowledge of the different rays will make all the difference between a good picture and a bad one. Of course the taking of a photograph means no more than causing the proper light-rays to act upon a surface made ready for them; and the camera, whether it be a mere box with a tiny hole in the end or a most elaborate instrument having a great number of attach- ments, is, after all, nothing but a means for the shut- ting out of all light except the particular part that we wish to use, and for letting in those rays that are to make the picture, in the right amount and for the right length of time to act upon the plate. This may seem to the reader at first as a primer- like way of stating a well-known fact, but it will be found, when we take up the question of using the dif- ferent parts of the camera and using them rightly, that we shall in this simple idea have a key to the right use of the most complicated apparatus. We know that the image within the camera is formed by separating from the numberless rays which are reflected from or sent out from any object, enough of them to give us an image more or less distinct ac- cording to what we want to have upon the plate, and at the same time to shut out all the other rays that would interfere with the correct image. The simplest form of camera, then, is a mere light- tight box that will keep out all rays of light except WHAT THE CAMERA. IS - - 15 those let in at one tiny opening or gate. If this gate is not small, the rays coming through it will be mixed up and we shall have no clear image formed ; but, if we make the gate small enough, we shall shut out all except a few chosen rays, and these will give us an image of whatever is opposite the little opening, for all light rays travel in a straight line if not interfered with. (Diagram I.) _--~~ .* _** ... → • * --> * _----T •T_-- - - - * * ST-- - - Y- *>- - * - -- S. *s *~~ * ~ TS- DIAGRAM I If, in such a camera, we put a sensitive plate so as to receive this image, we can take photographs, al- though we have no lens, rightly so-called, no shutter, no means of focusing and no plate-holders or other aids to the mere dark box with a hole in it. Let us keep this in mind as a foundation on which to build a right idea of photography, for in this simple box We have all that is really needed to take a picture. But so soon as we ask to do more, we shall have to improve this box in many ways. The little hole, in order to make a clear image, will, as experiment shows, 16 PHOTOGRAPHY FOR YOUNG PEOPLE need to be only about large enough to let a fine sew- ing-needle pass through it. Just so soon as one tries to make a larger opening to let in more light, he will find that the image becomes confused and spoiled, be- cause the rays of light go through in all directions and the effect is simply to light up the whole plate, instead of forming an image on it. If we make a big opening it is just as if we should punch a great number of little needle-holes close to- gether, causing their images to overlap one another so that we could not distinguish one from the other, and so that the different coloured rays would be all mixed up together, forming a white light, and merely light- ing the plate instead of forming a set of pictures upon it. The whole subject of lenses, stops, and focusing, depends upon understanding this state of things. All the space around us is full of crossing and re- crossing images. They interfere with one another when received on a surface unless we can shut off all but one, or can cause more than one to fall exactly upon the same space inside the camera. By means of the pinhole we make what is really one image, for al- though a number of light rays may go through together, yet the images they form are so nearly in the same place that we see a picture almost clear. But it is not entirely clear, and so the image formed by the pinhole is always a little blurred. Now let us see how a lens betters matters. We have seen that the few rays coming through a very small opening are kept separate, and that the image made by them is not confused. If, now, we try to make the hole larger, we get confused images, because it is the WHAT THE CAMERA. IS 17 same as if a lot of small holes were put close together, each forming an image at a different place. What we wish to do is to make a big gateway so that we can get as many rays as possible, and yet to bring all these rays into the path that would be travelled by them if they all had to come through the one small pinhole; that is, we want to bend them from their straight line of travel and send each ray where the other rays coming from the same point of the object are coming. To help make this important matter clear, let us suppose that we have three boxes, each with a pinhole in it, and each making an image. Now let us join these three boxes and make a sort of a treble box with three fronts and one back: `-------" ** --~ *" Y-- e” 4. º ><. **-><ſ - *s .* º *~~~~ º Cº- sº DIAGRAM II If we could take the three images formed by the three pinholes and make all of them fall in ea actly the same place, we should have an image three times as bright and clear as any one of the boxes would make alone. But we can do just this thing if we put into two of the pinholes little prisms that will bend the rays of light just enough to bring all three together. It will be necessary, to see how this is done, that we should 18 PHOTOGRAPHY FOR YOUNG PEOPLE understand the effect of transparent things in bending the rays of light from their paths, for it is easy to see that if we should so bend the rays we could bring all the images together. This bending is found to come whenever the rays of light pass from a thicker to a thinner substance, or from a thinner to a thicker medium. Experiment proves this, and it is not neces- sary for us just now to know more than that the path of the rays is changed. To understand just how light- rays are thus bent would require a long study into the theory of light waves. In fact, no one fully under- stands it. Perhaps the easiest illustration of this bending of the rays is observed when we thrust a stick into the water. We know that the stick does not bend, and yet any one who tries the experiment will see that it looks bent where it enters the water. This is be- cause the path of the rays of light is changed. In going from air into glass and from glass into the air again there are two bendings of a ray of light. If this ray goes through glass having parallel faces, as in the case of a plate glass window for example, the ray is first bent from its path on entering the glass, and is then bent back again just as much on going out, so that the general direction of the ray is not changed. (See Diagram III.) - But if the two faces of the glass are not parallel, but are inclined one to the other as in the case of a prism, the direction is changed upon entering the prism and again changed on coming out, but in a dif- ferent degree, so that the ray takes now a new direc- tion, which it does not do in going through the pane of a plate glass window. We can alter the direction WHAT THE CAMERA. IS 19 of the ray less or more as we like, by changing the way in which the two faces of the prism are inclined toward one another. DIAGRAM III Here, then, we have a means of bringing more than one image sent out by the same object to the same point. If we arrange a set of prisms rightly, we can direct a number of rays to the same point. Thus in Diagram IV we see that by two prisms we can make two rays from a single point on one side DIAGRAM IV of the lens meet at a single point on the other side, while plain glass with parallel faces in the middle would let a straight ray through in the middle. By 20 PHOTOGRAPHY FOR YOUNG PEOPLE making a circular ring of prisms (Diagram V) a whole ring of rays could all be brought to one point. Now we have only to suppose our ring of prisms to be melted together on the edges and the centre to be DIAGRAM W. filled up, and we shall have a lens such as is used in bringing the rays to a point. (Diagram VI.) You will notice that in these three diagrams I., II. and IV., we have used the same lettering — A for the DIAGRAM WI top of the object, B for the centre, C for the foot; a for the top of the image, b for the centre and c for the foot; and P stands for the “pinhole.” The line A Pa in WHAT THE CAMERA. IS 21 each figure shows the course of a light ray proceeding from A ; and BPb the course of one proceeding from B and so on. If you look at Diagram I, we think you will understand why the image thrown on the plate is always upside down, for no rays from A can reach C. In Diagram II we are supposing that our three pinholes will bend the rays just as we want them to go; so there are three rays from A, meeting at a, and three from C meeting at C ; and therefore three im- ages of AC, one on top of another. In Diagram IV, we have merely taken away the boxes, leaving only the prisms, so that you may see how they bend the rays. P cannot really mean “pinhole" in this figure, therefore, but we use it because, like a pinhole, the prism receives rays from A, B, and C, and distributes them again on the other side, in reverse order. A mere prism of course, cannot make an image, but can Only bend rays; but a lens, which is like a hundred kinds of prisms arranged rightly and then joined as if melted together, gathers all of the rays from all of the points of the object (within the angle of vision), and bends each ray just where it is needed for making the image. Thus we see how different the lens is from a pinhole, which (theoretically at least) lets in only one ray from each point of the object. A lens is like an infinite number of pinholes throwing their images one on top of another. It must be remembered that we can, if we like, by changing the shape of the glass through which rays are sent, make the rays bend in any direction. If, in- stead of putting our prisms thin edge outward, we put them all thin edge inward and suppose them again to be united into a lens, we would have a lens that would 22 PHOTOGRAPHY FOR YOUNG PEOPLE make the rays separate or diverge, instead of uniting. (Diagram VII.) This sort of lens also is useful in photography. Later on we shall explain the different classes of lenses, but it is enough now to understand that the simplest use of a lens is to bring a number of images within the camera to the same point and thus to get a brighter image because it is one made up of a great number of light rays. DIAGRAM WII Having followed this reasoning, it is evident at once why a photographer who could have a lens would never be satisfied to use the pinhole, unless for certain peculiar effects. Since the pinhole uses only a very small amount of light, it takes a very long time for its image to act upon the plate within the camera—so long that even under the best circumstances a pinhole might take three or four minutes to affect a plate as much as a quick lens would do in the five-hundredth part of a second, or less. We therefore now understand why a camera must be a light-tight box except where light comes through WHAT THE CAMERA. IS 23 to make the picture, and we also see what use there is in the lens. These matters we shall look into more closely afterward, trying now only to get the general ideas necessary to practical work. CHAPTER III GENERAL PRINCIPLES OF THE PROCESS What receives the image — The silver compound — The sensitive plate — What we must do to the plate — Avoiding light, pressure, moisture, heat — Putting the plate into the right position to re- ceive the image — Making sure the rays have a clear path to the plate — Why motion spoils a picture — Exposure depends on colour and strength of light — Care of the exposed plate — Its develop- ment — Water the true developer — The action of the chemicals — Fixing the plate — What a negative is — Using the negative to make a photograph — The few main principles. THE next matter is the question of receiving the image after it is brought to the right place in the camera. As before, we begin with the simplest way of thinking of the subject. It has been found that when light is allowed to shine upon certain compounds of silver it has the prop- erty of changing them chemically — that is, it changes their very nature. Two or three of these compounds have been found especially sensitive, and the plate or film that goes into the camera consists essentially of two things: first, the silver compound ; second, what holds it in place. The way in which the compound is prepared results in making a sort of a milky liquid containing the silver preparation mixed thoroughly with a gummy substance. This is prepared and spread upon a support, which may be either glass, celluloid, paper, or anything else that will hold it in place and will not interfere with its chemical properties. Upon 24 GENERAL PRINCIPLES OF THE PROCESS 25 this it dries (all the latter part of its preparation being carried on in a place free from the chemical rays of light) and with its supporting plates or films is then packed so as to keep it from any exposure to this light except such as is given to it in the camera itself. It is not important for us yet to consider just what sort of a support is used for the sensitive coating, as we are going to talk about things that are necessary no matter what sort of support is used ; and we shall take up the matter by thinking of the three steps in the making of a picture on a sensitive surface. We will call this surface a “plate,” meaning by that word to include not only glass plates, but films, whether in rolls or cut into separate pieces, and also any other methods of preparing the coating to be exposed in the Cà IIle I’8. The plate, then, comes to us packed away from the possibility of being touched by light, and with it we shall have to do three separate things. These three steps require, first, that the plate be kept from all things that will make an impression upon it until we are ready to expose it in the camera; second, that the plate be acted upon only by the rays desired to make the picture; and, thirdly, that the plate be changed after exposure from a sensitive plate into an insensi- tive negative that light will not affect. Before exposing, one most important thing is that there should be no light rays allowed to strike it ex- cept rays that will not produce an impression. So much you all know ; but there are other things beside light that will injure the plate as much. For example, it has been found that pressure upon the plate will hurt its surface and will often cause the plate to act at the 26 PHOTOGRAPHY FOR YOUNG PEOPLE place upon which pressure has been exerted as if light had touched it there. Then any moisture will injure it, even so little as may come from the touch of the fingers. Thirdly, a plate may be injured by high temperature. Con- sequently, if you desire to get good pictures, you must see that the plates remain in the dark, or in harmless light, that the surface is untouched, kept dry, and not heated. If these principles are borne in mind you will be able to get the plate into place within the camera and still keep it as sensitive as at first. - The next step in order is the placing of the plate so as to receive the image that is admitted into the camera. As to this, the main principles are few, but very important. You will remember that in talking about the forming of an image we have shown that the object of the lens is to bring the rays of images all to one plane (which in all ordinary cameras means all to the same flat surface), and that the surface is considered to be one truly parallel to the lens; that is, to a straight line joining its edges. Consequently the plate must be absolutely upright, and its right and left sides must be at the same distance from the front of the camera. If either the plate or the lens does not stand true, you will not get a clear image; if parts of the image are distinct, other parts are sure to be indistinct, because they will fall upon a portion of the plate at a different distance from the lens. Usually a camera is carefully made so as to bring about the right position of the plate, but if the camera gets out of order so that the plate no longer stands true with the lens, you cannot make good clear images until the fault be remedied, GENERAL PRINCIPLES OF THE PROCESS 27 The plate being correctly placed, we next have to admit the rays that form the image and allow them to strike the plate; but these rays must not be interfered with. If, for example, the plate is dusty, the rays will strike the particles of dust, and will not reach the plate beneath them. If there is dust floating in the camera, these little particles will come between rays and plate. If the lens is not clean, the rays will not get through without some interference. It will be found that all these necessities are remembered easiest by thinking of the one principle that there must be nothing to interfere with the striking of the rays upon the sensitive surface. It follows also from our purpose to have a clear image formed, that the plate, the lens, and the thing of which we are taking pictures, must all be motionless for as long as we need to let the rays act in making the picture, since motion will cause the forming of more than one image, and they will blur one another. To show that this is not a useless thing to remem- ber, it may be said that whenever you find that your developed plate contains a multiple of images — that is, for example, when you find two or three outlines for everything in your picture — you may know that the fault has been that the plate, camera, or object has moved. If this defect is not general, it is a proof that a part of what you are photographing has moved, While the camera and plate have been steady. The question of how long we shall allow the image to rest upon the plate brings up the whole question of exposure, which must be treated at a later time. Here we are really talking only of the most general rules, and we need say only that two things govern 28 PHOTOGRAPHY FOR YOUNG PEOPLE the length of time for the same plates and camera. These are the strength of the light, and the kind of light it is. To give a brief illustration: It will not do to rely upon what your eye tells you alone. For example, the light given by a brilliant red or yellow sunset is Very strong, so far as the eye can judge; but it is not a light that is strong to affect the plate; and the same thing to a less degree is true of such light as comes under the trees through the bright green leaves of spring- time. The eye finds such rays strong for seeing, but the plate finds them weak for taking pictures. Con- sequently it must be the brain and knowledge that de- cides how long the image is to rest on the plate, not the eye-judgment of clearness and light-strength. It follows from this that although it is a help to See what image is formed upon the ground-glass of a camera, or in the finder of a camera, it is no more than a help, as we shall explain more fully when treating of exposure. So soon as the exposure in the camera is finished, we must take the same care of the plate as before ex- posure is made, keeping it entirely from the things mentioned above as injuring its sensitive surface until we have changed it into a negative. And this change of a plate with a sensitive surface into a negative is the next process to be understood. To begin with, we must say that exactly what the light does to the plate nobody knows. We only know that it makes it ready for certain chemicals to act, and that on every part of the plate those chemicals will act more or less just in the same degree that the light has acted more or less. Where the light is strong the GENERAL PRINCIPLES OF THE PROCESS 29 chemicals act strongly ; where it is weak, weakly. Where the light has not touched at all the chemical has almost no action, unless after a very long time. Now, the general nature of the chemicals used to bring out the image on the plate is different from what most people suppose. One writer, in speaking of this subject in a photographic magazine, said, very truly, that the really active chemical was water; for the chemicals known as “developers ” act simply to Sep- arate water into the two gases of which it is composed. Even the simplest knowledge of chemistry teaches us that water is formed by the combining of two volumes of hydrogen with one of oxygen. When separated, these are gases ; when so united, they are a liquid. The developers are liquids that are eager to take up oxygen from water ; but this taking up of oxygen sets free the hydrogen, and hydrogen is the chemical that acts upon the sensitive substance of the plate, changing the compound of silver from one that is white to one that is dark wherever the light has made the compound of silver ready for the change; and the hydrogen acts just as strongly as the light has acted previously on the compound at different parts of the image. Thus, if a plate be held out in the open sunshine, and then put into the developer it will turn dark all over; for all the compound is ready to be changed by the hydrogen into dark silver. An unexposed plate put into the developer will remain unchanged in colour for some time, but after a long enough period there will be a slow action darkening the silver all over. This action, however, is so slight and so slow that ordinarily it need not be thought of. 30 PHOTOGRAPHY FOR YOUNG PEOPLE We have now a plate on the surface of which there remain after development two kinds of silver com- pounds, one dark and insensitive, the other light and still very sensitive to light. The next step is to take from the plate all of the compound that is not dark- ened. For this purpose the plate is put into another chemi- cal, which has the property of dissolving the sensitive part of the compounds of silver, while unable to dis- solve the other. When this chemical has acted, we have changed our sensitive plate into a non-sensitive negative. But this negative is still wet, still contains traces of the chemicals used, and therefore needs to be well cleaned and thoroughly dried. It is cleaned by washing, since water does not dissolve the darkened silver compound but does wash out the chemicals. Then by drying we get rid of the water and have left a negative ready for printing. We must now for a moment consider what a nega- tive is. In order to understand this clearly, let us suppose that we are to make a negative by photo- graphing the ace of clubs. When this is put up be- fore the camera and its image is carried by light rays through the lens and upon the sensitive plate, we shall have an image made up of white rays coming from all the surface of the card except the spot in the middle. From this there will be no light reflected, so the sensi- tive plate will all be affected by light except where rests the image of the spot in the centre of the card. Now we develop that plate. The developer will turn dark all the silver compound around the centre, but will not turn dark the compound where the spot rested. We then put the plate into a chemical that GENERAL PRINCIPLES OF THE PROCESS 31 removes the sensitive silver. When we take out the plate we shall find that the darkened silver remains on all the parts of the plate except the central spot where the undarkened silver has been dissolved out; and we shall then have a negative consisting of a plate darkened every where except in the centre — just the opposite of what we photographed, which was light everywhere except in the centre. Now negative means opposite; hence we see the reason for the Ila, Iſle. dº & Object Negative Print DIAGRAM VIII But no one in photographing a lady in a black dress would consider his work finished when he had pro- duced a negative showing a black-faced creature in a white dress; so the next step is to make from the negative a photograph or a “light-drawn picture.” For this purpose we have paper so prepared with a silver compound that is sensitive to light and so will turn dark where the light strikes it. Consequently, if we put a bit of this paper below our negative of the ace of clubs, after it has been left in the light for a while we shall find that the darkened silver on the negative has kept the light from darkening the paper below it, while the place where the silver compound 32 PHOTOGRAPHY FOR YOUNG PEOPLE has been removed, in the centre of the negative, lets the light rays through and blackens the paper. So by printing we reverse the negative, and get back to the correct image that was in the camera. The steps have been from the real object to an image like it ; then to a negative where light and shade are reversed; and then back again to a print like the image of the real object. Through all these processes there runs one very simple principle, namely, that we wish the light rays to act, to act in the right amount and direction, and without any interference. Consequently there is in the whole practice of photography nothing more im- portant than neatness and cleanliness. All the prin- ciples that have been explained in this chapter apply to the use of any kind of plates, any camera and lens, and to all the different methods of developing and printing. No matter how complicated directions for carrying out every process may seem to be, they will be readily understood if the principles here set forth, almost in primer language, are borne in mind. In truth, you will find that the thick books on photography are really no more than directions reasoned out from these few main principles, and put down as reminders to those who might forget them. When we shall come to give you practical advice about what sort of things are best for you to use in photography, they will be the things that will help you most to carry out these simple directions. It is a great mistake to think that the best camera is the one which looks most complicated, or that the best developers are those with the longest names or GENERAL PRINCIPLES OF THE PROCESS 33 the most complicated formulae. Neither should you make up your mind that because wise men have given years to the study of photography, the making of inventions, and the bringing out of new chemicals, that the subject is one which these simple principles will not enable you to understand. For example, years of study have gone to the mak- ing of lenses that will produce the best pictures under all sorts of conditions, but the whole result has simply been to make us able to throw upon the plate a clear image and one containing the right rays to act chemic. ally upon it. Even if eight pieces of glass, each made of different materials, and all ground to different shapes, are put together to form the lens, and so mounted as to be capable of many changes, the whole object is still the same — to bring the picture-making rays truly upon the sensitive surface — and by going carefully over the reasons for their making we shall readily be able to understand why one lens is better than another for this purpose. - Do not, therefore, lose sight of these first simple principles, but form the habit of reasoning about all things that seem complicated until you see for your- self how they come under these simple laws. We have given this general outline so that we may now take up matters more in detail and show you how and why the different things used in photography act to bring about the one simple result—a good negative and good prints from it. CHAPTER IV CHOOSING A CAMERA What the beginner needs—The question of expense — Advantages of Small camera – The 3}x4} size — Large photographs most im- pressive –The use of the ground-glass — Plates and films — Rolls, cut-films, and film-packs — The plate camera recommended for the learner-Using the ground-glass — Box cameras and fold- ing cameras — Meaning of “fixed focus ” — As to the possible exposure — Advantages of a shutter for various short exposures — The “finder,” in various forms — Other camera adjuncts — Focus, and what it is — Experiments that explain focusing. WHEN one comes to consider what sort of a camera to choose, it should be remembered that the beginner is entering a road which very soon will divide into a great many branches, and these will again divide un- til the map of Photography Land will be seen to in- clude a great many different destinations. The pur- pose of considering this is that we may make the right choice in the beginning and may select a camera that will teach us most about the art we are trying to practice. For this reason, it would not be good to buy the cheapest camera one could find, although there is no doubt that even for as low a price as one dollar a camera can be bought that will do excellent work. What should be selected by the beginner who wishes to learn is a camera that can be so changed as to do different kinds of work, so that he can make experi- ments and find out just what the camera does under different conditions. In the older books of photography there was a habit 34 CHOOSING A CAMERA 35 of advising beginners to choose first what was called a “view camera,” a rather large instrument meant to be used always on a tripod and without many of the devices needed in making quick exposures. The idea was that the beginner would become careless if he found his work made easy for him and was not forced to go about picture-making very slowly and carefully. But later authorities say, truly, that there is no sense in starting a beginner with an instrument different from what will be used later. The first consideration upon which the buying of a camera depends is how much you can afford to give for one, and in deciding this point it is not enough to look only at the price of the camera itself. It depends a great deal, also, on your own disposition. If one chooses to be economical in the use of plates and printing paper, a great deal need not be spent upon them; but it is very easy to waste them, and the be- ginner especially is likely, while the novelty of the pursuit tempts him, to take pictures recklessly and use up a great deal of material. For this reason, if saving is or ought to be an object to you, it will be best to commence with a moderately small camera, since the difference in expense between using a big one and a little one is mainly affected by the size of the plate you use. Also, with a small camera one can afford to make a great many experi- ments in order to learn the art, and may in making them feel that not too much has been spent. After you have learned to use material safely, it will be time enough to afford the larger camera, since you will have cut down the first expense of your materials very greatly. 36 PHOTOGRAPHY FOR YOUNG PEOPLE It is also wise in the beginning to choose one of the regular sizes of plates, so that you may be sure of finding supplies wherever you may be. For this rea- son probably the best size with which to begin is the so-called “quarter-plate" camera, which makes pic- tures 3}x4+ inches in size. This has the advantage of being a size used both in England and in America, and one that is always kept in stock by dealers not only in plates and films, but in all sorts of printing papers. A plate of this size is not too small for all sorts of uses and not large enough to be wasteful of material; for remember that the larger sizes require not only a larger camera, but larger plates, more chemicals, larger trays used in the dark room, larger printing- frames, larger papers, and so on. You save on all these items by using the smaller plate ; at the same time it is only fair to say that a photograph is impressive and striking directly in pro- portion to its size, especially if you take landscapes or interior views. But even here you may, whenever you like, make from the small negative larger prints at not very great cost, and yet this need not be done except in the case of a particularly good negative. The next question is what kind of camera in this size is best for the beginner. And as to this, cer- tainly he should have a camera in which he is able to see the image upon a ground-glass, otherwise he will do most of his work in the dark and by guess. And here, right at the beginning, we meet with the great question whether it is better to use plates or films; and this is a matter upon which you will be puzzled by receiving the most contrary advice — partly for the reason that there are a great many firms in the CHOOSING A CAMERA 37 photographic world deeply interested in your choice. There are a number who make plates, and a smaller number, perhaps, but an exceedingly powerful body of manufacturers, interested in making films and therefore in selling cameras to make the use of films easy. To go briefly into the matter, it should be said that there are advantages on each side. The users of plates find them cheaper; certainly quite as good, if not better, in results; easy to handle in developing and printing. But when you begin to collect nega- tives on glass you will find yourself in possession of bulky, breakable, and heavy glass plates, that, if kept, will become more and more of a nuisance. You need not keep them ; but, on the other hand, you will hate to destroy them. .. In favour of the films is their lightness, their dura- bility, and the fact that you may keep hundreds of them without trouble. If, however, you do your own work in developing and printing, you will find that the film is more troublesome to handle, always requires the use of glass in the printing frame, is a bother, if it be thin, from its tendency to curl up and to become stiff and unmanageable; for, in spite of what is advertised, you need not expect to find films that do not curl somewhat. All curl, more or less, and to be kept flat must be kept under pres- sure. There are, however, a number of things that cannot be done with plates in developing and so on, that can be done with films. Of course there is no variety in the choice of plates of glass, but when you consider the question of films there are three forms in which they may be bought, 38 PHOTOGRAPHY FOR YOUNG PEOPLE and certain varieties of these. You may buy films in the well known “rolls,” a long, coated strip that unrolls from one spool and is rolled up on another, while in the camera. It can be developed either in the strip or when cut up into its separate exposures. Then there are films cut to the plate-sizes and used just as plates are. Thirdly, there is the “film-pack,” a recent invention, where the films are packed into a sort of envelope in cut pieces so that they can be drawn from the front to back and exposed one by one. The cut-films first mentioned are exposed just exactly like plates. The roll-film may be cut apart and treated like plates, or may be developed in a strip, either by hand or in boxes that do away with the use of a dark room. A film-pack allows separate exposures and permits you to take out and develop separately ex- posures before you have finished the use of the whole pack; but works better if not opened till all are exposed. The only reason for considering this question at present is its bearing upon the choice of your camera ; and, as already stated, there are good reasons for choosing a camera in which you can use the ground- glass. It is possible to use films, and yet to focus on the ground-glass, but in order to do that, you will have to buy a special camera if you use the roll-film ; or if you use the film-pack it will have to be with a special device called the “film-pack adapter.” This device has a cover allowing you to remove the pack from your camera while you use the ground-glass. With plates or cut-films you use plate-holders, which also have a cover allowing them to be taken from the camera to permit the use of the ground-glass. There are, CHOOSING A CAMERA 39 besides, a number of “magazine cameras "using plates or cut-films, but not all of these permit use of the ground-glass. The conclusion is that a camera using ordinary plates in plate-holders, and using also a film-pack adapter, is probably the best for the beginner. With such a camera you can use the ground-glass for every exposure, if you like, may use either plates or films, and can thus have all the advantages of both. The only thing that you cannot do with such a camera is to use the roll-film — unless you buy for it a special “roll-holder,” which is quite expensive, and which is very little used at present. It must not be forgotten that this advice is addressed to the beginner, who is not yet certain just what sort of photographic work he means to do, and therefore ought to prepare himself for all kinds. The photog- rapher who has special work in view may find another kind of camera better adapted to it. For example, there are many good reasons why he might use a roll- film camera and develop all his exposures by means of the boxes and tanks used in the daylight. We do not mean to condemn this form in any way, but only to advise the beginner to choose as his first camera one that will teach him frequently to use the ground-glass before exposing. This “ground-glass” is a piece of glass fitted to the back of the camera so as to occupy when in use exactly the same place that the plate will occupy while being exposed. Consequently when the lens is open, the same image that is to be thrown on the plate is thrown upon the ground-glass and may be examined in order to see what you are going to take. The rough, or 40 |PHOTOGRAPHY FOR YOUNG PEOPLE ground side of the glass is toward the lens in the place where the sensitive film is to be. Like everything else about the camera, it should be kept scrupulously clean, since otherwise you cannot judge correctly all parts of the image received on it. The next question in regard to the camera is whether you shall choose what is known as a “box camera" or a “folding camera.” These two types are well known, and differ mainly in the fact that one has its Working parts concealed by the outward box, while the other opens to admit of the lens and its attach- ments being drawn out when focusing. Here again both forms have advantages, but perhaps the deciding points will be found in the question of your own character and the use you mean to make of the camera. If you are of a bashful temperament, you will often find that the folding camera will embarrass you, since before making an exposure it has to be opened and made ready for the exposure, which very much changes its appearance and shows all lookers-on that you are about to take a picture ; whereas the box camera looks the same in each case and attracts much less attention. Besides the box camera is all ready, or may be carried all ready for “snap-shots.” The name, “fixed focus,” is sometimes given to cameras, but it really means nothing more than that the lens is fastened in one place, so that the camera will photograph everything beyond a certain distance. There is no advantage in this over a camera with changeable focus, except that you have in using it no need to think about distance. The fixed-focus camera cannot do a great many things that are done by the others, while any camera may be made into a fixed- CEIOOSING A CAMERA 41 focus camera by simply fastening the lens at a certain place. Besides, the nodern folding cameras often have a device by which the lens can be instantly brought to the most generally useful focus — what would be its fixed focus. We have advised the use of the ground-glass because it enables one to know what image is coming through the lens; and in the same way we advise that a camera be selected that permits of giving a long or short time of exposure, and a time that you can measure. Usually for the amateur there is supplied in the cheaper cameras only two kinds of exposures, so-called “instantaneous ” and “time.” The instantaneous is made by pressing a button, causing the lens to open for a very short time, usually about one-twenty-fifth or one-fiftieth of a second. Time exposure may be, of course, made of any length beyond the time necessary to open and to close the shutter, since it will stay open until you close it. It is true that with these two kinds of exposure you can give any time you like beyond about one-half a second (except by using “stops,” as will appear later), but short of that, you can usually give only an ex- posure of one fixed length depending upon the quick- ness of action of the instantaneous shutter. But this is not enough. Most amateurs will wish to use the quick plates, and with these it is most important to be able to give various fractions of a second in exposing. Until we discuss this question fully, we can only say that on our general principle of knowing exactly what you are doing, you should be able to give more than one kind of very short exposure, and therefore we ad- vise strongly that you afford for your camera a price 42 PHOTOGRAPHY FOR YOUNG PEOPLE large enough to supply a shutter arranged for more than one short exposure. Until we can look more closely into the question of selecting the lens, it will be enough to say that in buying a camera with such a shutter as we have just spoken of, you will obtain a lens that will work rightly in connection with the shutter — which is all you need think of until you begin to do really expert work. It is worth knowing that the very expensive lenses are of little extra value to the amateur ; that sufficient clearness and practical accuracy can be obtained with moderate-priced lenses; and that in many kinds of pictures, such as portraits and landscapes, artistic effect may even be spoiled by a too precise clearness that shows every wrinkle, or every stick and stone. The high-priced lenses are generally “quicker,” re- quiring less exposure, so that with some of them you can take good snap-shots on dark days; but probably you will not need this rapidity very often. One adjunct of which we have merely spoken by name is the “finder.” This is a little camera, or box, which has but one purpose — to tell you, roughly, what is included in the image upon the ground-glass or upon the plate. The usual sort has in it a small lens, a piece of looking-glass, and a bit of ground-glass. The lens is so aimed as to give as near as possible the same image on a small scale that is given on a large scale by the lens of the camera. The looking-glass causes this image to appear right-side up, whereas the image on the ground-glass inside the camera is always upside down. But the finder is a tiny fixed-focus camera, and cannot tell you anything except the di- rection in which you have pointed your camera and CHOOSING A CAMERA 43 give you an idea of what you are taking. The image shown by the finder is always clear within certain limits of distance, and therefore does not tell you whether you have got your image on the ground-glass inside the camera (that is, on the plate), in the right focus. It is also reversed, because of the mirror used in it. Besides this form of finder, there are two others; one uses a lens in the top instead of the ground-glass, giving a slightly clearer and brighter image. The other is not a camera at all, being simply a sort of frame, either with or without glass, that shows you how much of the scene you are taking is in the image cast by your lens. The eye has to be at a fixed dis- tance from this last sort, and it acts on the same prin- ciple as the sights of a gun. There are other adjuncts of the camera, but they are all devoted to a few purposes, which may be briefly told as follows: Means for changing the distance be- tween lens and plate. Means for moving the lens up and down or right and left, so as to change the image thrown upon the plate. Means for turning the plate around so as to bring the image in a different position on the plate. Means for holding camera steady, and knowing when it is level. 44 PHOTOGRAPHY FOR YOUNG PEOPLE If we add to these the devices for making a longer or a shorter exposure, and for using more or less of the lens — that is, the shutter mechanism and the dia- phragm mechanism — we shall have covered the things used in making exposures. As to altering the distance between lens and plate, this covers the whole subject of focus. The word focus means “fireplace,” and came to be used in con- nection with the lens when the lens was used as a burning-glass. The plate is in focus when it is at the place where the rays coming through the lens from any given point outside the camera come to a point again inside of it. This place, in Diagram IV, is in- dicated by the line drawn through a, b and c. In the case of the burning-glass, the object whose image is cast by the glass is the sun. Before we discuss the theory of focusing, you will see the advantage of hav- ing a camera permitting the use of the ground-glass if you will make certain experiments in finding out the effect of changing the distance between your lens and the ground-glass. Perhaps the easiest way to do this is to light a lamp in a darkened room, and open your lens in order that the lamp may cast its image on the ground-glass. Then, as you slowly go nearer or move away, you will find that this image becomes less blurred, and finally becomes entirely clear. Now, leaving the camera at that point, you may move the lamp itself, and on examining the image again you will find that it is again blurred ; and in order to get a clear image you will have to move the camera again. If you have moved the lamp nearer to the camera, in order to restore the clearness of the image you will have to move the CHOOSING A CAMERA 45 camera further away. If you have increased the dis- tance between the camera and the lamp, you will have to bring the camera nearer to the lamp again. You will also notice that the size of the image changes ac- cording to the distance of the lamp from the lens. All these experiments should be made without changing the distance between the lens and the ground- glass. Next, having put the camera at such a distance as to give a clear image, move the lens further from the ground-glass, and you will find the image has blurred. In order to make the image clear again by moving the lamp, you must bring the lamp nearer. If you have brought your lens nearer to the ground- glass, you will have to put the lamp further off to get the clear image. DIAGRAM X These experiments are well worth making, and they will teach you the following rules: First, speaking generally, the greater the distance between lens and object, the nearer must the lens be to the ground-glass to give a clear image ; in Diagram X, above, you will see this shown : when the object is at M, the ground- glass must be at M ; when the object is at O, the ground-glass must be moved up to O. Second, there is a distance from the lens at which and beyond which 46 PHOTOGRAPHY FOR YOUNG PEOPLE all objects give a clear image; in the diagram this image is at F, and the object may be 100 feet or more away. Anything nearer than this will only give a clear image when the ground-glass is moved more or less away from the lens. Third, since your lens and ground-glass cannot be separated in the camera beyond a certain point (depending on the length of the box or bellows), you cannot make clear images of things nearer than a certain distance from any particular camera. Fourth, as you already know, but may well notice on the diagram for a clearer understanding, the farther away the object, the smaller the image of it on the ground-glass. To sum up these principles, we will say that with your lens there is a point beyond which all things are in focus when the lens is adjusted at a given point. Also, there is a limit to the nearness at which you can get clear images. This limit depends upon how far apart you can separate your lens and ground-glass. This simple experiment should make clear to you what is meant by the lens's “universal focus ”; the use of the long bellows in taking objects near to the lens; the need for moving the lens further from or nearer to the ground-glass to make a clear image; and also the fact that the size of the image on your ground- glass may be varied at will from a mere point to the image given when your lens is as far as possible from your ground-glass. CHAPTER W FIRST USE OF THE CAMERA Camera drill — The lens and shutter mechanism and diaphragms— The three kinds of exposures — The effect of the diaphragm — What is meant by “depth of focus ” — Length of exposure af- fected by sizes of opening in diaphragm —The “speed'’ of a lens depends on the opening — The first picture-taking — Loading plate-holders — Meaning of “dark room '' – Testing its safety — Ventilating — Precautions in loading — ‘‘Daylight loading” – Know what you are doing, and why — Device of a clever photog- rapher — Quick and slow plates — How light delays its own action — Advantages of slower plates — A common defect in plate- holders. SUPPOSING that you have such a camera as is recommended, you ought to make yourself very well acquainted with it before trying to use it for picture- taking. For this purpose it would be well to set aside an afternoon and to devote it to what is called by Bayley, the English photographer, “camera drill.” By this he means just such practice as is gone through by the young recruit with his rifle before he is allowed to load it. In the case of the recruit, this is done so that he may not do damage or waste ammunition when he actually fires the gun ; and in your case, it is so that you may not spoil plates when, with loaded camera, you try to take pictures. You should begin your camera drill by sitting down before a table that will support the camera and leave your hands free to try the working of the different parts. With the camera before you, go all over it, and be sure that you understand the purpose of every attachment. 47 48 PHOTOGRAPHY FOR YOUNG PEOPLE Most important portion of all, and therefore proba- bly a good thing to begin on, is the lens-and-shutter mechanism, including the diaphragms, or stops. An excellent way to understand this is to open the camera So that you can see the ground-glass, and then point your lens toward a window of the room so that the window will be reflected as a bright spot upon the glass. By looking at this bright spot you will see for yourself just what is the effect of the different ways of opening and closing the shutter. For example, you will probably find on your shutter front, the letters T, B, I. If, with shutter closed, you turn the little index pointer to the letter T (meaning “time ’’), and then touch the exposing lever, or squeeze the bulb (if there is a rubber bulb), you will see that the lens flies open, and that the image of the window appears on the ground-glass. A second pressure closes the shutter, and the image disappears. Next, turning the index to “B,” meaning “bulb,” touch the lever again, and you will find that this will open the shutter, but that it will stay open until you remove the pressure of the finger, or release the bulb. There remains the “instantaneous” mark, indicated by “I.” Turning the index to I, the exposing lever causes the shutter both to open and close again more or less quickly. These are the three kinds of exposure possible with the usual shutter. The third, or instantaneous, is varied in time. You will find a scale on the shutter marked with figures showing fractions of a second during which your shutter will remain open for in- stantaneous exposures. As the place of this device differs in different shutters, you will have to find it Courtesy of Eastman Kodak Co. Showing revolving back turned half-way to vertical position Courtesy of Eastman Kodak Co. Showing long bellows, fully extended CAMERA. Accessories Copyright, 1906, ºn 4. p phewan FIRST USE OF THE CAMERA 49 for yourself, or inquire which it is. Having found it, set the shutter successively for the different speeds, and by noticing the image on your ground-glass you will get an idea of how long each is. You may not be able to distinguish them very clearly, but until you come to do expert work the fractional differences will not be all-important. You will certainly know when you want the quickest possible exposure, or a slower one, and can distinguish between 9% or ; of a second and 3% or rºw. The usual figures are 1, 2, 5, 25, 50, 100. The first means one second, the next 9%, then comes #, 's, and so on — the bigger the number the smaller the fraction of a second. Also attached to your shutter-mechanism you will find some means for changing the lens-opening in size so as to let more or less light through your lens; that is, a larger or smaller number of rays or images. This device usually takes one of two forms. The simplest form is a slide with a round hole in it, to be placed in front of, between, or back of, the lenses, that will allow only a part of the central rays to pass. The second form is what is known as the “iris diaphragm,” and differs only in that it opens and closes circularly, like the iris of the human eye. In the first kind you are supplied with three or four openings (or “stops "), each one usually half the di- ameter of the next larger. The iris diaphragm, how- ever, can be made any size you choose from largest to smallest ; and the lever that moves it has an index scale attached showing the ordinary sizes. By changing the amount of light that passes through the lens you simply diminish the number of images that are brought to a single focus by the lens and thus 50 PHOTOGRAPHY FOR YOUNG PEOPLE bring about two results. Since your diaphragm cuts off light from the edges of the lens rather than its centre, and since the rays that come through the edges are the hardest to bring to a focus, at the same time that you diminish the number of images brought to a focus and so lessen the light-rays, you also use the very clearest ones and get rid of those hardest to bring to a true focus. Consequently, the things for you to remember in using the diaphragms are these : first, you lessen the amount of light admitted; second, you thereby make a longer ea posture necessary; third, you get a clearer image with less blurring ; fourth, you are working with what is really a smaller lens. Now as to this fourth, it has not yet been explained what the effect of working with a smaller lens is, and we prefer to take up that subject when we talk of lenses more in detail; but here we will simply say that experiment will show you that a small diaphragm al- lows more things to be in focus at the same time — that is, more things at different distances. For example, if you are taking a portrait of a friend standing in front of a grove of trees, when you use the largest diaphragm and so arrange your lens and ground-glass as to get a sharp image of the person you are photographing, by looking at the edges of the whole image on the ground-glass, you will see that the background is blurred, or “out of focus.” Now, if you leave the lens and ground-glass where they are, and simply change your diaphragm so as to give a smaller opening, you will find that the smaller the opening is made the more you bring both distant and nearer objects into focus at the same time that the FIRST USE OF THE CAMERA 51 person remains in focus. But the general lighting of your ground-glass is lessened, and longer exposure needed. So remember that by using the large diaphragm you get what is known as less “depth of focus.” That is, your main object will be in focus, but things only a little nearer or further away will be blurred. By using a smaller opening you will find greater “depth of focus,” or more things in focus, even though they are nearer or farther from your camera than the ob- ject on which you have focused sharply. (You must be careful not to confuse “depth of focus’ with “focal length,” which we explain later, for that is quite a different thing.) It is well worth while to experiment by focusing upon some brightly lighted scene, and then changing your diaphragm in order that you may become well acquainted with the effect in lessening the light, sharp- ening it, and changing the depth of focus. There is a simple rule, easily explained, by which you can understand just how much the change of open- ing by using diaphragms, or stops, affects the length of exposure. If you remember your school-books, you will under- stand that the amount of light admitted through a circular opening as compared with the light through another circular opening depends upon comparison of the squares of the diameters. Simply explained, this is only saying that the relation (or size compared to one another) of two circular openings is the same as the re- lation of two square openings. If we have a square two inches wide, or 2 x 2, it will admit four square inches of light. If we have a square 4 x 4, it will ad- 52 PHOTOGRAPHY FOR YOUNG PEOPLE mit stateen square inches of light; because doubling the sides doubles also the height. But the squares and the circles are related in the same way, so that if we double the diameter of a circle we shall admit through it four times as much light. Consequently the rule follows that a round stop, or diaphragm, which cuts down the width or diameter of the opening by half, requires an exposure four times as long. It may be well to say here that all clean and clear lenses ad- mit practically the same kind of light to the plate; if there is any difference it is too slight to count. Therefore the speed of a lens depends entirely upon how large an opening it admits of. A “rapid lens” is only one so perfectly made and shaped that it brings to a good focus nearly every ray (that is, photographic ray), that goes through it. A poor lens's action is likely to be worse and worse as you go from the centre toward the edges; consequently a poor lens to give a clear image must be used with a stop that shuts off the outer rays. A good lens, therefore, can be used with a wide opening exposing nearly all its surface; and so lenses are described as regards their working by telling the largest size of the opening at which they will give clear images. Since the largest stop or diaphragm provided for --------4 inches----------- ----2 inches--- +– DIAGRAM XI FIRST USE OF THE CAMERA 53 you to use with a given lens is the largest aperture at which your lens will work satisfactorily over the whole plate, it is an indication of how good a lens you have. The larger the opening in proportion to the diameter of the lens, the better and “quicker '' is the lens, simply because it uses more light-rays. Although it will be necessary to explain some other attachments that have to do with making exposures, we will leave these until we have to consider the special circumstances where those attachments are useful; and we will assume that you have made your- self familiar with the way of making an exposure, or, in other words, have completed your “camera drill” so that you are ready to load the camera and begin picture-taking, with some knowledge of what you are doing. Let us begin by loading your plate-holders with glass plates. This must, of course, be done in the “dark room,” and this will be a good place to explain what is meant by a dark room. From the general principles already set down you will understand that the purpose is to keep the new plates from any light that will act upon them. How sensitive plates are you may understand by thinking how faint a light is sufficient to impress itself on the plate during exposure in the camera. Examine a few photographs and you will see that they cover a wide range of lighting — possibly from the bright light of a White cloud to the shadowed side of a dark tree-trunk; and yet the plate is sensitive enough to record even the faint lightings in places that are almost quite dark. [n other words, the very faintest light leaves some “ace. So, to keep our new plates from spoiling, they 54 PHOTOGRAPHY FOR YOUNG PEOPLE must not receive the slightest touch of light that can act on them. The dark room, therefore, is a room from which all such light is kept out, and only the faint red and yellow rays (the non-photographic rays), are admitted to help us see what we are doing. By these we can see, even if they are too faint to affect the plate. The beginner is likely to fall into the error of think- ing a small window in his lamp, or in his dark room, is safer than a large one. This is not true. The light from the larger opening is no more dangerous to the plates than that from a tiny window. You may be led into this idea because we have just told you that increasing the size of the lens opening lets in a greater number of light rays. But the plain-glass window, you must remember, does not, like the lens, gather light rays into one spot; so a large glass does not increase the strength of the light, but merely ad- mits light over a greater space. As it fills the room fuller of light, it does leave fewer dark places in which one may lay the plate when not examin- ing it; but it is easy to screen the light from such parts as you wish to be in shadow. A large lamp with the flame turned low is safer than a small one with a big flame, as well as being much easier to work by. During the daylight it is almost impossible to find a place dark enough for handling new plates except when a room has been built for the purpose. But at night the problem is very much simpler. Unless there is bright moonlight, you can handle plates or develop safely in any room from which artificial light is abº sent; but it is wise to sit for a few moments in the { | FIRST USE OF THE CAMERA. 55 room, until your eyes become accustomed to the dark- ness, and then to examine whether there are any lights that shine in from outside, any reflections that bring in outer light, and so on. If there is no such outside light admitted, a room with shades drawn will be safe for your plates, especially if you do not leave them long exposed. If you wish to be very careful, you can test a room by leaving a plate face upward on a table in the dark, half of it being covered with black or red paper, the other half exposed to the ordi- nary light of the dark room. After developing such a plate, if you find the exposed side comes out darker than the other it is a proof that the room is not dark enough, or your developing light is not rightly guarded. But, having a room that is safe, you will light your dark-room lantern, which should consist of a lamp that gives light only through a piece of ruby glass, or, still better, through two panes of glass, one yellow and one ruby. The best lamps are so made. Here, again, you can profitably spend a little time in examining your lamp and seeing that there are no chinks from which light leaks to make spots of light on your table or on the ceiling. If such spots are found, the openings must be covered by gluing on bits of red paper or cloth. There is, however, no need to shut air out of your dark room. An oil lamp, especially if turned low, will tend to make the air close, and you will find it wise to have your room well ventilated. It is well, also, to have the room cool, especially when you come to developing. Having room and lamp safely prepared, open your 56 PHOTOGRAPHY FOR YOUNG PEOPLE box of plates by cutting around the lower edge, injur- ing the box no more than is necessary, since it will make an excellent receptacle for exposed plates or for unexposed plates you may not use right away, and afterward for finished negatives. But before un- covering the plates it is wise to do all that you can to make ready for the loading. Taking the covers from the plate-holders, place the covers and plate- holders at your right hand, put the box of plates at your left hand, and be sure you have in front of the lamp a clean place on which to work. It is also wise to have a soft brush, a clean cloth, or a little tuft of cotton, and with this to dust out the plate-holders and their covers before putting out all lights except your dark-room lamp. In other Words, make all the preparations you can in full light. Then, with your dark-room lamp turned somewhat down, but leaving yourself enough light to see what you are doing, open the box of plates (which will be found to consist of one box within another), put the first cover out of your way, then remove the second, and you will find the plates wrapped in black paper. Get one plate-holder ready so that you know where it is and where its covers are. Now raise the black paper and you will come upon the plates. These are always packed in couples, face to face ; so, on raising the paper, what is opposite you is the back of the first plate. It is slightly more shiny than the other side, and reflects the lantern light more clearly. It is assumed that you will already have discovered the workings of your plate-holder, which usually has a FIRST USE OF THE CAMERA 57 spring to press on one edge of the glass, and hold the plate firmly. Against this spring, or against the yielding inside edge of the plate-holder, which may conceal the spring, is put the plate; it is pressed into place gently and then of itself it is forced by the spring beneath a little ledge. The plate must not be touched on the sensitive side, and should be held, if possible, so that the direct light even of the lamp does not reach this side. Be careful, but don’t be scared. There are two ways of knowing which is the sensi- tive side. The back is plain glass and quite shiny, so that if you let it reflect the light from the lamp you will notice its brilliance. The other side is duller. Even if you cannot see, or are loading plate-holders in the dark, by just moistening the tip of your finger and trying at an extreme corner of the two sides, you will find that the sensitive side is a trifle sticky when wet. But, as we have already explained, the plates come in regular order, face to face, and by keeping count you will always know whether you are taking a plate out of the box back up or face up. The odd numbered plates are always back up. As soon as possible after putting the plate into the holder, insert the slide that covers the plate and adjust the little catch that keeps the slide from being again raised. While putting one plate in, it is well to leave all the rest shielded by the black paper, and, in general, even in the dark room, do not let any light whatever come to the plates if you can help it, never exposing more than one at a time. When you have loaded all your holders, give a last examination to see if all the slides are in, all 58 PHOTOGRAPHY FOR YOUNG PEOPLE plates covered, and so on, before you light the room again. Though the plates are so carefully wrapped, you will find it wise to dust off the surface of each one gently just before putting it into your holder, and also to dust the slide, since dust is every where. The more general principles apply to loading cameras of other kinds; that is, to get along with as little light as possible, even that of the lamp in the dark room. The reason is that even a slight effect upon the plate will prevent your getting clear blacks in your final print — which require, of course, almost perfectly clear glass in your negatives. As to the loading of cameras that take roll-films, modern cameras of this kind are usually loaded in day- light, and in this loading it is important to remember that by “daylight” is not necessarily meant the brightest light possible. It is much safer to get along with as little light as is convenient, avoiding bright sunshine or very brilliantly lighted rooms for fear that some little defect in your roll may let in a gleam of light. Be sure also to follow very carefully the direc- tions about getting your roll right-side up, and be sure that the film is going to run square and true between the rolls. If you happen to get a roll in wrongly, Wait until you can go to the dark room and begin over again; for, of course, “ daylight loading ” means only that it is safe to load in daylight when everything goes right. There are so many varieties of film and plate cameras that we can give no more than these general directions, but with each kind of film or camera you will find full directions given, or may get full ex- FIRST USE OF THE CAMERA 59 planations from dealers, who are only too glad to help the amateur by advice. Remember that it is to their interest that you should get good results, and do not be ashamed to ask about even the simplest matters. We have all been beginners, and all remain learners to the end. If you wish to be very methodical (and it is a most excellent plan) you can make a little list of the things it is necessary to do in loading your camera and ad- justing it for use, and then always refer to this list to make sure they are all done. But you really do not need to write out such a list, since you will find it printed, usually, in the directions that come with your camera. If you do not do this, you will find some- times you have loaded the camera while leaving the shutter open, thus spoiling the first plate ; or you have not set back to (l) the device for numbering the plates used in the magazine camera; or in some way have left a part unadjusted and so will spoil plates. Never be ashamed to take pains, as the best photog- raphers are those who are most careful of details. You will be amazed to find how many things can go wrong. After all, the best direction for all photographic Work is to use your brains to know what you are doing and why. As an illustration of this, one very clever worker suggested that if a man happened to be travelling and was in a hotel bedroom in the daylight, and yet had to load plate-holders, he could do this With perfect safety, in spite of the fact that he could neither block up the windows nor find a room or closet that was dark. The way in which this feat was accomplished was 60 PHOTOGRAPHY FOR YOUNG PEOPLE to thrust the box of plates and the plate-holders under the thick covers of his bed, then, working at arm's length with the bedcovers tight down, he was able to open the box, take out the plates, load the plate- holders, put in the covers, all without letting light reach the plates. Such a piece of ingenuity might do at a pinch, but it would require a very careful worker, and the bed- covering would have to be decidedly thick. It is not a method to be recommended, except as showing what may be done at a pinch. As to selecting plates, it will be enough at first to decide whether you are going to use slow or quick plates. This will depend upon what you mean to photograph. For snap-shots, you will want the quick plates; for landscapes or interiors or other subject in which there is time to make a long exposure, it is much wiser to get the slower plates. The difference between them mainly is in the thickness of their coat- ing and also in their chemical preparation. In the quick plates you must come closer to just the right time of exposure. The slow plates will give a good picture, even though you do not hit so closely the right time of exposing, for their thicker coating allows the action of the weaker rays to be impressed more deeply on the emulsion, and a little too much exposure given to the brighter rays does not so greatly matter because their action on the surface of the plate tends somewhat to protect the coating below from their further action. Thus the brightest rays do not produce a greater and greater effect in proportion to the exposure, but their action is slower and slower, leaving time for the less bright rays to “catch up,” FIRST USE OF THE CAMERA 61 as it were. We shall explain this more clearly later. The beginner will find it best to select a plate rec- ommended “for general work,” and to stick to that exclusively at first ; for until he becomes an expert, he will not have occasion to photograph unusual sub- jects, such as frost-markings, lace, or flowers, or waves or athletes in motion. You need remember now only that if you can give the right exposure for the slower plate you will be more apt to get good pictures than if you used the Quick plates, since the quick plates require you to be very exact in giving the right time. The quickness and slowness is denoted by names and numbers, the higher number meaning the quicker plate. In films, since these are prepared for general use, they are usually of one quickness, fitting them especially for snap-shots or instantaneous exposures. It is there- fore important to get the exposure of films right. Very slow plates are made for special purposes, such as copying other pictures, making transparencies, or lantern slides, and so on. It really would be wise for you to commence with not the quickest plates, though you will very soon begin to use these. And, indeed, there are but few subjects requiring extreme quickness, and those require also a “quick” lens — one with a wide opening — a good shutter and much skill in mak- ing exposures. There are many cases in which you will get richer, better negatives from the slower plates by giving them enough time. The slower plates also are less liable to be spoiled in the developing and other processes. Of course the taking of pictures in the flash of an 62 PHOTOGRAPHY FOR YOUNG PEOPLE eyelid is very wonderful, but, after all, the most satisfactory pictures are those that make one say “How beautiful!” rather than “How remarkable *; and you are really more likely to get the good pictures when you can take time enough to think of what you are taking. The difference between the so-called “quick” plates and those of the next degree of rapidity is less than the beginner might suppose. Before making your exposure, one caution is neces- sary : if you should take apart the plate-holder, you would find that there is inside a sort of little shutter — a strip moved by springs — which closes the slit through which the cover is withdrawn. This shutter, or strip, rests against the cover of the plate-holder as you withdraw it, and should close as soon as the cover is drawn completely out. If, now, you draw the cover out one corner first, this little shutter will Open and light will get in at the top of the holder, slightly affecting the plate at the upper edge. The same thing will happen if in putting back the cover you put one corner in first, instead of putting it in squarely. For this reason it is well to be sure that the cover is drawn out and put in smoothly and squarely, and it is also wise not to let the sunshine or a strong light fall upon the upper part of the plate-holder where it projects from the camera. If you wish to be especially care- ful you may put a cloth over the camera while you withdraw the slide, or COVer. This trouble with plate-holders is especially common with the cheaper grade, and with old plate-holders. You may know that this defect exists when you find the upper edge of your negatives spoiled by bands or portions of darkening while the rest of the neg. FIRST USE OF THE CAMERA 63 ative is clear and good. You may see where the light leaks in by withdrawing the cover as you look, toward the light, through the slit where the cover enters. CHAPTER WI LEARNING ABOUT EXPOSURES What to seek from your early exposures — The best first subjects — Making the camera ready — Things to be careful about — The most important question in photography — Length of exposure — Exposure meters — Things that affect exposure — Season of the year — Time of day — Weather — Plate-speed — Lens opening— Quality of subject — Distance from camera — How the latitude of the plate helps — A rule of thumb guide — Diaphragms — An experimental method — Exposure less difficult than it sounds — Development does little to aid poor exposure — The use of ready- made developers at first. WE have now supposed you to have gone as far as choosing a camera, learning about its more important parts, loading it with plates, and being ready to go forth into the broad world and take pictures. But we wish to warn you, at first, against going too fast. Do not be anxious to secure any result from your first few exposures except experience. It may be that you will hit upon a masterpiece of the photo- graphic art, but the odds are decidedly against it : and you will be likely to arrive at the masterpiece all the sooner if you look upon the first box of plates, at the very least, as being a means of teaching yourself what they will do. Set before yourself, therefore, the purpose of pro- ducing a good clear photograph of whatever you at: tempt, and put aside for the present all ideas of artistic results, interesting or picturesque composition, and other things that will come later. 64 LEARNING ABOUT EXPOSURES 65 If you wish to make sure that the first plate shall be a success, it will be best for you to make an ex- posure upon a distant landscape; for there is nothing in the world so easy to take. In the first place, by taking such a picture you get rid of all troubles about right focusing. You will find on your camera a focusing scale with a pointer that moves along it showing where the lens is to be placed in order to take objects at different distances in feet. If there are two sets of numbers, one is feet and the other meters. The highest number they give you is the place where you ought to put the pointer when you are taking a distant landscape. Your experiment in focusing upon a lighted lamp will have shown you already that be- yond a certain distance from the camera all objects are in true focus, or so near it that the eye cannot tell the difference. Before putting in the plate-holder, set your lens at this extreme distance, and move the camera in such a Way as to form upon the ground-glass any image that pleases your fancy. When you have selected the right thing to take, close your lens, insert the plate-holder, being sure that it goes in rightly until it is chock up in place. Set your shutter, and then draw out the plate-holder cover, leaving the plate ready for ex- posure. Remembering what has been said about the need of keeping the camera motionless, you will either have set it up upon a firmly planted tripod, all parts of Which are set securely, or will have selected some steady base on which to rest your camera. Having done so, be careful that you do not spoil your picture by setting the camera so that the picture is crooked 66 PHOTOGRAPHY FOR YOUNG PEOPLE upon the plate, or by striking the camera or the tripod in moving about it so as to shake your plate just at the moment of exposure. Unless you are careful of these things, you will occasionally do them. You have no idea how easy it is to catch your toe under One leg of the camera and upset the whole apparatus. The same cautions apply even more to snap-shot ex- posures, where the camera is in the hands or against the body. In this case even the breath must be held at the instant of exposure and the camera held as steadily as possible. It seems almost childish to insist upon things so evident, but the plates and exposures ruined by these very elementary errors are numbered by the thou- sands. If we could each imagine that plates were worth five dollars apiece, there would be ever so many fewer spoiled plates in the world ; and even though they are cheap, you should take pride in workman- like success. - Now you are ready to let the image be admitted to the sensitive plate, and here comes the most difficult question in photography — that of how much exposure to give. If you are using quick plates, and the light is strong, say such as that on a sunshiny day in sum- mer, the exposure will be a very small fraction of a second. It may be as small as the hundredth part, or even less with a quicker lens; that is, with one that admits of a wider opening without blurring some part of the image. We must lay down here the general principles that regulate exposure, and perhaps the quickest Way to get at this is to tell what “exposure meters” are. There are for sale various devices for measuring ex- IEARNING ABOUT EXPOSURES 67 posures, and by getting an idea of these you will see how many things have to be considered in order to decide just how long to expose a plate in a camera. These meters often contain a way of exposing to the light a little bit of sensitive paper, and from this as a starting-point they work out the problem of exposing. This problem involves a number of things. First, the time of the year. Though the light of the sun does not vary, the direction in which it comes to us does vary. In the northern hemisphere, in which we live, the sun, in summer, though farther away, is highest in the sky, that is, more directly overhead at O SUru. Surn. at Ito On. afnoon, Summer Winter DIAGRAM XII noon. In winter, it is further south ; that is, if its course were traced out as a line in the sky, there would be drawn for midsummer a semi-circular arch from east to west, going almost directly overhead. In winter there would be another similar arch, all of which would lie southward of the first. Now when the sunlight comes to us slanting, it travels through more air, and is weaker. So in winter 68 PHOTOGRAPHY FOR YOUNG PEOPLE exposures need to be longer than in summer. If you imagine the sun to be travelling on its course, either in winter or summer, you will see that it comes most directly to us at noon, and comes through thicker lay- ers of air both morning and evening. When just above the horizon, either east or west, it is at its worst for photography. At noon it is at its best so far as brightness is concerned and chemical action; (though We shall see later that the absence of long shadows in a picture taken at noon is considered by good pho- tographers a drawback). So we are compelled to con- sider time of year and time of day. Next we must bear in mind the speed of the plate We are using, and the size of the opening for light through the lens, - all these things, whatever the subject we are taking. Next we have to think of how much light the sub- ject gives off and the colour of that light. Last, we have to think of the question of distance from the camera. The further away the object is, the more the light will be interfered with by the air and the hazi- ness it produces, especially when containing dust or moisture. The effect of this is to soften or lighten distant shadows, producing the same effect as if there were more light on the object. This effect is not im- portant for distances less than perhaps a hundred feet from the camera, but beyond that it tends to shorten the exposure. Experts say that for very distant Ob- jects the exposure is perhaps lessened by one-tenth, for this reason. The further away an object is, also, the more light-rays will be reflected so as to enter the camera; the nearer it is to the lens, the less light it will reflect and the duller image it will give. Photograph by Dr. A. R. Benedict Courtesy ºf Photo-Era Magazine -- - - “THE MAN on THE I:ox * A good study in composition. The picture would lose much of its effect iſ the puddles in the foreground, catching the light, were absent, or if the cabman's body did not follow the lines of the trees overhead. - LEARNING ABOUT EXPOSURES 69 As to colour, we have already spoken. This whole matter turns on how many of the active rays, those toward the violet end of the spectrum, are sent into the camera, and how many of the less active rays, those toward the red end. All these things are laid down in the directions that come with the exposure meter. You have to set the little instrument for time of year, time of day, character of weather, whether bright or dull, nature of object taken, and its distance from the camera. Complicated as this sounds, fortunately we are not compelled to get an answer to the problem that would satisfy a college professor examining you in your knowledge of photography. The fact that the plates have a certain latitude comes to our assistance. This means that they will give good results even if you do not always work out the problem exactly to a small fraction of a second. Perhaps a good rule-of-thumb guide may be found in the fact that the ordinary film such as is supplied for cameras is sensitive enough to take good clear pictures on a bright day in something like one-fiftieth of a second, with a lens of fairly good quality working with an opening about one-eighth of the lens's focal distance (designated on the diaphragm indicator by the figure 8). It is such a lens as this that is supplied with most hand cameras of fairly good quality. This gives a sort of rule by which to estimate our exposures. Under very favourable conditions, you can take good pictures outdoors by means of instantaneous ex- posures of from one one-hundredth to one-fifteenth of a second. As to the use of diaphragms, you have already read 70 PHOTOGRAPHY FOR YOUNG PEOPLE the rule that we must multiply by four whenever we diminish the diameter of the opening one-half. As to subject, before we discuss this very closely, it will be enough to say that when you come to take indoor pic- tures near a Window, with the same sort of a camera that we have described, you will find yourself able to get good results by an exposure under favourable con- ditions, good light, and so on, of three to five seconds. In the middle of a dark room you might have to in- crease this exposure to thirty seconds. All this, you may well say, is vague ; but it is to know something more definite about these conditions that you are asked to make use of your first box of plates. There has been recommended recently in the photo- graphic magazines a very good method of judging the necessary amount of exposure by a practical trial. This is done by making several exposures on one plate, first withdrawing the cover slide of your plate holder only about one-fourth the distance, so as to expose a quarter of the plate only. To this you give an ex- posure of one-fiftieth of a second. Then, withdrawing the cover another quarter, or half way out, give a second exposure of the same length. Tepeat this for the two remaining quarters, being very careful not to stir the camera any more than you can help, and the result will be that you will have exposed a plate in four different strips along its length. The first strip will have been exposed for four-fiftieths of a second, the next for three-fiftieths of a second, the third for two- fiftieths of a second, and the last quarter for one- fiftieth of a second. This is supposed to be for such a distant landscape view as has been recommended for LEARNING ABOUT EXPOSURES 71 making your first exposure. When you come to develop this plate you will see experimentally for your- self what effect is produced by four exposures of dif- ferent lengths, the longest being four times as long as the shortest. This same experiment may of course be applied, and should be applied, to making time-exposures of greater length. In this case you might make the exposures four, three, two, and one seconds. If this is done upon a fairly lighted subject, not in full sunshine outdoors, you will probably find that your longest exposure is too long. Indeed, in a bright light they may all be too long; but on a grey day one of them is apt to be right, or nearly right, enough so that you can see which is nearest correct. We shall give you, in a chapter devoted to tables and formulae, some of the guides that have been drawn up by experts to help you to measure the strength of light and to judge of the subjects requir- ing longer and shorter exposures. By turning to these you will obtain an idea of these elements which change the amount of exposure ; but you may take comfort in the fact that every photographer very soon learns some knack at guessing correct exposures, or near enough to them for all practical purposes. Ex- posure meters are, however, very useful; even the simplest are useful as guides, and cost very little, con- sisting only of a card of paper or celluloid with sliders or disks allowing you to adjust them to suit the condi- tions of light and subject, lens and plate. You have been warned of all the difficulties of judg- ing an exposure, so that you may see it is a subject well worth your special attention; but we must repeat 72 PHOTOGRAPHY FOR YOUNG PEOPLE that it is not necessary to make a bogey of it. In actual practice, many of your pictures will be taken in the open air and in good light, with plates or films that give you a margin in judging the length of ex- posure; and you will realize that in taking indoor pic- tures the time required is increased from a fraction of a second perhaps to three or four seconds, or more in places not well lighted. For taking snap-shots in the winter months, when the light is poorest, you will need a diaphragm of large opening. If we add to these few general directions the fact that it is better to err on the side of giving plenty of time, and to expose for the shadows rather than the lights, we shall have told you all that is necessary for you to learn at the beginning. It used to be said that even if an exposure was not right, the error could be corrected when the plate was developed, by changing the proportions of different ingredients in the developer, or by developing for a longer or a shorter time, and so on. But the latest theories do not permit us to take this view. Even if developing can make some difference in plates, it is mainly a difference in the time required to make prints from them, and not a difference in the quality of the print produced — that is, in the relation of the light and shade. Consequently it is of the utmost importance to make your exposures with as much judgment as you can possibly give to them, and so we recommend un- qualifiedly the use of the exposure meter, at least in the beginning and until you have trained yourself to judge with some correctness about the conditions and to bear them all in mind. The expense is small; the LEARNING ABOUT EXPOSURES 73 benefit to your skill is very great, and the saving in plates will be considerable. Let us now suppose that after trying a landscape or two you have made several varying exposures to the best of your ability, and are ready to develop them. We do not need to repeat what we have already said in regard to the dark room, as to being sure that the light is safe and that the room is made as comfortable for you as possible. Developing is a matter that needs all one's careful attention, and you should not be distracted by being uncomfortable, by stumbling over furniture, by upsetting trays, by stopping to look for things in the dark. Again, you must begin by ar- ranging in convenient and handy places whatever you are going to use in the process. Ten or fifteen minutes is wisely expended in thinking over carefully just what you are going to do from beginning to end, and preparing everything ready to hand so that it may be picked up as soon as needed and in the order needed. Since it is the intention here to describe the most usual way of proceeding, we will not as yet take up the question of which developer you are to use; that will be treated later, and here we shall assume that you have the developer made ready by dissolving some of the powders already measured, and standing in a graduate, or measuring-glass, from which it is to be poured. - You should use the developing powders or mixed liquid developers as sold ready for use; for this is ad- visable at first. There is plenty to learn in photog- raphy without trying to learn all parts of the proc- esses at once. Therefore, until you have become used to the general way of taking pictures and making 74 PHOTOGRAPHY FOR YOUNG PEOPLE negatives you will profit by getting materials all ready-made, and giving your attention to learning what they will do and how they act. So follow directions, and leave the “whys” of chemistry until later. CHAPTER VII FIRST STEPS IN DEVELOPING The necessities — Taking out the plate — Pouring on the developer — First signs of development — Burton on the magic of developing —Watching development — What takes place — Keeping the de- veloper at right temperature — When development is complete — Fixing the plate — How long to leave it in the hypo — The reason for washing after fixing —Thorough washing necessary — Drying —Warnishing especially valuable negatives. THE real necessities of developing are: three trays, at the least ; one for the developer, which should stand directly in front of you and where it can re- ceive the light of the lantern. Next to that, right or left, as you find it convenient, have a tray of cold water; beyond that, your tray of hypo. A fourth tray, for washing, will make your work easier. Be- sides the trays, you will find it well to have something to lift the plates from the different trays. For this purpose we think there is nothing better than a clean new stick, sharpened to a broad, flat end. You also should have a piece of cloth to serve as a towel, but one that you will not mind spoiling with chemicals; a large, clean rag is just the thing. Now, with the lamp turned pretty well down, but still high enough to give you a fair amount of light, and with your glass of developer standing close to your developing tray where you can pick it up quickly without knocking it over, you are ready to begin. Holding your plate-holder vertical in such a way 75 76 PHOTOGRAPHY FOR YOUNG PEOPLE that the plate you are to develop is toward you and away from the light, draw out the cover promptly, press down the little spring that keeps the plate in place, letting the plate be tipped a little forward so that you can take it by the edges but keeping it close to your body so it will not fall out. It is then wise to dust off the surface very gently with a soft, dry brush of camel's-hair or with a bit of cotton. Put it into the developing tray, back downward, without delay, and then raising the tray and plate in your left hand, pour the developer over the plate in the way recom- mended by Bayley, the English photographer; that is, letting it flow without splashing, but very quickly, from one corner of the plate in a little wave over the whole surface. This will prevent little bubbles of air being caught below the developer and making spots, and will avoid streaks caused by wetting the plate unevenly. As soon as the plate is seen to be covered and free from air bubbles, put a piece of pasteboard over the tray so that while the plate is still sensitive it may be as nearly in the dark as possible. If your plate has been exposed somewhere near the right time, it will, after a few seconds, begin to show signs of develop- ment, and by raising the pasteboard now and then for an instant, you may keep on the watch for these signs. From what has been said already you know that the effect of the exposure has been to make some un- known change in the coating of the plate, preparing it to be acted on by the developer; and that this change has been greater or less according to the dif- ferent amounts of light that have been thrown by the FIRST STEPS IN DEVELOPING 77 lens upon different parts of its surface. Wherever the brightest light has rested, the action of the developer will begin earliest : the plate will be seen to darken at this point. One of the pioneers of modern photography, the Englishman, Burton, says in regard to developing: “Now, if everything has been rightly done, will be- gin one of the most wonderful of the phenomena of science or nature which man has been given the power to control, a phenomenon which is always new and always beautiful — the development of the latent image. Let the beginner watch it closely. The plate has no indication of having been acted upon at all, before the developer was poured over it. After perhaps twenty or thirty seconds there is a slight darkening of some part . . . the brighter parts of the landscape have become visible in negative. Now is the time when you can tell whether the exposure has been correct. If it has been, the development will progress with beautiful regu- larity.” We would by all means advise you to see a correctly exposed plate developed by some one else who is familiar with the process before attempting it for yourself. But if you have taken the advice given, to begin by making an exposure upon a distant land- scape, and have given anywhere near the correct ex- posure, you will probably have no difficulty in devel- oping your first plate. As you watch the process you will see the brightest parts appear first and these will be followed by others in regular order until every part of the plate is dark- ened except those parts where the light has hardly 78 PHOTOGRAPHY FOR YOUNG PEOPLE acted at all — that is, those parts of the landscape which looked very, very dark to the eye. The next question that will come up for your de- cision is when to stop the development by taking the plate out of the developer. A photographic dealer suggested to the writer that amateurs should be carefully informed that the devel- oping solution will not “eat away the plate ’” — which, he says, is a very prevalent idea. You need not be afraid of this, as the effect of the developer is only to darken the silver compound where light has acted, and in proportion as it has acted. It is true that the Solution does soak into and thus soften the emulsion ; if it did n’t, it could not reach the silver compound in it, but the emulsion will not dissolve if your solution is not too warm. It certainly should not be warmer than sixty-five degrees, and may be as cold as sixty degrees. This need not worry you, however, for it really is only the temperature of a rather cool room, not hot enough to make you uncomfortable, nor cold enough to make you chilly. In summer, you may easily keep your developer at the right temperature by partly filling a rubber bag (hot-water bag) with cold water, and resting your tray upon this. Or you may rest your developing tray in an outer one in which there is a little water kept cool by a bit of ice. The hot-water bag filled with warm water could also be used in winter if you have to develop in a very cold I’OOIſl. As to judging when the plate has been sufficiently developed, that is another of the things best learned by experience; but, in general, you should keep it in the developer until all of the detail can be seen fairly TIRST STEPS IN DEVELOPING 79 well when the developed plate is held up between your eye and the dark-room lantern. By the time the de- velopment is completed, too, you will be able to see at least the dark portions of the image by looking at the reverse side of the plate. It is well to develop pretty thoroughly, since the effect of a long development, if not extreme, is mainly to make the plate print a little more slowly, while under-development will leave cer- tain portions of the image unfinished, not brought out — a much more serious fault. The methods of developing by time and temperature alone, without watching, will be given at another place. As soon as the image has appeared over the whole plate, you may safely turn up your red light flame so as to be able to see very clearly, for the plate has lost a great deal of its sensitiveness and does n’t need nearly so much protection from red light. - As soon as you have decided the plate to be rightly developed, place it in a tray of clear water for a mo- ment, so as to rinse the developer from it, and then put it promptly into the hypo tray. Of course in all cases your plate should be face upward so that noth- ing will injure its surface, and nothing but the solu- tion should touch the surface, since when wet it is very easily injured. For this reason, if you use the sticks for lifting, do it with the utmost caution to prevent their touching the face of the plate. The only object in using them is not to put the fingers too much into the liquids. - What you have done so far is to change that portion of the silver compound which has been affected by the light into metallic silver, which, when finally divided, 80 PHOTOGRAPHY FOR YOUNG PEOPLE is dark, and which is insoluble in water or hypo. The next step, the one which you began by putting your plate in the hypo tray, is to melt away the compound that has not been made insoluble by light and devel- oper compounds. Consequently you leave the plate in the hypo until this white compound, or part that is unaffected, completely disappears, and your plate looks dark all over. But even then the hypo has not finished its work. It has dissolved the undarkened silver, but it has changed it into another chemical compound that also must be dis- solved out, even though it is an invisible one. Conse- quently, to get rid of this, you must leave the plate in the hypo nearly as long again. After coming from the hypo bath, the plate has ceased to be sensitive to light, and so far as that plate is concerned, you are at liberty to examine it freely by any artificial light, or even by daylight. But although our plate is now safe from light, it is not yet clear of chemicals that will do it injury. It now consists of a wet compound containing the me- tallic silver that makes the negative, but also contain- ing the hypo solution, which, if left in the negative, would crystallize when dry, and ruin it. Consequently there must follow a thorough washing, either in run- ning water or in successive baths, until all the hypo is drained out. This process is usually underdone, but if your nega- tive is to last, it must be done thoroughly, and “thor- oughly " means until you are tired to death of it. The makers of the kodak film, for example, recommend that their films be soaked in five changes of water, five minutes each time, occasionally moving the film TIRST STEPS IN DEVELOPING 81 about. Or they recommend two such changes, fol- lowed by an hour in gently running water. The plate will not require quite so long a washing, but you will be very glad if you always err on the side of thorough- ness. Otherwise, some time in the future when you take up a favourite negative you will find it stained and ruined, and will recall sadly Whittier's lines about what “might have been.” After the washing, comes the drying. You may safely, if carefully, wipe all moisture from the back of the plate, but avoid the tragedy of making a mistake as to which is the back. By looking along the edges you will soon see the difference between the smooth edge of the glass side and the slightly puffy, irregular edge of the film side. The plate should not be set up to dry so that it will touch anything else. If it is put with others in the drying-rack, there should be a good distance between them — certainly two or three inches, at least — otherwise your plates will dry too slowly. A quick drying is important, since in some cases skilled photographers tell us that the clearness and sharpness of the image suffers by too prolonged a dry- ing. But remember that the drying must not be helped by putting the plate in warm air or in the sun- shine, for fear of melting the softened film — which is easily done. A little point worth remembering is the necessity of removing from the lowest corner of the plate the drop of water that forms there when it is put up to dry. You can remove this by a touch of a soft cloth or a bit of cotton, or even with the finger, and your plate will dry faster. Until thoroughly dry, do not think of attempting to print from the negative, for 82 EPHOTOGRAPEHY FOR YOUNG PEOPLE fear that the printing-out paper and the negative will stick together in the frame. We do not know anything more important to insist upon in all this question of developing than care in not letting anything touch the film and injure the negative. It is so easy, and so irremediable, to dam- age the wet surface. Once the negative is dry, it is not so easily hurt. A last process to insure the keeping of the negative is to warnish it. This is done by gently warming the dried plate, and pouring the warnishing liquid Smoothly over the level surface, and then draining the surplus off at one corner into the bottle again. It is, how- ever, not necessary to varnish plates except as an extra precaution to preserve an unusually valuable negative. If negatives are properly kept in paper or in boxes, they will be safe enough. CHAPTER VIII MAKING A PRINT Judging your negative — The true object to get good prints — print- ing-out paper and developing paper — The printing-frame— Errors in using the printing-frame — Printing by diffused light — Toning the print — Washing before toning — Toning with gold — Fixing with hypo — Cleanliness essential — Trimming the prints—Mounting — Developing papers — The strength of light in printing — How to test it — Varieties of developing papers — Brush-development—Local development. WHEN your plate is thoroughly dry, and not until then, will you know for certain the value of the result you have reached, for the only test of a negative is the making of a print from it; and this for the reason that the transparency of the plate when held up to the light does not give you an entirely correct idea of what sort of a print can be made from it. It does, however, tell you a great deal about the relation of lights and shades in your negative — whether there is a good gradation from the darkest to the lightest, or whether they are too much alike all through. Even if your plate, however, should not be very transparent to your eye, if, in other words, although it has a good breadth of values (which means a great many different darker and lighter shades, shown in the right relation to one another) it may yet give you an excellent print provided it be left long enough ex- posed to the light in the printing-frame. And in the same way, even if your plate be what is called “thin,” 83 84 BHOTOGRAPHY FOR YOUNG PEOPLE that is, very transparent in general, yet if there is the same range in value, the same differences in light and shade, you will get a good print from the nega- tive provided you do not leave it printing too long. This is another way of saying that what we must try to get in our exposure and developing is true relation in light and shade, whether the whole plate be dense or thin — that is, whether it needs to be printed only a short time, or is a slow printer. In examining your negative, therefore, the first thing is to compare its lightest with its darkest parts, and to see whether there is something of the same difference between them that there was in the scene you have photographed. If you have succeeded in keeping the relation true, if your blacks and whites are not too near together or too far apart in value, you may be sure that you have made a good negative, and with care you will be able to make a good print from it. It is a wise maxim in photography that the object of the whole process from the beginning is to get good prints, and all the rest is but a means to this end. Until you have made a good print, you have not done what you set out to do. As to printing methods, we shall consider in this general going over the subject only two main methods of printing from the negative. These two consist really in using two kinds of paper. One sort is known as “printing-out” paper (or as the English call it, “P. O. P.”) for the reason that by exposing a piece of the paper to light when it is covered by the negative we secure a print at once. The other method uses what is known as “developing paper” (such as MAKING A PRINT 85 bromide, Velox, Cyko, and so on). In this, although there is a printing process, the paper is developed by a process of regular developing, exactly as if you had exposed a plate, and until development is finished you do not see the print in anything like the state it is to reach. - The first of these methods is the older one, and consists in using paper so coated that under the nega- tive it is exposed to the light and printed until the image is as dark or darker than it is meant finally to be. The apparatus used for this purpose is known as a printing-frame. It consists of a frame that holds the negative, film side inward, so that the paper can be placed with its glossy side toward the film, and then covered by means of a hinged back. The whole object of the frame is to keep the paper and film firmly and immovably together while printing, and yet allow you to examine a part of the print to see whether it is printed enough. The best printing-frames are those which are closely fitted to the size of the negative you are using and allow the widest surface of the negative to be reached by the light. The front of the frame should be thick enough to be rigid, but should cast as little shadow as possible on the negative. The back should also be hinged firmly so as not to move from side to side, the pieces under which the springs go should be kept tightly screwed into place, and the springs should be strong enough to exert quite a pressure upon the paper but yet to turn easily when the movable part of the back is being opened to look at the print. The best backs are those which are cut in two unequal pieces so that the larger one will allow you to see a 86 PHOTOGRAPHY FOR YOUNG PEOPLE large part of the print. Sometimes you will find on them a little numbered wheel. This is merely a means by which the printer keeps account of the number of prints he has taken from that frame. In setting up your frame for printing be careful to turn it squarely toward the light so that the front of the frame shall not by means of its edges cast little shadows, shadows that will keep part of the negative from printing. The mistakes one is apt to make in printing are: allowing the negative to fall, putting the paper in with the back against the negative, or crooked, setting the frame where a shadow will fall across it, either at the time it is set out or later (because the earth is moving), unfastening both ends of the back at once before you are certain the printing is finished, and (for a beginner) forgetting that you are making a print, and so leaving it too long. You may not think you are apt to forget having put a printing-frame in the light, but if you are busy at other things you will often find that the print is entirely forgotten, while you are about something else. Skilled photographers will tell you that it is always best to print by means of diffused light — that is, not in the direct rays of the sun. This is undoubtedly sound advice, although if you always take it you will be more docile and patient than most amateurs. The reason the advice is good is that the printing in direct sunshine is very apt to be harsh, and if there are any slight defects in the glass, or there is dust or any impurity on the back of the negative, it will seriously affect the print. Diffused light will give softer prints and defects will be less apt to show. The usual way of avoiding direct sunlight printing is to put MAKING A PRINT 87 tissue paper or a piece of ground-glass over the face of the frame. Other matters in which care is necessary are in ex- amining the print. This should never be done in direct sunlight, since you may always, when opening the frame, shade it by your body, and it is best en- tirely to avoid touching the front of the paper with the fingers, or scratching the negative as you raise the paper. As fast as prints are dark enough, which in nearly all these processes means quite a little darker than they are finally to be, they may be placed in a box, a table-drawer, or shut between the pages of a book, which will entirely protect them until you are ready for the next step. In speaking especially of printing, there are a num- ber of methods that will be mentioned later, but here we shall take always the very simplest and most straightforward methods until we have been through one whole process from exposure to finished print. The next step with your prints is to tone them — that is, to substitute a pleasanter and an enduring colour. After printing, you will have a picture from which you can get an excellent idea of the success of your work, but it is still somewhat sensitive to light, and would of course gradually turn dark all over un- less protected. But do not be afraid, if your paper is fairly well protected from long exposure to light, dampness, and so on, that there will be any change until you are ready to tone. The steps in toning are these. First, to wash in water made slightly salty with a little table-salt, for the purpose of removing as much as you can of the silver compound that has not been turned dark by the 88 PHOTOGRAPHY FOR YOUNG PEOPLE .* light. This compound, when dissolved in the water, makes the water slightly milky, and therefore so long as by gently rinsing the print the water still whitens, you may know that you have not removed all the silver compound possible. When the water remains almost clear, which will be after a few minutes' wash- ing, you are ready to change the colour of the print. This is done by taking away from the print a portion of the darkened silver and supplying in its place a darker compound made from gold. Usually chloride of gold is used in a weak solution, as the formula at the back of the book will show you. In this solution the print is placed and kept gently mov- ing, so that any little particles floating about will not settle in one place. You will then see that the print will gradually change in hue, losing its reddish tone and taking on a little darker tone, approaching nearer to a purple-black — the usual colour of a finished photograph with which we are all so familiar. When the colour is right, the print is put into a hypo solution which dissolves out still more of the unchanged silver compound, but does not attack the darkened portions. The print is now not sensitive to light, but, being soaked in hypo, has to be washed just as the plates were washed after developing, and even more thoroughly, since the hypo in this case has soaked well into the fibre of the paper, as well as into the coating. All through the processes of washing, toning, and fixing prints, cleanliness is, if possible, more important than in making the negative. It will be wise to handle the prints as little as possible, lifting them when neces: sary by the corner or by using a glass rod. Then, Photograph by Mr. K. Theodor Krantº * BRoadway in A SNow-Storm. " An artistic picture obtained from an ordinary city scene. In the original the effect of falling snow was increased by using a rough surfaced bromide paper. Courtesy of the Photographic Times The photograph was made during the snow-storm. MAKING A PRINT 89 too, they must be dried, and for this purpose many use a specially made blotting-paper, the fibres of which do not come off on the prints. Photographic supply dealers sell “blotter books” in which leaves of blot- ting-paper alternate with leaves of oiled paper. The prints are laid in facing the oiled paper and put under gentle pressure. Before putting prints between blotters, you should mop off all surface wetness with an old soft handkerchief. They may afterward be pinned up by the corners, after being slightly blotted on the back; but, whatever you do, they will, in drying, curl more or less, since the coating on them tends to contract and roll them up face inward. This, however, can be corrected afterward, by passing a stiff card or flat paper-cutter over the back of the print with a wiping motion, while holding up one edge with the other hand. The curl- ing that occurs after they are mounted may be reme- died by running the photograph through a cold bur- nishing machine. If your prints when taken from the washing bath seem particularly soft, tender and inclined to stick to the blotter, let them dry first in any fashion that they will, spread out in any convenient place. When they are dry, dip them into water again only long enough to make them limp, and place them between blotters; this time, not being quite so saturated, they are less likely to stick. Before you come to mounting, however, you have an excellent chance to show your good sense and artistic taste in the great art of trimming, and for this purpose there is nothing better as a guide than two pieces of cardboard cut into two right angles. These two pieces, each shaped something like a carpenter's try- 90 PHOTOGRAPHY FOR YOUNG PEOPLE Square, can be slid one over the other so as to leave an opening between them of any rectangular shape. By placing them over your print, and trying them at different places, you can find out just how much of the print is best saved. Having decided this, holding your pasteboards steady, mark lightly with a pencil on the print where it is to be cut, or, with a pin or needle point mark the four corners. With the four corners marked by tiny holes, you can turn the print Over, rule between the holes, and then cut out the print with knife or scissors, either of which is quite as good, carefully used, as the sharpened wheel sometimes sold , in the shops for the purpose. The question of mounting your print comes next, and is almost endless in variety. But for mounts and so on, you must refer to the dealers' catalogues and stocks. It will be better for you to use either the pure photographic pastes sold for the purpose, or the dry mounting-tissue which, pressed under a hot iron, fixes the print firmly and keeps it from curling. If you use paste, it should be put on very evenly from the centre outward, placing your print face downward on a news- paper. The print should then be applied to the card- board, middle first, paper put over both, and pressure gently applied from the centre outward, making sure that the extreme edges stick. Then wipe the edges clean with a damp cloth. Dry the whole under heavy pressure, and you will have done all that you can do unless you go into the matter of burnishing the surface, or giving it a glacé finish. After the print is mounted there is no way of burnishing it except with a rotary burnisher, which is rather an elaborate machine and hardly Worth the ex- MAKING A PRINT 91 pense. The glossy surface is not much liked at present; but if desired it can easily be obtained on P. O. P. by the use of a “ferrotype plate,” a thin sheet of soft iron coated with black enamel, sold by photographic dealers. The ferrotype plate is prepared by putting on it a few drops of benzine in which a little paraffine has been dissolved, and then polishing the plate off; this is to prevent the print from sticking. The print while quite wet is laid on the plate and the air bubbles pressed out lightly with a blotter. When it is dry, it will easily come off, showing a high surface. A “matt” surface that is really more satisfactory to the eye may be obtained on P. O. P. by using a good piece of ground-glass in place of the ferrotype plate. Besides the method of mounting the print on a card there is that of “tipping ” the print on by its two upper corners. Of course, in this case the print must be made to lie flat, and in this respect platinum, gum and carbon prints (which will be explained in another place) have an advantage, for they have no tendency to curl. But the method is good for all prints in that it allows the use of mounting papers in beautiful shades, which may be had from dealers in fancy and “cover * papers. These are made to be used on covers of booklets, programs, and the like. Any obliging dealer will furnish a sample book of cover papers and will probably sell as few as half a dozen sheets of whatever you select. The developing papers, or “gaslight papers,” as they are sometimes called, are really much like slow plates in their action, and the method of treatment is so similar to that of developing plates that the same * 92 PHOTOGRAPHY FOR YOUNG PEOPLE principles apply to it, except that there is a difference in the emulsions used. As to the printing, it has the great advantage of being done by artificial light, the strength of which can be perfectly regulated, so that, having learned just how to make a print of a certain quality by regulating the light and the time and dis- tance you can repeat the same method again and again, getting uniform prints. Of course, in the printing-out papers you use day- light, or sunlight. This varies in strength, and con- sequently your prints are not so certain to be uniform. The best way of finding out how to print a negative under artificial light is to take a sheet of paper, such as Velox or Cyko, cut it into a number of narrow strips, perhaps half a dozen, keeping all these strips except one protected from the light ; put this one strip under the negative, and keeping it at a known distance from your light, whether it be candle, lamp, gas, or electricity, guess as near as you can at the right ex- posure after reading the directions that come with the paper. Then develop that tiny strip. If it is right, make your exposures at the same distance and for the same length of time. If it does not make a good print, take a second strip and try a different time at the same distance, and so on until you have a strip printed to suit you. By these experiments you will discover the best time for printing each particular negative at a certain distance from a certain light. If you are truly sys- tematic, this can be noted down, so that you will always know how to print that particular negative ; for negatives differ in their printing quality, needing different exposures according to whether they are MAKING A PRINT 93 more or less transparent and contain more or less variations in their lights and shades. The Welsbach gas lamp is said to be the quickest in its printing action on developing papers, and with a rightly exposed negative the print is made in ten or fifteen seconds, but some dense negatives may not give good prints in less than three or even five minutes. It is sometimes well to print from such negatives by faint daylight, in spite of the fact that in daylight printing it is difficult to judge exposure of the print. A negative which by artificial light yields a print that is harsh and too violent in its contrasts will give a softer print, with better detail in the shad. ows, by daylight exposure. A secret worth knowing, if you are ever without a printing-frame, is that developing papers may be quite as easily printed by holding the negative and paper in the hand. A piece of pasteboard of the size of the plate should be placed back of the paper, and an old plate, or any other plate, should be placed back of that. If gripped firmly, with the knuckle of the fore- finger pressing on the rear plate, there is no danger of the print shifting its position. Strong elastics or metal clips may be used to hold the plates to- gether if one does not want to hold them with the hand. It is understood, of course, that in the developing paper no image is visible, even when the paper is printed correctly, until you have put the paper into the developer and waited for the image to appear. The manner of developing these papers is exactly the same in principle as the manner of developing plates, and the processes throughout may be said to be the same — 94 PHOTOGRAPHY FOR YOUNG PEOPLE that is, they must be developed, rinsed, fixed in hypo, Washed, thoroughly dried. You will notice, however, that there is no toning, if you are making simply a black and white print. An advantage of this method of printing is the fact that you can buy the sensitive paper in perhaps half a dozen different qualities, thin and thick, quick and slow, glossy or rough, and that each of these varieties is of great use in securing the best effect from partic- ular negatives. Another advantage is the fact that since these papers are printed in the evening, the prints can be made when the amateur is at leisure. Although the process is generally like that of developing negatives, there is a method of develop- ment for these papers which should be mentioned, since it is a very economical and easy way of working and tends to keep your solutions clean. This is what is known as “brush development.” After you have printed the paper, it is placed face upward upon a glass plate lying in and against the side of a tray. With one hand you hold the print down against the glass, touching it with your fingers only at the cor- ners, and then with a wide camel's-hair brush made for the purpose, or a tuft of cotton, the developer is gently applied to the face of the print, at first in a few broad sweeps so as to cover it all evenly and quickly, and then to and fro across the face, keeping it evenly wet. In this way you “brush out ’’ the image, using only enough developer to keep the surface wet, letting the surplus solution run down the glass plate into the tray. Thus for each new print you use fresh developer, keeping the solution clean. Otherwise brush development proceeds as before. To a certain MAKING A PRINT * 95 extent you can bring out with the brush certain parts of your print, only leaving others undeveloped ; but this art can be acquired only by experiment, and much the same effects can be attained by methods of print- ing. CHAPTER IX WHAT TO PHOTOGRAPH Photography and art — Choice of subject — The effect of colour — The importance of contrast — The eye and the camera — Imagination and fact — The eye's wide view -– A view-finder – Possibilities of a small camera – An instance given — Suiting the work to the camera — Pictorial facts and pictures for pleasure — Portraiture partakes of the actual and the artistic. THERE has been a great deal of ink wasted over the question whether photography is, or is not, an art, but no such discussion leads to any practical result. So far as the amateur is concerned, he must treat photog- raphy as an art in order to derive either pleasure or profit from it; and even if some wise professor is able to prove by a series of perfect arguments that photog- raphy is not entitled to be thought one of the fine arts, all we should have to do to satisfy him is to cease to use the word “art ’’ as applied to photography and content ourselves by calling it “photography.” In other words, the whole thing is a mere matter of names and ways of expression. It is undoubted that photography is a means of producing pictures, and that these pictures are of two kinds — good and bad. Our purpose is to make good pictures whenever we can ; and in order that they should be good, the first thing to resolve upon is to choose such subjects that photog- raphy is able to make them into good pictures. At the very beginning we must never forget that, so far as we are concerned, we are making a black and white negative. The charms of colour may afterward 96 WHAT TO PHOTOGRAPH 97 in various ways be added to the photograph, but in all cases except a few complicated processes carried on under peculiar conditions, the first necessity is a good black and white negative. Consequently the first thing to learn in thinking of what to photograph is how any natural object will translate into black and white. Of course, in certain processes the photograph is afterward printed in other colours than black and white, and so by the terms “black and white ” we must be understood to mean also lighter and darker shades of the same colour — in other words, monochrome — for unless a picture is good in black and white, good in its gradations, it will not be good in any tint. The next thing to think of is what shades of black and white are produced by natural colours in photographs. For the amateur it is perhaps enough to remem- ber the general principle that of the three main colours, – red, yellow, and blue — red and yellow will come out darker than either appears, and blue, lighter. With this rough guide we shall be able to judge generally the effect of colours when translated into the photograph. As to tints between the three primary colours, we can judge of the effect of these by remembering of what they are composed. To take the two common- est—green and brown — we must remember that green is made of yellow and blue in varying proportions, and consequently it will incline to light or dark in the photograph as it has more of blue or of yellow. The yellower the green, the darker it will be so far as colour is concerned, though it must not be forgotten in applying this rule that brilliancy of light, the amount of light reflected, has much to do with the 98 PHOTOGRAPHY FOR YOUNG PEOPLE result. The second common colour, brown, is made of all three primary colours, or, it may be said to be a mixture of red and green. Here, again, we must judge of its effect in the photograph by a general idea of the proportions of the three main colours a common brown contains. You will not often need to think of these things in taking outdoor pictures, but when you come to con- sider the effect of different colours in costume, you will find these principles a great help in getting good results. Even more important than the question of colour is the question of contrast. In fact, an old photographer has declared that the whole secret of making, good pictures by means of the camera consists in being sure to secure your contrast of light against dark and dark against light. Whenever you are thinking of mak- ing a photograph of any scene or object, it is well to form the habit of examining the whole subject of your photograph in order to see whether light things are brought against dark backgrounds and dark things against light backgrounds. That is, of course, unless you wish certain parts not to stand out strongly. In taking a portrait of a person in a white dress, you would usually want the face, which is the important thing, to stand out, and the dress to be less notice- able; SO you might use a light background behind the dress. It is amazing, in examining a number of snap-shots, to see how many pictures are spoiled in effect by the coming of things of much the same tone one against the other. You will secure many almost charming pictures that would be exactly what you desire except WHAT TO PHOTOGRAPH 99 for some unfortunate carelessness in bringing (for example) the face of your principal figure against a background in which it is almost lost, or in losing the outline of the head against a background too like the hair. And the remedying of this defect is often exceed- ingly easy. It may mean only a moment's experi- menting in moving the camera a little more, up or down, right or left, so as to bring nearer and more important objects against backgrounds of the right shade. Here, too, the colour question comes in. To give a simple example, imagine a young girl wearing a bunch of red roses on the front of her bodice. If the dress be black, the contrast of colour may appear strong and artistic; but in the photograph if the red happens to be the pure red shade that makes little impression on the plate, you will lose this contrast almost entirely. Unless you bear this principle of contrast constantly in mind, it is not a matter that will be suggested to you by the eye, because the eye sees largely as the brain directs it, while the camera is a mere brainless machine. When we look at a scene, a group, or a person, what we see with the eye is largely governed by our interest in the subject. We are unconscious of what does not interest us, but the camera is just as much interested in an ugly background as in the most charming person who stands against it, in the gleam of a brass button as in the bright eye of a belle. This same remark applies just as forcibly to the foreground. The eye overlooks many trifling ob- structions in giving its whole attention to the main subject of the picture; but the camera is quite as 2 º e - e : º © 100 PHOTOGRAPHY FOR YOUNG PEOPLE willing to take the picture of a dead branch that comes in front of a medieval castle as it is to receive the impression of the romantic old castle itself. You must therefore teach your eye to examine the whole scene with the impartial, matter-of-fact, un- romantic eye of the camera lens, for the camera will not pay any attention to your preferences as to what it should take. A rather poetic and yet useful way of putting the suggestion as to what subjects ought to be chosen will be conveyed by saying that while the human mind is infinite, the camera and the picture that comes from it are finite. This means that the picture made on the retina of the human eye is not thought of exactly as it is, but is thought of in connection with what we are imagining about it; it is unlimited. The pleasure that we take in a scene comes not alone from what we see, but sometimes even more from what We are thinking about what we see. When the same scene is taken upon a sensitive plate in the camera, We get only what was seen and not what the mind of the photographer had added to it. It may well be that when the picture is shown to another eye than his, the mind of the other person will think Very differently about the scene, and so may miss the very things that made it charming to the photographer himself. In one thing especially is this true. The eye at one time can take in a very wide horizon, and every part of that horizon, even if it be not distinctly seen, has its effect upon the mind and so helps to decide the effect of the view. Usually the camera can take in but a small angle of the horizon, or, if it takes in a e • *e e © ſº WHAT TO PHOTOGRAPH 101 larger angle, this must be at such a distance that the objects included are so reduced in size as to lose much of their character. Hence it is that in considering what to photograph we must try so far as possible to put ourselves in the place of the camera, giving our attention only to what appears within its angle of view, and consider- ing all things that are within this view as equally important. An excellent way to teach us how to know just what the camera will include is to cut out of a sleet of paper a small square opening, perhaps not more than half an inch on a side, or, better yet, a small ob- long opening of the general proportion of the plate used. Holding this paper at such a distance from the eye that it will include as near as possible the same view that is shown by the finder, we shall be able to know beforehand how much of a given view will be included upon our plate in the picture to be taken. By moving this screen in different directions we shall soon find that there are a great number of different pictures to be taken from nearly the same point. After a time we can use the finder of the camera for the same purpose, but at first it will be better to use the screen with a hole in it because the image seen through the opening is very much brighter than that reflected in the finder, and is much easier to be studied. There are, it has been mentioned already, a great number of finders made upon this principle — an oblong opening serving simply as a frame to show what the camera includes; and these, of course, offer the same advantages as the paper screen, excepting only the fact that they do not shut out surroundings. 102 PHOTOGRAPHY FOR YOUNG PEOPLE Unless you use some such device you will be sure to make the mistake of trying to include upon a 3% x 4% plate a scene that would be too much even for a plate of quadruple the size. For example, admiring the view from some mountain top, you will unsling your portable camera and make an exposure with some idea that you have secured upon your plate at least a faint impression of the wide expanse before you, with its sense of distance and space. When a print is made from such a negative it will be amazing if you have not a most commonplace and uninteresting result. If, beforehand, you had used the paper screen and reflected that you could not possibly get on your plate more than the little section of the distance visible through the opening, you would have saved yourself your plate, your trouble in ex- posing, developing, and in printing, and a sense of dis- appointment over the limitations of photography. This does not mean that even with a tiny camera it is not possible to secure distant views that are well worth while. Give a skillful photographer even one of the miniature cameras of west-pocket dimensions, and he will secure for you results that for artistic value compare favourably with those of twenty times the dimensions. For example, there was a young man amateur who took a great fancy to the original “Pocket Rodak,” the small oblong box camera brought out a number of years ago, and small enough to be held in the palm. Using this little box upon an ocean voy- age, he brought home a number of beautiful prints that owe their value almost entirely to the good sense and artistic taste he had used in making the exposures. The prints were one and a half by two inches in size, Photograph by Miss Florence M. Robuts Courtesy of Photo-Era Magazine Courtesy of American Photography This picture would have been better with a light background for the small boy, showing his head more plainly and giving less promi. - - nence to his white suit. Effective Photographs Taken With Small Cameras WHAT TO PEIOTOGRAPH 103 z' and yet by making sure that he did not forget what his camera could and could not do, he secured beauti- ful pictures. Of course many of them were vessels passed on the voyage, but the time of taking each picture was chosen exactly right. If he made a snap- shot of a passing steamer, the picture was so placed that the trailing smoke, the passing boat, and the lighting of the waves, made up a charming composi- tion. Or, if there was a particularly artistic effect of clouds during a sunset or a storm, he had chosen just the right section of sea and sky that made a picture. Aboard ship he had been careful not to get too near his subject, and had thus avoided bad proportions — that is, the proportions which were not such as the eye recognizes as usual; and he had also been thoughtful in placing figures against the right background or in the right surroundings, and so had been as wise in his compositions as when making little distant views. Probably if this same man had owned three or four cameras of different sizes he would never have become so skillful with the baby camera he carried; but prac- tice and natural good taste taught him to use the lit- tle box to the very best advantage. We have spared a little space to tell of his success because it carries in it the secret of good art, or good photography. A good workman fits his work to the tools he uses, not attempting to execute miniatures on ivory with a house painter's brush, nor to paint a board fence with a fine red-sable pencil. Consequently you must first of all remember to fit the work you are about to do to your camera and the size of its picture and the speed of its lens, to your own skill in handling it, and to the purposes of your 104 PHOTOGRAPHY FOR YOUNG PEOPLE work. The meaning of this last phrase is to remind you that there is more than one reason for taking photographs. We deal mainly in this book with the pictorial side of photography, but it is often the case that a photograph will be made for scientific purposes, or for a record. We wish to remember certain facts, and find the camera a most accurate and ready means of keeping them for the future. Much of the work that is done by tourists in foreig. lands must be of this character. It is intended to be shown to friends at home and to convey do them certain facts we wish them to know. For such photography our standards must always be a little different from those by which we go when making pictures for artistic reasons. It may be that much of the dispute that has taken place about photographs and their artistic value has come from not clearly understanding that many pho- tographs are no more than pictorial facts, instead of being pictures created for mere esthetic pleasure. And yet the distinction is one of the greatest im- portance to the young photographer, and should be borne in mind when he is choosing his subject and posing his picture, for the principles governing the two kinds of work are widely different. In the one case you must secure your facts, whatever else you sacri- fice; and you cannot therefore pay chief attention to mere matters of composition and arrangement. For the artistic picture the thing to think about is the im- pression to be made upon the mind of the spectator, and the question of mere fact is quite unimportant in comparison. The case of making portraits partakes, strangely enough, of both sorts of photography. It must at the WHAT TO PHOTOGRAPH 105 same time be a record of recognizable facts about the person photographed, or the picture must be a failure as a portrait ; and the portrait must also be so artistic as to make the right impression, or it will be no more than a sort of catalogue of facts about a human being and will lose all personal interest. This all sounds rather difficult, but unless pho- tography was difficult in these very ways — unless it gave you a chanci to show your own good sense and good taste — it would have no charm and only a very practical value without artist; pleasure. - CHAPTER X OUTDOOR PEIOTOGRAPHY Differences between indoor and outdoor work—Light and distance — Width of view — Landscapes — Views — People — Plant life — Animal life — The seasons — Cautions about each season's work — Landscape work – How to look at a landscape — Seeing truly — Artistic composition — Need of a principal object — Avoiding exact divisions — Place of the sky-line — Leading the eye into the picture — An outlet — The study of composition — Right lighting — Pointing the camera toward the Sun — Making a screen — Tak- ing near objects — Effect of tipping the camera – Wind blowing blurs branches — Value of reflections from water — Emphasizing Ş. character — Taking portraits outdoors — Position of the eyes — \ Direction of motion important –Seizing the quict moment — Nature photography — Value of the tripod. So far nearly all the principles of which we have been talking apply to every kind of work, but when \ we speak of outdoor photography it will be necessary \to divide the subject somewhat so that we may give imore definite directions; for it will be readily ad- n itted that so broad a phrase as “all outdoors” is ra. her a wide and comprehensive matter to talk about. Yet there is a difference between all camera work done under the sky from that done under a roof. There is a marked decrease in light just so soon as you enter a house. Outdoors, light rays are diffused in all directions, to be everywhere present, ready to act pon the plate. Consequently, in general, and except \r the early morning or later evening hours, outdoor tography is a matter of comparatively short ex- 106 OUTDOOR PEIOTOGRAPHY 107 It has also for the most part to deal with varying distances; that is to say, the distance of the object taken may be from a very few feet to as far as the eye can see. Indoors, on the contrary, the light is more concentrated in direction, less abundant, making longer exposures usual, and the distances at which objects are taken are greatly limited. These differences alto- gether bring it about that most Outdoor exposures are snap-shots, or very short ; most indoor exposures re- quire considerable time. Another difference is the range of view. Since, as we have already pointed out, the angle of view of the camera — that is, the field of the scene it can take in — grows larger the further the objects are from the camera, it follows that indoors the field of view is very narrow, and outdoors it may be exceedingly wide. We can divide the subjects for outdoor pictures only very generally into classes. The first of these we may call “Landscape,” including in the term views the pur- pose of which is to show aspects of nature, large natural objects, or scenes. For the second we shall have to make up a name, and call them “Views,” meaning outdoor pictures in which the main interest consists in objects not very far from the camera, cer- tainly not more than a hundred feet. The third class may be generally called “People,” including such views as owe their interest to persons, or human life. In addition to these we may consider the photograph- ing of animal life and of plant life. Though these terms do not by any means cover all possible subjects, yet they will be found to serve as good general names for the most usual classes of out. door work. 108 PHOTOGRAPHY FOR YOUNG PEOPLE But before taking up these separately something should be said about work at different seasons. Tak- ing these in their regular order, beginning with the spring, it must be remembered that though the light is growing stronger every day, it is not yet nearly equal to the light at midsummer, and allowance for Athis must be made in exposing. The great charm of spring landscapes lies in their delicate colouring and in what the budding foliage promises to the mind. Both of these features are commonly not to be ob- tained in a photograph. The delicate colouring, un- less by a happy accident of contrast, is lost in a hazy shade, and the promise, is one wholly of the human imagination, the sparse foliage (until it is well out, at least), being rendered by the camera usually as a col- lection of uninteresting dots. In order to make pic- tures that shall give the impression of spring, much careful study will be necessary and such early vegeta- tion selected as is by contrast made very evident to the eye. When we come to summer, the conditions for photog- raphy are at their best so far as the light is concerned and so far as the masses of foliage help in the composi- tion of the picture. But there are times of day when the strong light from near the zenith, at noon, gives harsh and unpleasant shadows, owing to the too strong contrast between light and shade. The heavy shadows cast by the trees in summer also make photog- raphy difficult in shady places and exposure must be lengthened to compensate for bad lighting. In places where the uninterrupted glare of the sun lights every- thing with great brilliancy, summer is the time to beware of over exposures. This is especially the case OUTDOOR PHOTOGRAPHY 109 at the seashore or on the ocean, where, in addition to the light of the sky is the light reflected back from the water-surface in all directions. This also must be allowed for by shortening the time of exposure, or, more easily perhaps, by using a sumaller stop for the lens thus making less exposure without changing the speed of the shutter. There are innumerable failures made upon the seashore every year by amateur photog- raphers who do not realize that the Ocean and sand are enormous reflectors turning back into the air the vast numbers of rays of light that on land are absorbed by the vegetation of the earth. - In autumn the American photographer, especially, needs to be warned against trying to secure by means of the camera the exquisite autumnal colouring that can be got only by the artist's eye and palette. Yellow and red are the dominant notes in this gorgeous dis- play of nature, and they are not good photographic colours, as you know. Consequently, where the eye sees a sharp, brilliant and striking contrast, the photo- graphic plate will give a dull and uninteresting result. Nothing has yet been said of “orthochromatic ’’ photography in this book, but since that is a means of holding back the quicker-acting light so that the slower-coloured light may have time to do its work on the plate, it usually means a slower exposure, and con- sequently must in most cases be reserved for such pic- tures as will admit of time-exposure. In the same general way we shall say of winter pho- tography that, with all its charm, it is difficult. The two things to bear in mind in winter are the weakness of the light, owing to the low angle of the course of the sun, which then is further south in our latitudes, and, 110 PHOTOGRAPHY FOR YOUNG PEOPLE Consequently, the fact that where there is snow in a Scene the exposure should be adapted rather to the shadows than to the bright lights. This for the reason that it is a good general rule in photography to look out for the shadow-exposure and leave the lights to take care of themselves, since the plate in a way pro- tects itself after the first instant that light has acted and does not, in the well-lighted portions, receive so much effect afterward as in those that are dark. The first chemical effect of the light on the surface makes the spot where the lights touch less sensitive, so they do not afterward receive the same action in proportion that is exerted upon the shadows. If this be borne in mind, and sufficient exposure be given, winter scenes will be found to give excellent results for the reason that there is less interference of de- tails, more breadth and simplicity in the views. The coating of the snow changes a rough and irregular ground into a more uniform surface. Shadows cast upon it are more sharply cut, and the absence of foli- age makes broad views possible while the often cloudy skies give excellent contrast with the whitened earth. So much for the four seasons. In regard to distant landscapes, the photographer will do well to acquire the artist's habit of squinting the eyes to get the general view — to lose sight of de- tails. In this way, without the trouble of looking into his finder or using the paper screen, or view- finder we have recommended, one may at a glance make a rapid estimate of the value of different views he sees; for when reduced to the scale necessary to include a distant view upon a small plate a great deal of the detail seen by the eye is necessarily lost. Trees OUTDOOR PHOTOGRAPHY 111 become masses, buildings do not show their smaller features, and, in general, we see only the broader effects. Another excellent hint is contained in the advice to look at a scene with one eye, thereby getting rid of the stereoscopic effect, that is, the effect of re- lief given by two-eyed vision. The camera gives this flat or one-eyed view, having the same lack of relief that is given by vision with a single eye. As to the natural features of the landscape, it is only people whose eyes have been trained that see them truly. It is well known among artists that we mentally exaggerate mountains, for example, as is shown by the fact that only very careful draughts- men will draw a distant range of mountains truly ; the temptation to the human fancy is to make them much higher than they really are. From this error the camera of course is free; and when it gives us a true picture of a distant range of mountains or of a single peak we know to be impressive, we are often disappointed to see how it is reduced by the camera to a not at all surprising feature of the landscape. As to the making up of a distant picture, the selec- tion of a good composition, of course this is so vast a subject that artists spend their lives in studying noth- ing else. It brings in the whole question of artistic composition. Nevertheless, a few principles are so simple and so well understood that they should be borne in mind. Perhaps the most important of these is what is known as “principality.” This means the necessity that the picture should have in it at least one main object that exceeds all others in interest. In making, for example, the picture of a distant horizon, you will 112 PHOTOGRAPHY FOR YOUNG PEOPLE obtain nothing interesting if one part of the horizon is no more interesting than every other. Somewhere there must be a point that attracts the eye, even if it be no more than a bit of cloud, a distant vessel, a single tree, or an abrupt headland. A second princi- ple forbids the dividing of your picture surface ex- actly in the middle by the horizon line. As to this, it can be said only that such a division is seldom pleas- ant to the eye, that either the sky or land portion of the picture should get the lion's share. In many old Dutch pictures, for example, the artists have made the sky and its clouds the most important part of their painting, while the wide and flat stretch of land be- low, diversified perhaps by a windmill or the sail of a sloop here and there, does little more than give one the impression of distance. It will be a good lesson to photograph the same scene from the same point, but at different elevations; so as to make a number of pictures that are alike ex- cept in proportion of sky they include. In pictures of the sea, especially, this question of the sky-line and its place on the plate is most important. In pictures taken on land it will be found most valuable to in- clude, if possible, some effect that leads the mind of the spectator to travel into your picture. This may be, for example, a bit of road or a pathway that serves as a means of measuring the extent of the picture, gives some idea of the distance included, and directs the eye from the foreground gradually to the distance. A stream occasionally catching glimpses of light by reflection will serve the same purpose of giving the spectator the unconscious belief that it is possible to go into the picture. Perhaps equally important is to give OUTDOOR PHOTOGRAPHY 113 the mind also an outlet from the picture. Landscape artists, except when they are seeking eccentric effects, are accustomed wherever it is possible, to give at least a small portion of their picture to a bit of distance, or to a spot of sky, to prevent the effect of being shut in among the nearer objects of the picture. As we talk on this subject we are constantly com- pelled to refer to the practice of painters, for this is really their art and one which has been studied since the beginning of landscape art. The best place to learn about the composition of landscapes is in the great picture-galleries where we can see the work of capable painters and can pick up hints as to the meth- ods of making their pictures successful. If you have the ability to draw at all, it will be a most valuable exercise to take to a picture-gallery a small pad of paper, or a sketch-book, and on this make little outline studies showing the composition of pictures admired. These studies should not be larger than a visiting- card, for they are not meant to include any study of detail whatever, but only to guide you to the general principles upon which artists act in the composition of their landscapes. If you are wise enough to take advantage of this suggestion, pay especial attention in each case to the direction from which the light of the pictures comes. This the shadows will show you. You will soon discover that much of the picture's value is due to right lighting, and you will begin to understand why a scene that is comparatively uninteresting at midday may be full of charm shortly after dawn or when the sinking sun casts longer shadows toward the east. Unfortunately, some of the most delicate lighting 114 PHOTOGRAPHY FOR YOUNG PEOPLE effects are not the best for photography, since in order to act well upon the plate the sun must be some distance above the horizon. It may be well here to say a word about pictures taken with the camera pointed more or less toward the sun. Naturally enough, those who publish in- structions for amateurs desire to make their picture- taking as easy as possible, and they almost invariably direct the photographer to take things upon which the sun falls, and not to point the camera toward the sun. As a general rule, this is well enough, but like other general rules in art it is to be ruthlessly broken under certain circumstances. It is true, of course, that sun-lighted objects take most easily in the camera. It is also true that it will not do to let the blazing sun strike through the lens upon the plate. But very many beautiful effects will be secured by taking pictures in which the light comes from in front; you thereby photograph the shadow side of objects against a lighter background, and you secure shadows running toward the spectator. In order to take these pictures, however, the lens must be protected by a hood, so that the direct rays of the sun will not enter it. This hood can be cut from a piece of cardboard, like the peak of a cap, and secured over the top of the lens or a little to one side, as is necessary to screen it, being fastened in place by a rubber band. So protected, you may safely take pictures toward the sun, if only the sun's rays are kept from the lens itself. You may even shade the lens with your hand, or your hat, for the moment of making an exposure. This question of the direction of light becomes OUTDOOR PEIOTOGRAPHY 115 especially important so soon as we change from the taking of distant landscape to the photographing of nearer scenes, in which, of course, the interest of the picture depends mainly upon a few principal things in the foreground. The lighting will be found to make all the difference between an attractive picture and a failure. A very little change in the point of view — holding the camera a foot or two higher or lower, more to the right or to the left — will give an entirely different effect. In such subjects we must recall to mind the importance of securing contrast by choosing a back- ground that will relieve the light and dark sides of the principal object. If you are taking buildings, monu- ments, or other structures in which there are hori- zontal and level lines, it becomes most important that the camera should be held level, since tipping it in any way gives you a very different result from that the eye sees. As to tipping the camera up or down, the effect will be to change the distance of the upper and lower parts of the object from the lens and plate. Tipping up the front of the camera has the same effect upon the picture, or view, that would be caused if you could view it from a station or bit of ground tipped in the same way. Also, by the change of perspective it causes all perpendicular lines to seem to come together as they recede. The tipping of the camera will make your vertical lines seem to come to- gether toward the top, if the camera is tipped up, or toward the ground if the camera is tipped down. In either way you will get an unnatural and distorted view, more amusing than valuable. This does not apply with so much force to natural 116 PHOTOGRAPHY FOR YOUNG PEOPLE objects, as these seldom have truly vertical lines and Consequently a slight distortion of them does not strike the eye as an impossibility. The matter of keeping the camera level sideways is of much less importance. Even if your view is a little tilted to right or left, the worst effect produced is the loss of a portion of it when you come to trim down your print so as to make the lines of the picture square with the edges. Consequently, unless you are photographing something in which the view is important up to the very edge of the plate, there will be little harm done even if your camera is tipped a little right or left. In photographing natural objects outdoors, such as trees and plants, you must be careful to remember the effect of the wind in blurring moving branches. For near objects this is important; and you will have to make a very quick exposure, or else select a calm day, if you wish to avoid a woolly appearance in foliage. A most valuable help in making little natural pic- tures will be found if you are able to include in the view even a small bit of water. A tiny pond some- times by its reflections brings the light of the sky into dark spots and so gives life and variety to your photo- graph. When the object is to bring out the beauties of rocky formations, or such natural banks as the shores of streams and rivers, it will be found most helpful to take up a position from which you bring the outlines of your foreground sharply against the sky or against brightly lighted fields or masses of foliage so as to give the outline, or profile, great strength by COntrast. And this suggests the secret of making successful OUTDOOR PHOTOGRAPHY 117 pictures of natural scenery — which is to decide what is the character of the scene and then to emphasize this by selecting the right point of view, the right lighting, and suitable position. You will see how this applies to the photographing of a rocky ledge, for example. If such a ledge be photographed from directly in front, it will lose its character of rockiness and angular strength unless the lighting is such as to throw portions of it into deep shadow and others into high light. In the same way the picture of a beach should derive its interest from the apparently limitless expanse of shore line and ought to be so taken as to conduct the eye naturally along the foreground to the distance. Here again we must refer you to the suc- cessful work of painters, who embody these principles in their best work. When you photograph people outdoors you will be guided by your purpose in taking the picture — that is, Whether you are seeking to make portraits, to secure incidents, or to make attractive compositions. In the case of a group taken for the sake of the portraits, you will find it almost impossible to get good results if the group is too near the camera. As the figures approach the camera a little difference in distance makes a very great difference in the scale governing the size of the figures on the plate. As a proof of this let us take, for example, a row of persons standing in a straight line at about ten feet from the camera. You will see that the shortest dis- tance between the camera and this line will be drawn from the lens to the centre of it. The longest distance Will be drawn from the lens to the two persons at the ends of the line. Consequently the people nearest © 118 PHOTOGRAPHY FOR YOUNG PEOPLE the centre will be shown on a larger scale in the pic- ture than those at the two ends, and the picture will not truly represent their heights. If, on the contrary, you place the same people in a semi-circular line all at the same distance from the lens, they will be truly represented in the picture, all being at nearly the same distance from the camera. The nearer the whole group is to the camera, the more difference is made by taking the portraits at different distances. As you go further away from the camera the differ- ence in distance from the lens becomes of less and less importance. In making outdoor portraits, if the light is bright you ought to have little difficulty in securing the natural expression on the faces of the people you photograph. You have only to watch the group un- til they have lost for a moment the stiff attitudes they will all try to assume, and then to make your quick exposure while they are at their ease. A very common fault is carelessness about the di- rection in which people are looking. To have them gaze fixedly into the lens is bad enough, but to have them look far off to one side is still worse, since the light striking upon the white of the eyeball usually gives a ghastly expression to the face. When it is a question of pictures of incident, you will find it makes a great difference in taking moving pictures whether the direction of motion is directly across the camera, or coming toward or receding from it. During the time of exposure, objects that move across the camera of course displace their images most upon the plate, and the quicker the motion the more likely are the images to be blurred. Hence it is that OUTDOOR PHOTOGRAPHY 119 in order to take pictures of moving objects the point of view should be a little in front or a little to the rear of a moving object, rather than directly across its line of motion. You will also secure many more successes if you will notice that in all such motions as walking, run- ning, jumping, throwing, and so forth, there are certain moments in which the motion is at its least. Thus, in taking a walking figure, if you catch the swing of the foot at either end of its motion, you will be likely to get a clear picture ; but if you time your exposure so that the moving foot is swinging past the other, it will be almost sure to be blurred. Suppose, again, a ball be tossed into the air. It is not difficult to catch an image of it at just the mo- ment when the ascent ceases and changes into descent. But when the ball has fallen almost to the ground, its speed is so great that it is beyond the capabilities of any except the quickest lenses and shutters. There- fore, before taking pictures of moving objects be sure to think out clearly the nature of the motion and to select that part of it which is slowest. Fortunately this will give you the effect with which the human eye is most familiar, for it is one which the eye most frequently catches and remembers. The human eye is far slower than many of the quickest photographic shutters, and so it is quite possible for you with a shutter moving at no greater speed than the fiftieth of a second to obtain pictures that to the eye mean very rapid motion. These principles will be particularly helpful to you when you are making portraits of children and babies. Though their motions are very quick, there is in any. 120 PHOTOGRAPHY FOR YOUNG PEOPLE occupation nearly always some instant at which they can be caught by the camera. When we come to the photographing of animals, in- sects, and flowers, we come to a field in which there is room for all manner of ingenuity, but we must be guided somewhat by what has been said about the sort of picture we desire to secure. If our object is scientific, and we wish to make merely a record of use- ful views, we must keep in mind exactly what those facts are and arrange our picture to bring them out plainly. But if the purpose is artistic, it should never be forgotten that we must secure such views as the eye is likely to catch. The camera must be placed as nearly as possible in the position from which the eye ordinarily views the object. It is far better in such pictures to get things upon a smaller scale rather than from unnatural points of view. - Take, for instance, the question of making a picture of a squirrel in a tree. There is very little object in so tipping the camera as to give a view of a squirrel upon a tree that, though upright, seems in the picture to lean at an angle of forty five degrees, even if by this we can get the animal upon a larger scale. With flowers it may be that this rule need not be so strictly followed. These are so frequently brought in- doors and arranged decoratively that we become famil- iar with them from all points of view, and so it is in- different from what point they are taken with the camera. In illustration of the ingenuity shown by some workers in this branch of photography we read that in order to secure clear-cut views of flowers, a clever photographer used light backgrounds of tissue paper of any desired colour which could be stretched Made with a Bausch & Lomb-Zºr'ss Tessar tº: INSTANTANEous Photography OUTDOOR PEIOTOGRAPHY 121 upon a slight frame of sticks and set up behind the flower he wished to photograph, so as to give him a picture of the entire plant without interference with other growths. By changing the colour of this little screen he could be sure of getting good contrast photographically whatever the colour of the natural flower. We will, in closing, make a little plea for the tripod. Unless the light and season are such that you may be sure of taking snap-shots at will, be sure to take your tripod with you whenever you go out with the camera. By its use you will be sure of being able to make a time exposure whenever and wherever you choose, and will thus secure pictures otherwise impossible. Merely because it is an accident that so often happens, we wish to warn you once more against walking against the legs of the spread tripod. While you are absorbed in arranging your camera, or in studying your view, it is fatally easy to forget the little tripod legs that straddle out so widely, and if you upset your camera you will be lucky indeed to escape injuring it. CHAPTER XI PHOTOGRAPHY INDOORS IT is evident at once that the chief difference be- tween outdoor and indoor photography is a matter of quantity of light, or rather one of length of exposure. It is true, of course, that in certain very brightly lighted rooms a shorter exposure may be given than in certain dark places in woods or between cliffs, and so on, outdoors. But even when the indoor light is apparently quite as strong, it will be found that the reflected lights which are so generally present out-of- doors are lacking indoors, and that the illumination is therefore less even. Especially will this be found true in the taking of portraits. We are more used to seeing people quiet indoors, and so are more familiar with the scheme of lighting. It is only when we come to making photographic portraits that we find how crude that lighting is, and how strong are the con- trasts between the lighted and the shadowed side in- doors. There is also a very great difference between the light at or near windows and doors and that even a very few feet away toward the centres of rooms. From this it comes that the best general rule in using the camera in this weaker light is to be sure not to underestimate the right exposure. If you must err, let the error be always on the side of giving the full length of time to the darker shadows. 122 PHOTOGRAPHY INDOORS 123 An experiment easily tried, and well worth trying for the information it gives, is to expose a piece of ordinary printing-out paper to the light in the mid- dle of a fairly lighted room and to note how very slowly its tint is darkened. Then, on even a dull day expose the same kind of paper outdoors, and you will see that the rate of darkening is very much more rapid. From this general statement you may draw the necessary rules for indoor photography in ordinary houses, for of course we are not here considering such lighting as the professional photographer gets in a studio especially prepared with skylights and side- lights and curtains. Under such a big skylight the times of exposure may be very nearly as short as out- doors. But in our own homes most of the lighting is from windows in the side walls that seldom give the direct light of the sky, and the colours of hangings, walls, furniture, and so on, are such as absorb light rays and prevent their being reflected back again. The two chief principles of indoor photography, therefore, are to give enough exposure and to secure an even lighting. The first is a matter of judgment and experience. If you are at all systematic you will by a few experiments learn about the right number of seconds to give when taking photographs in certain rooms of your house, and will allow a little more time whenever you are further from the source of light. In some of the circulars and hand-books, particularly those that come with small cameras, you are directed to use for indoor pictures a smaller stop than that used for snap-shots outdoors. There is no sensible reason for this piece of advice, unless it be the fact 124 PHOTOGRAPHY FOR YOUNG PEOPLE that in a long exposure, the beginner has more leeway, and a few seconds more or less will not spoil his nega- tive. The large diaphragm f/8 is the natural one for portrait photography, and an even larger one is often desirable ; for the shorter the exposure, the less chance there is of your subject's moving, or losing the charm of a fleeting expression. Besides, the sharp detail produced by a small stop is generally objectionable in a portrait. Perhaps, when you photograph your dog you may like to be able to see every hair distinct; but in the face of a person, sharp lines and little de- fects are things to be made inconspicuous, for the camera records many things which one's friendly eyes do not perceive. Five seconds ought to suffice you for a portrait exposure; rather than take longer, you had better secure brighter lighting. In a light room or sheltered part of a piazza you may be able to get the exposure down to less than a second ; in which case, if you have a shutter that can be regulated, you will find it convenient to use it set for one second or less. As to the length for different plates and films, you may secure very valuable hints in the directions given . by the manufacturers, especially those issued by the Kodak Company or by companies that sell exposure meters. Remember, however, that it is to the interest of these professionals to make sure that the amateur gives plenty of time, so you need not be afraid of err- ing if you do not go beyond the various lengths of exposure they set down for rooms variously lighted and variously finished in colouring. Even if you make no further use of an exposure meter than to adopt it for a set of trials to aid your judgment, the small amount the meter costs will be PHOTOGRAPHY INDOORS 12.5 very wisely spent in teaching you to judge conditions of light. Even those cheapest forms consisting of celluloid cards, or little disks that revolve upon a card, may be so used as to give you within a very short period most excellent ideas of the right exposure un- der various circumstances, at different times of day, and different conditions of the weather. From them you will at least learn, as we have remarked before, to think of all the different elements that go to make up judgment of exposure; and without some such mechan- ical aid the chances are very much against your guess- ing the right exposure until you have had considera- ble experience and thereby spoiled much material. As to the second principle, that of securing even lighting, this is largely a matter of common sense and home-made contrivances. For example, if you wish to take a portrait indoors, and should place your sitter close to a window with the light striking upon one side of the face, it is almost inevitable that you will get a very harsh result, full of contrast, and thereby make a picture that will strongly accent all wrinkles, irregularities of the face, and defects of complexion. And yet, even with the sitter in this position, a mo- ment's reflection and a little ingenuity will show you that it is a very simple matter to arrange white cloth or a large sheet of paper so as to reflect the light of the window upon the shaded side of the face, and thus greatly reduce the excessive contrast in lighting. This is often recommended. A still better plan is to place your sitter facing, or nearly facing, a window while you take the picture from near the window, looking at the fully lighted side. And even the fact that the sitter holds a book or 126 PHOTOGRAPHY FOR YOUNG PEOPLE newspaper as if reading it, will make all the difference between a pleasing and an unpleasing portrait, on ac- count of the lights reflected from the surface of the paper upon the sitter's face. If you wish to get an even stronger reflected light, it is often possible to do it by setting up a mirror in the right position to re- flect, not the sunshine, but the White light, where it is needed. The flash-light, too, may be used for the same purpose even in the daytime. The same sort of home-mad , will often serve to give you a plain ba at will throw out the sitter's head into excellu, v relief. If you wish to avoid showing the detail of this background, you should not use your lens with a small aperture, since the smaller the stop opening the more depth of focus there will be — that is to say, the more things will be in focus at the same time. Another way of avoiding detail in a background is to keep that back- ground in motion, so that it will be blurred in the photograph. Thus, behind the sitter's head you might have some one to hold up a plain shawl and to keep it gently moving so as to destroy the effect of its texture. If you do not have an artificial background, remem- ber what has been said already about the great im- portance of noticing all the little things that come into your picture, in order to make sure that there is no small detail to take attention from the portrait. We have seen, as a horrible example, a portrait group, one member of which, a bald-headed man, happened to be so posed that his head apparently formed part of a drawing of the “Sistine Madonna" and served as a convenient resting-place for the Child in his mother's arms. The one who took the photograph was so used PHOTOGRAPHY INDOORS 127 to the presence of the picture on the wall that he never noticed the absurd effect until it was brought out clearly by the photograph, and the group picture thereby made an absurdity. Of course such a blunder as this ought easily to be avoided. One you will be less apt to notice is the presence of little reflections of light from the glass of pictures, from the surface of polished furniture, or even from the backs of books. These reflections, hardly noti ve, often make very emphatic white streaks - raph and require much treat- ment of the negative or print to remove them. These things ought of course to be noticed in the finder at the time of taking the picture, but only a very minute examination will show them there, because of the small scale. A very slight change of position of either camera or sitter will usually enable you to leave out objects that interfere with the simplicity and direct- ness of the portrait. Since photography is with the amateur so often a summer amusement, a warning to him to consider dark piazzas as part of “indoors ” will not come amiss. Usually their ceilings are low and shut out the light of the sky, so as to make a long exposure necessary. If the sunlight strikes upon the sitters there is danger again of harsh contrasts and crude lighting effects. Perhaps, as an aid to the young photographer, an account of an actual experience in judging and making an exposure may be helpful. An amateur photog- rapher, sitting upon the piazza in a country place, noticed that his daughter, sprawled upon the piazza floor, had taken a rather picturesque attitude assumed unconsciously while reading. Being a believer in keep- 128 PHOTOGRAPHY FOR YOUNG PEOPLE ing a camera at hand, he warned the little subject against moving, stepped inside the door and brought out his magazine camera containing twelve 4 x 5 plates. The first thing was to see that the camera was in order, but a glance was enough to make sure of this. That glance showed that the shutter was closed, that the speed indicator was at one-fiftieth of a second (instantaneous), and that the diaphragm, or stop, was set at f/7.5. It was not necessary to see that the plates were in position, as the camera had been newly loaded and the index set at No. 1. Consequently the Only adjustment that had to be made was for distance, and the indicator was set at ten feet, since the object was to include not only the child, but something of the background and the surroundings, which were pictur- esque. The next matter was to determine the length of the exposure. For this purpose an exposure meter was used, being the one fitted into the cover of a little photographic diary issued in England. This diary contained all necessary directions, tables, and so forth, for the photographer, and was used to find out the necessary factors that go to make a correct exposure. The first thing to ascertain was the nature of the view to be taken. This, on a well-lighted piazza almost directly under the sky, evidently belonged to the class called “light foreground.” One reason for this decision was the fact that the house was of rough-cast painted white, and gave much reflected light. The next thing to be sought was the “light value.” This, as given in the tables printed, was, for the month of June, between the hours of 9 A. M. and 3 P. M., the fraction W6. This fraction referred to the meter, 1PHOTOGRAPHY INDOORS 129 where different light values appeared on a little wheel. The third question was that of the plate used. From a list of different plates was taken the figure opposite the Hammer brand, 94. This also referred to a set of numbers on the meter. The exposure meter was a disk, and the directions were to turn this disk until the nature of the scene (light foreground) came below the light value figure (%). This turning of the disk moved, of course, the whole edge. The next step was to find the plate- number (54) on the lower edge of the disk. Opposite this plate-number, on the paper back of the disk, were found, printed in red ink, the figures º'o - that is, so of a second was indicated as the correct exposure, all the things mentioned being taken into account. But this correct exposure was for the stop f/8, and conse- quently for f/7.5 the exposure might have been a trifle shorter, since the opening was larger. It was not neces- sary, however, to be so exact, since the plate, like most modern plates, had sufficient latitude to allow for the exposure being not quite correct, and no account was taken of this difference by the photographer because it is better to err, if at all, on the side of giving plenty of time. It will be seen that the shutter happened to be set at the right stop, and so the photographer had nothing to do but to look into the finder, see that the attitude of the subject and the surroundings were what he thought picturesque, and then to press the bulb that made the exposure. Immediately after making the exposure, the photog- 'rapher, having had several years’ experience, changed the plate. That is, he turned the handle which put 130 PHOTOGRAPHY FOR YOUNG PEOPLE the exposed plate away, and brought a fresh one into place. This to avoid the danger of a double exposure on the plate already used. If your subjects are interiors without figures, or in which the figures are subordinate, the main things to be guarded against are distorted perspective and halation. Distorted perspective comes from so taking a picture that the lines of objects are not such as the eye usually sees. It is not that the perspective is untrue; it is true for the lens, ordinarily. But if we take such views as are unfamiliar to the human eye, the pictures will appear absurd, unfamiliar, or mon- Strous. An early attempt of one amateur to take a photo- graph of a small child at the breakfast table, resulted, because of his inexperience, in the picture of a very small human being in the background and a gigantic coffee-pot dominating the whole photograph in the foreground. No doubt the human eye in this case would really have seen the coffee-pot on the colossal scale shown in the print; but since the mind of the observer would have been fixed entirely upon the child, the coffee-pot would not have been present in his mental impression. In taking interiors, therefore, be careful to remove such objects of furniture as come too near the camera and so seem greatly enlarged. Get as far away as you conveniently can from the room or from the walls that show in the picture, so as to secure ordinary perspective effects. We shall not here speak of the means of lighting up dark corners by the use of flash-lights and reflectors; but we should say, merely as a reminder, that it will not greatly help except in very long exposures to use PHOTOGRAPHY INDOORS 131 gaslight or lamplight, since neither is able to act strongly upon the photographic plate. Halation is the tendency of strongly lighted spaces or objects to affect the photographic plate beyond their true outlines. Thus, in a photograph if halation is not prevented a brightly lighted window will seem to be surrounded by a little halo of light, and the same effect will be produced by an electric light or by any point that strongly reflects a beam of light. This effect is produced in the following way: The rays of light go through the photographic emulsion on the plate, then through the glass or cellu- loid, and are somewhat reflected back again into the emulsion. You will see by a moment's thinking that the glass plate or film back of the emulsion having -> C Nº. .A. Yº: A §§e 43' * 4—Emulsion. <– Glass zr-º- Emulsion. *— Glas s ~ Bacting DIAGIRAM XIII behind it a dark surface is really a mirror, and as such reflects such rays of light as pass through the emulsion and support. Since these rays are reflected back, they follow the regular rule in regard to such reflected rays — that is, they make the same angle in striking the reflecting surface and in being reflected from it. The diagram shows how the amount of space affected by halation depends upon the thickness of the support 132 PHOTOGRAPHY FOR YOUNG PEOPLE of the emulsion and is wider as this is thicker. In Order to prevent halation plates are often “backed ”; that is, they are painted with some substance or pro- vided with a backing of some material good to absorb light rather than reflect it. Very often halation can be greatly avoided by making two exposures in taking the photograph of a single room. The first exposure is made with the windows covered — an easy matter when the room has white window shades. When sufficient exposure has been given, the lens is closed without moving the camera, the coverings are removed from the windows, and a very short exposure is given so as to show the windows uncovered. If it is desired that the view out- side the window shall also be clear and distinct, the fo- cus may be shifted to the proper distance before the sec- ond exposure. This should be done with care, so as not to move the camera, and by means of the focusing scale only, for it will not be safe to remove the plate-holder. It is usually best in taking interiors to select a view that will make the danger of halation smallest. But by the use of specially made non-halation plates, or by using films, which being thin have much less tendency to halation, it is not difficult to avoid the spreading of the light effect. In taking pictures of interiors when architectural features are important, as in public buildings, it is often well to use the “wide-angle ’ lenses — lenses so made as to take in more of an object close to the lens. Their effect really is to show the object as it would be if the observer were farther off than the camera stands — sometimes as if he were at a distance that would take him outside of the building altogether. CHAPTER XII FROM RULE OF THUMB TO KNOWLEDGE Résumé – Rule of thumb — What can be done by it — Rnowledge and its advantages—Steps necessary to knowing photography – Op- tics — Mechanics — Chemistry — What each includes for the pho- tographer — Laws of light — Theory of the camera — The emul- sion — The developer — The fixing solution — Washing—Toning — Different processes—The old and the new — Value of the his- tory of photography — “Photographer ” and “amateur.” So far, after a general talk about photography, We have tried to give you merely a short and practical account of the ways of picture-taking, with hints about the best subjects and about what to look for if you wish to get good results. There has been no dis- cussion as to why certain things are done, and no giving of reasons for the taking of some steps rather than others. Even in all this we have spoken to the beginner, and suggested what is best suited to him. In so do- ing, however, we have tried to tell especially those things that are not made clear in the printed circulars of directions, and to give the warnings that we should have found most useful when taking our first lessons in the art. Now we are convinced that the time to save plates is before the exposure is made, and that the most economical way of taking pictures is ex- pressed in old Davy Crockett's motto — “Be sure you're right, then go ahead ' " But in order to be sure one is right, it is not enough to go by directions given by others. The rule of thumb is only good 133 134 PHOTOGRAPHY FOR YOUNG PEOPLE until one has something better. Even by its guidance a careful photographer can do much. So many are the books and pamphlets and circulars that there is little for which directions cannot be found; and if these are closely followed, bad failures may be avoided. But there will be no improvement, no deep interest in the work, no delight in making skill take the place of elaborate devices, none of the pleasure that comes from seeing and overcoming difficulties. It cannot be necessary to say to young people of to- day that there is more education, more pleasure, and more benefit generally to be derived from a game or amusement requiring skill than in one depending on chance. Photography so greatly repays knowledge and skill that it is foolish indeed to depend upon mere chance for your results. As well might one own a horse, and never learn to ride, or a rifle without learn- ing to shoot, as to pretend to be master of a camera without understanding how to make it do its work. Neither should the young photographer be content to know the process of picture-making only in part. He need not know every way by which prints can be produced, but he should be able to make exposures, finish his own negatives, print from them satisfac- torily, and understand, in general, the “reasons why ’’ for each step he takes. If there were no other argu- ment for this, it would be found in the increased pleasure brought by fuller knowledge. For example, there are a few main principles that will give a good understanding of how rays of light act in passing through the air, and through glass, or through other substances, or in being reflected from surfaces. These the young photographer will find it FROM RULE OF THUMB TO KNOWLEDGE 135 helpful to know, and they may be known without delving too deep into the science of optics. Knowing these principles, the subject of lenses and their making will to a great extent become clear. He will see why one glass or a number are used ; he will be able to comprehend the making of compound lenses, and see why the surfaces take certain curves. He will have no trouble in seeing the use of the dia- phragm. He will find out what causes lens-makers to charge high prices for a few pieces of glass cemented together; and also he will be glad to learn that even with a low-priced lens excellent work can be done within its own rightful field. He will be able to understand the reference books, the special articles, that are all the time coming out to help the learner ; and he will not be misled by absurd and impossible statements made by irresponsible dealers or ignorant salesmen. Best of all, he will get the best results from his own camera, whatever it may be. A knowledge of the mechanical side of photography also has its great value. The modern camera is so made that, like an excellent rifle, it requires to be understood if one is to take advantage of its capabil- ities. It is humiliating to possess one of these ex- Quisite machines, fitted with every needful device, and yet to know little more than the names of its parts. The best cameras are really works of art, and marvels of skill; they deserve the careful study and expert use of which they are capable. Besides, every bit of knowledge one gains leads to more, and widens the field of the instrument's use, whether as a helper or as a pastime, as an instrument of pre- cision or as an artistic resource. 136 PHOTOGRAPHY FOR YOUNG PEOPLE The chemistry of the subject is undoubtedly very deep; but even this part of photography has its more general rules which can be readily acquired, and used to aid one in consulting books whenever more exact information is needed. For, after all, photography is a practical matter, and one can pursue each part of it knowingly without needing to carry the whole science in one's head. But the elements must be known so that the particular directions may be understood and rightly applied. He who would get the best results from photog- raphy must therefore know at least in a broad way the laws of light — how it is produced, how it travels, of what different kinds it consists, what effects these kinds have upon the compounds used in photography, how the light is affected by passing through lenses, or by being reflected by differently curved surfaces, or absorbed by others. He must be able to tell what parts of the camera are really essential, and what parts can be spared. He must understand how to ad- just the camera to meet various conditions of work, and how to remedy those little defects that might interfere with its best working, and how to keep it in the best condition for use. It is not necessary to be able to manufacture all one's own plates and papers, but one should be able to make an intelligent choice after having tested different makers’ goods, and to find out which are the best for his own use, whether for one occasion or another. And the same thing may be said of the chemicals used in developing and printing. There is a great variety of them to-day, and though they do not differ so greatly as was formerly supposed, yet FROM RULE OF THUMB TO KNOWLEDGE 137 there are uses for which each is best fitted, and some make easy results that are difficult if others be used. Knowing the general laws by which they act, the right chemicals for each kind of work may be chosen. The securing of a good negative is not always easy, and no one can tell beforehand just at what step of the process a difficulty may arise. The only safe way is to understand what is taking place, so that the right remedy may be applied when the hitch occurs. If you know how to do everything rightly, you will know at once when anything goes wrong, and so can do what is necessary to save your negative or your print. Knowledge also prevents much unnecessary drudgery in following rule-of-thumb rules without good reason. It is worth while to see a professional at work in order to see with what ease, rapidity and certainty the different processes may be carried out when one has a clear idea of what is to be done and how to do it. Washing and toning, fixing and drying, all can be done cleverly or stupidly ; and whoever has seen such things rightly and intelligently carried through will thereafter be unwilling to go blindly through a half- understood procedure. It is not, of course, necessary to know all the different ways of making prints. But it is well to study out those that you like best, and to understand these from end to end so they may be done in the best way and will produce the highest results. The interest one takes in photography will be enormously increased when at least some of the more common processes are entirely understood. Then the technical magazines will take on new interest, the 138 PHOTOGRAPHY FOR YOUNG PEOPLE exhibitions and competitions will have a new mean- ing, and will become helpful in your own work. You will be able also to keep up with the progress of the art, appreciating new discoveries and inventions, and taking advantage of what other workers are doing. The history of photography is not a long one. The whole story, from the first prints made upon sensitive paper to the improvements of our own time, covers.lit- tle more than the life of one man. The growth of the art and science, from being merely a curiosity and amusement to its present position when it is one of the most valuable of all helpers to exact knowledge, covers a still shorter time. To read the whole record, or even to study it carefully, does not demand much time or a great number of books, and yet will greatly add to one's appreciation of the wonderful achievements due to modern makers of lenses, of cameras, and of modern dry-plates. There is a debt of gratitude and a tribute of fairly won fame owed to the men who have created pho- tography, and have shown others how to follow in their footsteps. The work of such men should be familiar to us, and we should be ashamed to forget them while we remember the names of poets, Warriors, monarchs, and teachers to whom possibly is due no more of the benefits that make our lives pleasanter and more useful. If, however, one cares only to follow blindly the rules given, and to be satisfled with chance results, he may be entitled to the name “photographer,” but he has no rightful claim to be ranked among the “ama- teurs” — who love the art as well as practice it. CHAPTER XIII ABOUT LENSES AND THEIR QUALITIES The pinhole — Its faults and their correcting — Difficulties with lenses —Spherical aberration — Chromatic aberration — Distortion — Curvature of field — Astigmatism — Forms of lenses — Simple lenses — Rectilinear lenses — The anastigmats — Covering power — Rapidity — Convertible lenses — Portrait lens — The telephoto lens — Expensive lenses are for special work. IN order to understand fully the theory of the pho- tographic lens, one must go to the special books on the subject, as much space and many diagrams are neces- sary to make the whole matter clear. Here we shall try to give the amateur some acquaintance with the different kinds of lenses, the meaning of the names given them, the uses for which each is fitted, and their right management. We have already shown that a small clear opening — a pinhole — will take pictures, and would be the best of lenses except that it has certain serious faults. It is, when made carefully in thin material, really bet- ter than any lens in several respects: It is (within wide limits) always in focus ; it never distorts its image; it takes far and near objects with equal re- sults; it includes an angle of 180°– half the whole view ; covers any size plate; and lights all parts of the plate equally. These virtues are hard to equal in the best lenses, and until the defects are explained One is inclined to say, “What lens can be better than a mere pinhole P” 139 140 PHOTOGRAPHY FOR YOUNG PEOPLE One is reminded of the horse which had but two faults — he was hard to catch, and no good when caught. So with the pinhole. Its two defects are lack of rapidity, and lack of definition. That is, it admits very little light, and does not give a clear, sharp image on the plate. It is a perfect lens where one wants only a general soft picture, and is in no hurry. But nearly every photographer requires either good, clear definition, or quick exposing; and conse- quently we are driven to use lenses for the purpose of taking in a great many rays of light, so as to get quick exposures, and for the purpose of causing all the rays possible to come to the same focus, so as to get clear, distinct images. - Thus the whole purpose of the lens-maker is to keep the advantages of the pinhole while adding rapidity and sharpness. Hence the value of a lens depends on the number of rays it can bring to a true sharp image — that is, on “rapidity" and “definition.” But in trying to get these virtues, we meet with difficulties brought in by the use of the glass disk or disks. These difficulties are described as follows: Spherical aberration. To make lenses their curved surfaces must be spherical, so that they may be ground by tools that can move from one part of the surface to another without fitting unevenly. On a sphere all parts of the surface have the same curve, and the same tool will fit any part. Now the truly perfect lens should have another kind of curve known as the parabola or parabolic; but this is so difficult to make that it is never attempted, especially because it is easier to correct the fault of curvature in another Way, ABOUT LENSES AND THEIR QUALITIES 141 The effect of spherical aberration is to make the rays nearer the edges of the lens come to a different focus from those nearer the centre. Chromatic aberration. Of this we have already spoken. When the rays go through a lens the differ- ent colours are differently bent or refracted, and so come to different focuses, being separated by the lens. Distortion. This means the changing of straight lines in the object to curved lines in the image. When a stop or diaphragm is used in front of a single lens, it cuts off certain of the oblique or slanting rays com- ing from the margins of the scene photographed. These rays are those that would go through the centre of the lens, and instead of them the diaphragm lets through the slanting rays that go through parts of the lens further from the centre. These are not bent to the same point as the others, and so make the image at a different point on the plate. So the further away these points strike from the centre of the lens the more they are bent. & A C DIAGRAM XIV Hence if we photograph a square (a) it becomes in the image barrel-shaped (b) — the images of the corner part of the lines being brought too near the centre. If the diaphragm be put behind the lens (between lens and plate), it cuts off the rays that pass furthest from the centre, letting pass the more central rays, which 142 PHOTOGRAPHY FOR YOUNG PEOPLE are less bent. Consequently the curving is reversed, and the image of the square becomes cushion-shaped (c). Taking a single lens, and putting a diaphragm made of paper before it and behind it, successively, while casting an image of a sharply drawn square, will show this effect, though it is not very marked in a small picture, and is of less importance in a smaller camera. In a double lens, with the diaphragm be- ſ tween lenses, the distortion | caused at the first lens is -] cured by that | at the other, and the im- age c 0 m e S right. Curvature of field. The ordinary lens brings its image to a surface that is not really flat – like the sensitive plate or ground-glass – but curved, or saucer. shaped. (Diagram XVIII.) That is, when we focus to get perfect definition at the middle of the plate, we find the marginal parts slightly blurred. If we focus for these, the middle is blurred. To get perfect deſi- nition, the plate or ground-glass would have to be slightly saucer-shaped, which though possible is not convenient. - Astigmatism. Astigmatism means that the lens having this fault will not focus truly horizontal and perpendicular lines at the same time. Thus in trying to get a perfectly sharp image of a cross, we should have to make the horizontal arm sharp, and the up. right one blurred or vice versa. Or else we may so DIAGRAM XV –CURVATURE OF FIELD ABOUT LENSES AND THEIR QUALITIES 143 focus as to have a compromise— neither very sharp nor very blurred ; and this fault is worst at the edges of the plate. Where correctness throughout the whole plate is needed, astigmatism is a serious fault. There are other errors possible in lenses, but these are the ones that are considered in dividing lenses into classes, and the most important in practice. These errors can be corrected more or less, and in the best lenses the most serious are corrected. But it is not possible to correct all errors in any case, because all merits cannot exist in a single lens or system of lenses ; the merits do not go together. An example of this is seen in the fact that there is always some loss When light goes through even the cleanest glass, and yet some of the finest lenses require eight or more disks of glass to give them their good qualities; and that to get rapidity the lens should have a wide open- ing, while to get clear definition the opening must be kept small in comparison with the lens. So in mak- ing lenses the object to be attained is borne in mind and the lens made to suit that object. Here (a, b, c, d, e and f) are the simple forms of lenses from which all the combinations are made up ; (! b C d .* € f DIAGRAM XVI These may be understood quickly by noticing that either side may be flat in a lens if the other be curved; 144 PHGTOGRAPHY FOR YOUNG PEOPLE that both may be curved ; that in the case of a curve it may be concave or convex. These forms all bend rays of light ; and rays coming from a convex surface are brought together ; from a concave surface are separated; from a flat surface they come unchanged. By knowing these principles, and by using surfaces curved more or less, lens makers make the rays go where they please. But it is also true that different shapes of glass bend rays differently, and by putting together lenses of varying sorts of glass, the faults of one can be corrected by the merits of another. Let us see how these methods are used in making lenses use- ful in photography. The simplest lens is the bi-convex (a), which makes an image, but has all the faults possible to a lens, being entirely uncorrected. It is practically never used alone. The ordinary “single lens” is really made of two pieces of glass; and the bi-convex if found in a camera will be supplied with a small stop, an opening about 3% of its focal length in size. With this small opening only the very middle of the lens is used, where the errors are least. The only advantages of this “single non-achromatic ’’ are the fact that it ab- sorbs little light and is not apt to reflect light from its curved surfaces — a defect known as “flare.” It is slow, has poor definition, and is generally lacking in all good qualities. It can be useful only in very bright light, with a small stop, and where defining power and correctness of lines are not important. The “single achromatic " or “meniscus” or “achro- matic meniscus ” lenses are made of two lenses cemented together. The “meniscus’ lens is one with a concave surface on one side, and a convex on the * º - - Photograph by Mr. Ellwood Crane Courtesy of Photo-Era Magazine A Pinhole Photograph Notice:–1. Depth of focus, or equal definition of near and far objects. 2. Equal definition at corners and at centre. 3. Absence of distortion. 4. Absence of halation or ſogging, shown in the detail in the curtain. ABOUT LENSES AND THEIR QUALITIES 145 other (c). By grinding these surfaces to the right curvatures, or by putting together two lenses of dif- ferent shape (Diagram XXI), the errors of chromatic and spherical aberration are lessened or corrected. Sometimes a “ double meniscus, non-achromatic ’’ lens is made (Diagram XX) with a diaphragm midway be- Diaphragm tween the lenses; but this is not corrected for the chromatic error, and con- sequently the focus of its photographic rays is not the same as the focus of the visual rays, or the image DIAGRAM XVII seen on the ground-glass. If put into a camera, it is usually one that focuses en- tirely by scale, not on a ground-glass, and so allows for this defect. Yet putting this lens at the right dis- tance does not make it act like an achromatic lens, for the less active rays, though not in focus, act some- what on the plate to blur it. The true “single achromatic lens,” of two kinds of glass, is corrected somewhat for chromatic and spherical aberration, and when used with a small stop is capable of good work on bright sunny days, or on quiet sub- jects not needing great quickness. If used with a wide opening, these lenses show distortion and some astig- matism, which becomes evident when straight lines appear in the picture. In purely pictorial work the single achromatic lens is more useful. Its small aper- ture gives depth of definition, and its lack of sharp- ness is often an advantage. The amateur must not think that the “perfect lens” T Wº | 146 PHOTOGRAPHY FOR YOUNG PEOPLE is indispensable for good work in photography. For example, the smaller kodak cameras, Brownies, Num- ber 0, No. 1 Folding and No. 1 A Folding, with which so many delightful pictures are taken are supplied with meniscus lenses, and meniscus achromatic lenses. An expert could in a moment prove their limitations, but many of their pictures can hardly be improved upon because the camera has been used under the *ight conditions. ØN §§ º 2S § § RRCTILINEAR LENS WIDE ANGLE RECTILINEAR DIAGRAM XVIII The “Rectilinear ’’ lenses (also called “symmet- rical,” “aplanatic,” and so on) are made up of two lenses or lens combinations, mounted in a tube with a diaphragm between. (Diagram XXI.) They are “symmetrical” when the two combina- tions are alike in focus and make up. These lenses are usually so corrected that they will do good work with an opening of 96 the focus or more. They bring the colour rays together, have little spherical aber- ration, and little distortion. It is an excellent lens for all except the most rapid and most exactly defined work, provided it be good of its kind — which can only be known by actual test. The “Photo Minia- ABOUT LENSES AND THEIR QUALITIES 147 ture' on lenses (No. 79) says of the rectilinear : “It is still quite good enough for 80 per cent. of the work of the photographer, provided he does not attempt high-speed work, three-colour, or fine reproduction or scientific photography,” and again, “For all ordinary purposes, where critical definition from the centre to the edges of the plate and rapidity are not essential, the rectilinear of to-day with a rapidity expressed by an aperture of f/8 is as good a lens as the amateur can desire.” The Anastigmat lens is one that may be described as the highest type of rectilinear — one that carries the corrections to the furthest extent possible for the pur- pose it is intended to serve. To discuss all the different types would be only to copy the learning of others from various books on the subject. The anastigmat lenses became possible when the new kinds of glass, made in the town of Jena, Prussia, led to new experi- ments and triumphs in lens-making. Though even with the older varieties of glass the highest classes of lenses can now be made, it was the Jena glass that first caused their making, and showed them to be possible. The anastigmat lenses, because of their superior corrections, possess many advantages over the rectilinear. First, they are able to focus sharply at the same time both vertical and horizontal lines. Second, being so corrected, they can be used with a bigger opening, and so are quicker because they let in more light to the plate. Third, they have a flatter field — that is, bring the image nearly into a single flat surface, and so can be used with clear definition OVer a larger plate. All this amounts to saying that 148 PHOTOGRAPHY FOR YOUNG PEOPLE the anastigmat is a better corrected lens than the rectilinear, and so makes a better, clearer, brighter image on the photographic plate. Since the different anastigmats vary in their quality and Work, it is not possible to pick out particular ones as “best "for all sorts of work. The qualities that are best worth seeking are thus set forth in the “Photo Miniature" on lenses (No. 79): Covering power. Select a lens with which one can focus with a large opening, and yet keep the same covering power if the opening is made smaller. Select that giving the widest angle of view. Rapidity. Choose the lens working at the larger aperture if it is equally good otherwise. Convertible lenses. Choose a lens of which the Separate parts, when unscrewed, can be used as separate lenses of different focal lengths, if the whole lens is equally good. As to these matters, in buying of a dealer of good reputation, you may seek his aid and advice. But be careful to bear in mind, and to let him know, the pur- pose for which you mean to use the lens. For general hand-camera work, such as most amateurs will do, there is no need to pay for a lens of the greatest possi- ble speed and perfection. Such are made for scientific work, reporters on race-tracks, and for the making of process plates to be used in publications. A reason- ably fast lens — one working sharply and clearly at an opening of f/8 — will do everything except the taking of objects in very rapid motion; and for these there will be needed the very quickest forms of shut- ters — such as the focal plane. So far as picture-making is concerned, the really ABOUT LENSES AND THEIR QUALITIES 149 “instantaneous pictures” are seldom very pleasing, and except for these the chief benefit of using the quicker lens is in the ability to take snap-shots on grey days. Therefore do not be dissatisfied even if you cannot pay from $20 to $150 or more for a lens; excellent work is done daily with rectilinear lenses costing only four or five dollars. There are certain special lenses made for particular classes of work, and with these the young photog- rapher should have some acquaintance. There are the Wide-Angle lenses, which are merely lenses of shorter focus (or “focal length '') than is usually em- ployed with a plate of a given size in a certain camera. All lenses of the same focus, used on the same size plate, give the same amount of a given view — that is, they cover the same angle of view. A wide-angle lens is therefore one made to include a wider view on a given size of plate. It is useful to enable you to get more of a scene upon the plate your camera uses, but in order to widen the angle, the focus of the lens is made short, and it often works at a smaller aperture, being therefore slower. The small aperture is necessary in order that the illumination may be made as even as possible, for wide-angle lenses cause the illumination to decrease rapidly as the edge of the plate is ap- proached; and, besides, these lenses made for special, limited use, are often not so well corrected as finer lenses, and must be used with a smaller opening in Order to give even definition. The Portrait lens is one so made as to give clear definition over a limited part of the plate and to be usable at a very wide opening, giving great speed. The same class of work can be done with the best 150 PHOTOGRAPHY FOR YOUNG PEOPLE anastigmats, which besides have other advantages. If a soft, not too defined effect is sought, it can be had by slightly changing the focus of the lens that will give clear definition, so even on this ground the por- trait lens possesses no necessary advantage. The Telephoto lens is merely an additional lens (or set of lenses) that will give larger images of distant objects. The size of an image depends on two things — the distance from the camera, and the focus of the lens that is used. The nearer you bring the camera, the bigger is the image ; the longer the focus of your lens, the bigger is the image, other conditions being the same. The telephoto lens is merely a means of adding to the lenses on your camera another lens (or more lenses) that will make the whole combination act with a longer focus, and thus make a larger image on the plate. Since it spreads the image over more space, it gives an image less bright, and so must have a longer exposure, to make up for this. Also, as will be seen when we speak of diaphragms, the addition of the telephoto attachment making the focus of the lens longer changes the value of the number of your stop. It is not possible in one chapter to do more than state certain general principles about lenses. The sub- ject may be studied more closely in books devoted especially to the subject, and also in the pamphlets and catalogues issued by lens-makers. Remember, in closing, that in order to decide upon the lens you need, you must sacrifice those qualities which are least im- portant to secure those that are most important in the work you are doing. You must choose your lens to suit your camera, your plates, the subjects photo- graphed, and your purse. It is absurd to buy a lens Taken with a Bausch & Lomb-Zeiss Protar, Series VII a, with a High Power Tele-Photo Attachment The Magnifying Power of A Tele-Photo LENs The small picture in the upper corner shows the same scene as it appears in a photograph made with the same lens without the Tele-Photo Attachment. ABOUT LENSES AND THEIR QUALITIES 151 at a great price when you can do your work with one that costs a fraction as much. Expensive lenses are meant for securing the greatest possible speed, defini- tion, and covering power. For hand-camera work on small plates and for the general run of amateur sub- jects, a lens of reasonable cost will serve every purpose until you reach a very high degree of skill. CHAPTER XIV THE CAMERA AND ITS ATTACHMENTS Value of the tripod — Various attachments of the camera—Simplest camera the best —The level — Distance-measures — The swing- back—How it is used — Swing-bed — Reversible and revolving backs — Rising and falling front — Cross-swing — The value of a long bellows — Extension front — Drop front — The finder — Ex- posing with a cap – The virtues of a shutter — The focal-plane shutter — Its merits and its defects — The multi-speed shutter, and the reason for its action. WE shall limit this big subject at once by confining overselves to the “hand camera,” as it is with the port- able camera that young people have to do ; but it must not be concluded that we mean to say nothing of the tripod. On the contrary, we recommend the tripod should be used whenever possible, which means always except for snap-shot work. And in order that you may be willing to carry the tripod about, be sure to get one that is compact, small, and simple. The metal tripods that have telescoping legs are by far the best except that they are not (and cannot be) so steady as the wooden ones; but care in their use will remedy unsteadiness, and it is to be feared that you will dislike the trouble of setting up the other sort, and so will leave them at home. The same convenience in use recommends the box camera, as we have already said. It is ready always, and attracts less attention from onlookers. But the folding cameras are small, light, and will probably be 152 THE CAMERA AND ITS ATTACHMENTS 153 carried oftener, and you should get into the habit of having your camera at hand. But whichever sort of camera you choose, there are important things to know about its equipment and the uses of its important parts. These are divided mainly into attachments relating to the position of the camera, the placing of the plate, the moving of the lens, seeing the image, the regulation of the exposure, the changing of the plates. At least, these are the most essential. Under one of these headings come all ordinary devices that have to do with the exposure of photo- graphic plates in the camera. We cannot describe them all, but mean to give the chief kinds, and to explain the principles upon which they act. Knowing these principles the young photographer will learn how to use his own camera, and will understand the action of other cameras, and their advantages for special kinds of work. Still, though it is well to understand com- plicated apparatus, for regular use we are told by the most experienced photographers to choose the simplest camera that will do good work of the sort we want. If your attention is given to making all sorts of adjustments of the camera parts, you will not give your main thought to what is most important — the subject you are taking, the value of the light, the length of exposure. - To begin with the tripod, the amateur should choose one that is firm when set up, and light to carry. The metal tripods are most portable, the wooden ones firmer. When putting the camera on the top, screw it fast. If it rocks or turns when you make the exposure your plate is ruined, and it will rock or turn unless it be screwed fast. There are adjustable heads that allow 154 PHOTOGRAPHY FOR YOUNG PEOPLE the camera to be movable, but you will want your camera level except for special and peculiar work, and the plain tripod is therefore most useful. In tripod work, that is, for time-exposures, you may find use for the level. The best form is the single level, with a circular box. The level is only useful in Work that must be very accurate, such as architectural pictures; and for this work, you will have plenty of time to see that the bubble is in just the right place. In hand-camera work, the picture, if slightly crooked on the plate can be corrected by trimming the print true to the picture lines, and in such work the level is almost useless, merely taking your attention from more important matters. The same criticism may be made on the little plumb-line attachment for levelling, and on the distance- measures and so on. They are seldom useful, and often distracting. You will soon learn to judge distances fairly, and also will learn to make your camera level and straight by the eye alone. The real essential is a firm tripod and care in placing the camera. The attachments meant to move the plate, to change its relation to the lens, are the swing-back and the reversible or revolving back. The swing-back allows the plate to be tilted or turned on its centre so as to bring one edge nearer the lens than another. This of course changes the focussing of part of the subject. Suppose, for example, you are making a portrait of a man seated. If you bring the camera near him to get a large image, you may find that his feet are apparently magnified, and look out of proportion. By using the swing-back, you may bring the upper part of your plate nearer to the lens, thus getting a smaller image THE CAMERA AND ITS ATTACHMENTS 155 of the lower part of your subject. Trying the experi- ment with the ground-glass, you will see how this may be done. In the same way, you may better the appearance of a landscape subject at times by changing the focus of part of the plate. Another use of the swing-back is to make plate and subject parallel even when the camera has been slightly tipped up or down to take in a different part of a subject. Unless plate and subject are kept parallel, the focussing is changed on different parts of the plate — as we have just shown. So — unless we mean to make this change — whenever the camera is pointed up or down, the plate must be brought parallel with the subject by means of the swing- back. Ordinarily the tipping will be very slight, and the swing-back will be used only to keep the straight lines of buildings, pillars, and so on from being made to look out of perspective. The same effect can be produced by means of what is known as a “swing-bed.” In this arrangement the lens is tipped by raising or lowering the part of the camera on which it is supported. Besides being able to tip the plate on its centre, we can change its position by means of the attachments known as “reversible " or “revolving ” backs. The “reversible back" can be turned so as to bring the plate either long way or short way upward. The “re- Volving back" may be put in any position to suit the subject taken. Combined with a swing back, the re- Versible back allows almost any part of the plate, except the exact centre, to be slightly changed in focus. But these adjustments will not be often used by the 156 PHOTOGRAPHY FOR YOUNG PEOPLE amateur, and the want of them is not a defect in a camera although they are convenient at times. More important is the “rising and falling front,” and the “cross-swing.” These are methods of allow- ing the lens to be moved up or down, right or left, without moving the part that holds the plate. The lens-board is held between two uprights so it may be raised or lowered, by loosening a screw. The effect is to make the lens take a higher or lower view of the subject. Thus, if the lens be raised, it will take in more of a tall building; if it be lowered, it will include more foreground. The cross-swing allows the lens to be moved sideways — viewing more of one side or the other. Of course, if the camera be turned on its side (as so many cameras may be) these attach- ments exchange offices. If your camera has these attachments, include them in your “camera drill,” using the ground-glass to see how much the view is affected by each of the move- ments of the lens out of its usual place. Though you may not often use these attachments, now and then they become important, and will help to get a good picture otherwise impossible. The other way of moving your lens — to or from the plate — is of vital importance unless you are using the simplest “fixed-focus camera.” You will not be able to get all the good out of your lens unless your camera has a long bellows, and some means for supporting the lens firmly when the bellows is at its longest extension. The nearer you bring your camera to an object you wish to photograph, the further away must the plate be from the lens. Notice the divisions on your focussing-scale, and Courtesy of Eastman Kodak Co. º Eastman Kodak Co. . - - Courtesy of Ordinary Shutter, with Iris Focal-plane Shutter Diaphragm Courtesy of Courtesy of Eastman Kodak co. Messrs. Burke & James Developing Tank for Roll Film Developing Tank for Plates CAMERA Accessories . . . . . . * * - - -- THE CAMERA AND ITS ATTACHMENTS 157 you will see how quickly the spaces between the marks increase in length as you come nearer your sub- ject. With a short bellows you cannot get near views, or views on a large scale, without the use of an additional lens; usually you can get nothing nearer than about eight or ten feet. But with a long bellows, a view within two feet or even less is quite possible, and this is often desirable in taking portraits, pictures of flowers, insects, or still-life objects. The long bellows is often supported by an “extension front”— a part of the base that is arranged to slide forward. The long bellows, having many folds, sometimes needs a support from above, and a ring is attached so that a cord may be tied to it and to the top of the camera to keep the bellows from sagging by its own weight, and so cutting off part of the image. These things may seem very elementary, but often they are not explained in the directions for using cameras. The long bellows camera may be utilized also as a copying apparatus. If you have a photograph already on hand of which you want to make an enlarged or reduced copy, by setting it up in a bright light before the camera, extended at length, you may photograph it as you would any other object. It will probably be necessary in this case to unscrew and take off one of the lenses of your camera, if your lens is of the sort to permit the use of half of it at a time. By using the ground-glass, you can determine this. Be careful to arrange matters so as to have no reflec- tions from the surface of the picture you are copying. With this class of work, however, one cannot obtain the best results without special “copying plates” and development to bring out strong contrasts. 158 PHOTOGRAPHY FOR YOUNG PEOPLE One more mechanical attachment or arrangement is the “drop front.” When a very short focus or wide- angle lens is used, the front that extends out to sup- port the bellows might be in the way, and cut off part of the view. The “drop front ’’ is hinged, and can be turned down so as to be out of the view. Of the different sorts of finders, we have already spoken, and here we need only repeat the warning that the finder remains unchanged even when the main camera has been adjusted in several ways. The finder usually shows only the view that the camera, unadjusted, takes in : so remember that you may have altered the view the finder shows — especially when you change the focus or move the lens in relation to the plate. Possibly it may be well to say that the glasses of many finders are framed in an opening of this shape (a): F---------- l - - - - - - - - - * * * * * ** !----------— ©2 A. C DIAGRAM XIX This is when they are reversible, and is meant to show the limits of the view when the plate is turned one way or the other. Whichever way the finder is used, you may see what is on the plate provided you remember that the plate ends at the projecting corners, and you must take your oblong space either straight THE CAMERA AND ITS ATTACHMENTS 159 across, as in b , or upright, as in c, leaving out the pro- jections. Possibly it will be well for you to mark in ink or paint the limits of the views, as they are dotted in the two diagrams; it will save you some blunders. There are plenty of little things to think about when using a camera intelligently, and every help is useful in saving errors and trouble. In this chapter we shall not speak of exposure except as connected with the mechanical arrangements for regulating it. The earliest of these we all re- member from experiences at the professional photog- raphers. It is not nearly so much used as it deserves to be. It is the “cap,” or little leather cover that can be removed from and replaced over the lens. Of course it is used practically always in time-exposures, but for these it is most valuable, and often recommended by very skillful workers. Rightly used, it avoids all jarring of the camera, enables one to regulate exposure very accurately, and is simple in use. The usual fault of the amateur being to under-expose, the cap has the advantage of lengthening the exposure a little by the time between the decision to end the exposure and the putting on of the cap. Besides all this, the cap is simple. You cannot help knowing when you take it off and when you put it on. It should be put on and taken off by means of a turning or screwing motion. As to shutters, they should of course work promptly, smoothly, and without jarring. The ideal shutter should expose a plate wholly, during all the time it is open, or at least should expose all parts of the plate With exact equality. There is only one shutter in common use that does this — the “focal plane’” 160 PHOTOGRAPHY FOR YOUNG PEOPLE shutter, the sort that is used in making the very shortest exposures. The focal-plane shutter is put as near the plate- surface as possible, and consists of a long curtain like a window shade, wound on two rollers, top and bottom. In this curtain are one or more slits crosswise, the full width of the plate. If there is one slit, it is adjustable so that it may be either a wide or narrow space. If there are more than one, they are of different sizes. By loosening or tightening the spring that moves the curtain, or by using a wide or a narrow slit, the plate is exposed for a longer or a shorter time. DIAGRAM XX—CURTAIN OF FOCAL-PLANE SHUTTER Suppose the spring so set that the curtain will be pulled across the plate (say, four inches) in 's second. Now suppose the slit in the curtain is 9% inch across. That yá is in front of each bit of the plate successively. There are of an inch in the four inches across the plate, so the slit covers 32 spaces in ſo of a second and each space gets an equal exposure of 330 of a second — from top to bottom of the plate. Again, if the slit moves across in ºn of a second, then each space gets an exposure of rº'ow of a second, and so on. Compare this with a shutter that opens from the centre, and then closes to the centre again, and you will see that the ordinary shutter lights the middle of Courtesy of Motor Photograph MADE WITH A Focal-PLANE Shutter, at Slow Speed (See explanation on page 161) THE CAMERA AND ITS ATTACHMENTS 161 the plate first, and darkens it last — so the edges of the plate are for a much shorter time exposed to light than the middle. Different forms of shutter-leaves have been made to remedy this inequality somewhat, but the only one that does so entirely is ingeniously made so that its four leaves begin their opening at the centre, open into a star-shape, then (turning over on their pivots) close from another part of the circle, so exposing the edges a little longer than the centre, but making the exposure nearly equal all over the plate, and bringing the longer exposure where it is most needed. This is the “Multi-Speed" shutter, and remarkable pictures are said to be secured by its use. It is to be hoped that this shutter will prove to be what is claimed, since the focal-plane shutters are open to the serious defect that the picture secured is made up of strips taken at different instants. Now, suppos- ing a locomotive or an automobile to be photographed by means of the focal-plane shutter, it is clear that the object moves forward a little between the times of taking the top and the bottom of the car, making a slight misfit ; and causing the picture to seem distorted. This effect must always be present to some extent, and in taking pictures of very quickly moving objects it may spoil the picture. Of course, if an object is moving downward or upward, the picture is affected otherwise, and the object is apparently shortened or lengthened as it happens to be moving with the slit or against its motion. So much for the focal-plane shutter, which, though mainly used for very short ex- posures, may also be made so it can be set for all lengths. CHAPTER XV PRACTIOAL HINTS ON EXPOSUIRE Importance of right exposures — The latitude of plates — Practical ways of judging exposure — Time of year and day — Speed of lens — Size of image – Effect of diaphragms — “Catching up ’’ of weaker lights — Effect of over-exposure — Effect of under- exposure — “Expose for the shadows " — General lighting of Subject — Exposure-meters — The system of marking the stops — Adapting exposure to your shutter-speed — How the stop affects depth of focus — Measuring time-exposures — Objects in motion — Exposure tables — A photographer's advice. ENOUGII has been said already, it is hoped, to convince the young reader of the importance of making right exposures. It is so entirely the key to success in photographic work that it comes second only to the choice of subject — hardly to that, for unless you can get a good picture, the selection of the subject is of no use. Consequently you must fix your mind on the question of exposure every time you take a picture, so as to get into the habit of judging exposures correctly. Fortunately you are not required to make a bull's- eye at every shot. The photographic plates have much “latitude,” or range, and may give good results even if you give as much as double the exposure — speaking generally. If you will think the matter over you will see that whenever you take a picture contain- ing variously lighted surfaces, you are making a single exposure do for lights of greatly differing strength; in a landscape, for example, if you take a snap-shot of ºn of a second you give that time both to 162 1PRACTICAL HINTS ON EXPOSURE 163 sunlighted spaces, and spaces in shadow. It is the latitude of the plate that gives good results in both parts of the picture. You will also see that it is the same latitude of the plate that gives good gradation – or wide variety in your lights and darks. Now, plates of medium speed have the most latitude, and give the most gradation, having a thicker coating, and more ability to record different kinds of lighting. In making exposures, then, you have only to get the time generally right — fitting it to the average lighting of your picture (except, of course, in scientific work, copying work, and other such cases where exact results are possible and necessary). The practical way of getting at the right exposures is to do one of two things. Either you must get all the information your can about your plates, camera, and the light, and then follow fixed rules taken from books and directions; or you must learn by practice, keeping a record of your trials under various circum- stances and with various apparatus. A third way — if you “don’t care,” is to guess at it blindly, and trust to hitting the right exposure now and then. But this we do not advise unless you have a long stock of patience and can afford to waste time and material. As to getting information on the subject of ex- posures, and proceeding scientifically, the Italian proverb is a good adviser, “ Chi va piano, va samo; chi va Sano, va lontano,”—“Who goes slowly, goes safely; who goes safely, goes far.” It is the surest method of learning to make your exposures correct, and your pictures good. The things to be determined are five : 1. The light strength. 2. The lens speed. 3. The 164 PHOTOGRAPHY FOR YOUNG PEOPLE plate's speed and latitude. 4. The lighting of the subject in general. 5. The question of motion. The first of these means the value of the light at different times. As to this, it is a matter fixed by the position of the sun in the sky and this depends on the time of year, and time of day. Consequently, it is to be found out from tables regularly printed in photo- graphic books, almanacs, diaries and so on. Such a table is in the chapter of this book given to rules and formulae. Lens-speed is only another way of saying size of the lens-opening compared with its focal length. Focal length is, to be exact, the distance from the “optical centre' of a lens to its “principal focus”: and the principal focus is the point back of your lens where parallel rays coming from outside of the camera meet. But, since the rays coming through your lens from a point a great distance away are pretty nearly parallel, the principal focus of your lens is about at the place where the ground-glass is when you adjust it for objects 100 feet away or more ; and the focal length of your lens, roughly speaking, is the distance from the centre of the lens or from the diaphragm between the lenses to the ground-glass when set for 100 feet away. Other names for focal length are “equivalent focal length,” “ or “equivalent focus.” The word “focus’’ (meaning “principal focus ”) is fre- quently used to mean focal length. The reason why the focal length of a lens affects length of exposure is simply because it affects the distance of the plate from the lens, and so the size of the image and the amount of surface over which the light from any object is spread on the plate. PRACTICAL ELINTS ON EXPOSURE 165 Whatever the size of the image, from any object, the light from that object makes the image. Suppose a square piece of paper, two inclies on a side, to be the thing we are photographing. The image on the plate gets all its light from the rays reflected from those four square inches. If the image is doubled in height on the plate by using a lens of greater focal length, the image is made by the same light spread over a sur- face farther away from the lens and four times as large. Consequently it is one-fourth as strong, and requires four times the exposure. DIAGRAM XXI Diagram XXIV shows this principle. Through b, which represents a card with a round hole in it, pass a certain number of rays from the candle, a. C is a card, say, four inches from a and d a card eight inches from a. The light spot made on d is four times as large and four times as weak as that on c. --> A large camera, say one taking a 5 x 7 plate, has usually a lens of greater focal length than a small one. But you must not think that with a large camera it is necessary to make a longer exposure than with a small camera ! It would be so, if the two lenses were the 166 PHOTOGRAPHY FOR YOUNG PEOPLE same size; but in the large camera the manufacturer puts a larger lens, and usually, a better one, so that the greater distance of the plate from the lens in a large camera is more than made up for by the larger number of rays admitted. But first, the size of the image depends on the focal length of the lens and the distance of the object; secondly, the amount of light admitted depends on the size of the opening. A lens of short focal length makes a small image; a long-focus lens makes a large image, if both are used at their principal focus. For this reason, “wide angle "lenses, which are always of short focus, are used to photograph rooms in which one cannot get far off and yet wishes to get everything in. For objects very much nearer than 100 feet (as in copying, and enlarging), the lens is really used as one of a different focal length. And this becomes important when we consider the effect of the diaphragms or stops on exposure. Since stops are named by their fractional value compared to the focal length of the lens — as f/8, f/12, meaning an opening with a diameter V6 of the focal length, or with a diameter I's of the focal length, when we change the focus at which we use a lens, the stops change in value. This is only important, of course, where the change is large — as usually in taking photographs very near the object, in enlarging, and in copying, where the ground-glass or the plate, is moved far away from the lens. Of course this theory is only to help you in seeing the reason why. The practical thing to remember is that when you make a big image, you are spreading Courtesy of American Photography The EFFEct of Focal LeNoth iN Photography The numbers on the portraits indicate the focal length of the lens used. the 6-inch lens it was necessary to place the camera very near to the subject, hence the great disproportion between the nearer and the farther hand. As the lenses of greater focal length were used, the camera was moved further away, and the dis. With proportion became less. PRACTICAL ELINTS ON EXPOSURE 167 over a larger surface the light that makes the small image — and so must lengthen exposure to make up. And this is true whether you get the big image by bringing your camera near to the object or by using a lens of longer focus — as you do by adding a magnifying portrait lens, or a telephoto lens, both of which merely make your lens equivalent to one of longer focus, and so spread the image. It is, perhaps, a little hard to understand why the image of a near-by object is less strong than that of a farther object. An additional reason why this is so is the fact that for near objects the ground- glass screen is moved farther away from the lens, spreading the image over more surface. You will be helped by referring again to Diagram X, several chap- ters back. The plate's speed, or latitude, of course affects the exposure by the ability of the chemicals in the plate- coating to receive an effect quickly or slowly. If you use rapid plates or films, you can use your lens at smaller openings, or for quicker exposures. Slow plates require the larger openings or longer exposures. Now, the effect of light on a plate is greatest at first (at any given spot), and then lessens because the place already acted on is less and less sensitive. So long ex- posure tends to give the weaker lights time to catch up with the stronger ones. Therefore a plate that can be exposed a longer time will show the effect of more lights of varying strength, than a short-exposure plate will record. If you expose too long, all parts of the plate will tend to arrive at the same state of exposure. If too short an exposure be made, the strong lights will act, 168 PHOTOGRAPHY FOR YOUNG PEOPLE the others will not. Stopping exposure at the right time, you will get the strong lights not too strong, and yet the weaker lights will have a fair chance to catch up, and will have their right relation in the negative. Suppose, as an illustration, your plate was divided into a lot of minute squares, and each square would hold only a given amount of water. Then suppose the light rays to be streams of water of different sizes and speeds. Turning on all these streams together, we may accomplish three results. If we turn them on for a mere instant, a few boxes will be filled by strong streams, some partly filled, others nearly empty. If we keep them turned on too long, all the boxes will be equally full. Neither case will give us a result from which we get a close idea of the amount of water that should go to each box to record the flow in right proportion. We must let the streams run long enough to fill up only the boxes where the strongest streams are, and must shut off the water before the weaker streams can have as much effect as the stronger ones. Over-exposure overflows all the boxes. Under- exposure gives too little to the boxes where streams are small. Right exposure represents fairly all the intensities. Right exposure begins when the weakest light has had time to act on the plate, and ends at the moment when there ceases to be difference between the highest lights and those not quite so bright. You can see that the important matter is to give the duller lights time; the higher lights will cease to act so rapidly before the other lights are through their work. Therefore, it is an old maxim, “Expose for the shadows.” But this does not mean to forget the high PRACTICAL HINTS ON EXPOSURE 169 lights entirely; it means only that they hurt your plate less by a little over-action than the plate suffers from failing to record the duller lights. A quick plate is sensitive, and goes through its whole action rapidly — arriving sooner at the “over- exposed ” state. The slow plate gives more time to the whole process, and having a thicker or richer emulsion, gives the high lights more to do in affecting the chemicals, so that it does not so soon become over- exposed, and the range of action is wider. It is not unlike a long distance foot-race compared to a short dash. Supposing the light rays to be runners, the long distance race will leave them more spread out, and will record their relative speeds more plainly than the short dash. As to the question of the general lighting of the subject, there have been many attempts to classify subjects in regard to length of exposure, and there will be as many as there are authorities. The things to bear in mind chiefly are the colour and the amounts of light and shade. Of colour we have already said much, and we need only remind you that red and yel- low rays mean dark, blue and violet rays, light to the camera. Green in nature is more apt to act as yellow than as blue ; and the difference of lighting between the sky regions and the earth regions, is simply enor- mous. We shall give the usual suggestions as to sub- ject, however, in the chapter for such tables, leaving you to consider them as guides only. Many exposure meters exist, and are especially helpful in training your judgment. They are not exact when based upon the effect of exposure as judged from the turning dark of a piece of printing. 170 PHOTOGRAPHY FOR YOUNG PEOPLE out paper, since the light does not act on the plate just as light acts on the paper. Neither can they be based on transparency of any material as judged by the eye, for vision-light and photographic-light differ. Still they help you to think of all the things that af. fect exposure, and the latitude, or range, of plates helps to make up for their shortcomings. You will find that the exposure-meters give you the right time for a certain stop or diaphragm opening. You have already been told how the diaphragm af- fects the speed of your lens by regulating the light that is admitted through the opening. We must, therefore, consider the stop as a means helping toward right exposure. Luckily, the relation between stops themselves is very simple, the rule being to take the ratio between the stops, and square it to get the increase or decrease of time. That is, twice the diameter across, requires four times the ex- posure. Stops are marked in two systems. One gives the diameter of each stop as a fraction of the focal length of the lens. The usual openings in this system are f/4, f/8, f/12, f/16, f/22, f/32, f/45, f/64. This means that the openings an e V4, 96, ', and so on, of the focus of the lens. Supposing a 6-inch focus lens, the openings would be , , ;", and so on, of an inch, or I }% inch, 34 inch, 9% inch across. Conse- quently, if for the stop f/8 you needed to give (by your meter exposure) 1 second, for f/16 (which is a stop of half the diameter) you would need to give four seconds. All this you will find given in the tables. Ordinarily you will be able to go by your general rule that y4 the opening means 4 times the exposure, or PRACTICAL HINTS ON EXPOSURE 171 twice the opening, 94 the exposure. This is the focal or “f” system. The other system is the “Uniform System,” or “ U. S.” method of marking. This is so marked as to save you from calculating. In this the openings are marked 1, 2, 4, 8, 16, 32 and so on — each number be- ing twice the last, and requiring twice the exposure. The number 1, U. S., corresponds to f/4 in the other ; consequently the f/8 is U. S. 4, and f/12 is (nearly) U. S. 8; and, luckily, f/16 agrees with U. S. 16 — which enables you to compare the two systems with- out a table. You have simply to write down your f / system numbers, and then put U. S. 16 opposite f/16. Then you can calculate the other U. S. num- bers thus: f /4 U. S. 1 f /5 U. S. 2 f / 8 U. S. 4 f / 12 U. S. 8 f /16 U. S. 16 f/22 U. S. 32 The fnumbers you will soon learn, as they are likely to be marked on your stops. But if the U. S. numbers are on you, stops, it will be well to learn what they agree with, for writers on photography constantly refer to the fºsystem. To make short exposures, use the wider stops; to lengthen the time of exposing — as in the blinding light of the seashore, or on the open sea in sunshine, wse the smaller stops, and keep the shutter speed the same. The stops thus help to prevent over-exposure. With a lens good enough to be usable with a wide opening, you may often select a length of exposure to 172 PHOTOGRAPHY FOR YOUNG PEOPLE suit your shutter-speed, since a longer exposure with a small opening has the same effect as a shorter ex- posure with a wide opening. Thus ºn of a second at f/16, has the same effect upon the plate as sºn of a second at f/8 — so far as mere exposure goes. You must remember, however, that using a smaller stop brings more objects into correct focus; and also that motions which sºn at f/8 will catch may be blurred if you expose for ºn second at f/16. All these matters should be thought of whenever you change the diaphragms. In order to make time exposures, either measure them by the second hand of your watch, or learn by a little practice, to count seconds thus: “One and — two, and three, and four.” Try this with watch in hand, and you will soon hit on the right rhythm. Or you may say, “One second, two seconds, three sec- onds " — and so on. As rate of speaking differs you must find out your own rate. Another way is to swing a small pendulum, made of a bullet painted white and attached to a string about ten inches long. This will beat seconds very closely, and you can see it without looking at it directly. As a general rule, give generous time whenever you can do so without spoiling your picture because of moving objects. Learn all about your camera and its lens, so you know what it will do for you when in various kinds of light. There is no attempt made here to go into details, for you will in all doubtful cases be guided by the tables made for the purpose ; but do not forget that tables are made to suit certain stops, and are of little use unless you know at what opening your lens is working. PRACTICAL HINTS ON EXPOSURE 173 The catching of objects when in motion is often a matter of cleverness in the use of the camera. The secret of the whole matter is to suit your exposure to the kind of motion, and also to make the exposure at the right time and from the best point of view. The rapidity with which an image changes place on the plate, depends on how near you are to the object, and upon whether the moving things are in motion at right angles to the direction in which the camera is pointed. If you are near, the image moves fast, and so slower exposures may be made as you are further away. If the motion is directly across the line of the camera, the image moves faster than when motion is nearer in the direction of the pointing. Consequently, to catch a rapid object, get as far from it as you can afford to, and let the camera be pointed somewhat to- ward the direction of motion. Thus, in D i a g r a m XXV, he re, the object moving from A to B takes long er to T- move its im- B D & 2. age across the plate than one moving from C to D. And a to b is a path longer than A to B, while c to d is longer than from C to D. Consequently the shortest exposure is required for the path C to D, the longest may be made on a to b. Then, too, make the exposure just at the slow- ing down point, if there be one, as when an ob- C A. C Če DIAGRAM XXII 174 PHOTOGRAPHY FOR YOUNG PEOPLE ject thrown upward is just changing motion from up to down. A few cents spent for exposure tables, which come in note-books for recording your work, will save you time and trouble in the long run, and will teach you much. But, above all, do not be afraid to try experiments so long as you learn something from each one. The making of creditable photographs is done by thousands of people every where, every day, and this would not be so, if the subject of exposing correctly was an in- soluble mystery. One writer in a photographic magazine says: — “From one-tenth to one-fourth of a second is far more apt to be suitable to average outdoor pictures than one one-hundredth, and to make slow exposures the camera cannot be held in the hand. “It would almost insure success, so far as printing quality may be concerned, if one who knew little of photography used a rapid plate, a rather large stop, and a quarter-second exposure invariably. IIe would certainly obtain far more printable negatives than he would at a fiftieth or a hundredth, and the artistic value would, whether he knew it or not, be greatly enhanced through better definition of distance, better perspective and more truthful representation of what might be doing.” CHAPTER XVI MODERN DEVELOPING The new knowledge — The old way – Hurter and Driffield system — Their method of work — A “good negative '' – How it must be judged — The laws of transparency — The curve of development— Conclusions from it — The four stages in development — Explan- ation of them — Developing to keep the right transparencies — Effect of long developing — The rules resulting from the new knowledge — The factorial system – Effect of temperature — Tank and machine development — The old and new contrasted — Choice of a developer — Need for exactness in new methods. WITHIN four or five years there has been an entire change in the art of developing photographic expo- sures. This has come from new knowledge about the process, and this knowledge is entirely scientific. That is to say, it is the result of study meant to find out in a scientific way just what are the principles and rules by which plates must be treated in order to get the best results. Before these studies were made, each photographer made his own experiments, reported his results, and gave his advice to others. This filled the photographic books and magazines with a lot of receipts, dodges, notions, and suggestions not unlike those to be found to-day in cook-books. The result was to leave both professionals and ama- teurs to grope in the dark. Some did well, others badly; but none were certain. The wise ones with plenty of experience learned to get good negatives 175 - 176 PHOTOGRAPHY FOR YOUNG PEOPLE most of the time by sticking to the same plates, the same developer, and the same general procedure. But this was to go by “rule of thumb,” and often their ideas about the process were all wrong in spite of the fact that their results were good nearly every time. In very truth it may be said that their notions were always wrong, for they believed that development could do many things now known to be impossible. The change came about solely through the wise, pa- tient and able work of two amateurs in photography — an eminent chemist, Dr. Hurter, and Mr. W. C. Driffield, an engineer who was his fellow worker. These men about the year 1890, after some years of careful study succeeded in finding out and setting forth the principles on which the process of development depended. This was no fortunate accident, but the result of a determination to make developing scientific. By exposing and developing plates under known conditions, and by carefully testing the results in each case, they found out the exact rules by which negatives can be produced, and then put the rules in such form that others could understand them, follow them, and secure certain kinds of negatives at will. In brief, they created a science of developing. Although their experiments and discussions are not easy for young readers to follow, the general idea of them is simple enough to be easily known by every user of a camera. Here is a brief statement of the method by which they came to their conclusions. In order to get a good negative, the first thing is to fix in our minds what is meant by those two words. If we think over the question we shall see that we are MODERN DEVELOPING 177 seeking to make a negative containing parts of differ- ent resistances to the passing of light. The whole Ob- ject of a negative is to make a good print. A good print is one in which the lighter and darker parts are lighter or darker just as the lights reflected from the original scene into the camera were lighter and darker. The print must represent the original scene in its gra- dations from lightest to darkest. If it does this fairly and truly, it is a good print. But the print depends upon the negative. So the negative must be such that light (in making the print) must come through lighter and darker portions in the same relations as that light was reflected from the original scene. To put it in other words — the trans- parency of the negative must be in right proportions, in agreement, with the lighting of the original scene. So the whole question is to secure just the right grades of transparency in the negative. So far there is no disagreement with the old notions. But here the dif- ference begins. ~ The old way of judging this transparency was by the eye or by actual trial in making a print. The new way is to inquire “what makes a negative transparent in some places and less so in others?” And to settle this question Hurter and Driffield made their experi- ments, in order to get actual scientific answers, rather than guess work. They proved that the transparency or opacity of any part of a plate (that is its power to let light through) depended on the amount of silver which ex- posure and developing brought theretostay. Then they showed by a long list of accurate experiments the laws by which silver was made in various parts of the plate. 178 PHOTOGRAPHY FOR YOUNG PEOPLE This amount of silver depended upon the length of the exposure to light, so they measured the rate at which the light acted in preparing silver to be dark- / N / \ |/ Jº | * | | | | , | } o 1 2 4 8 16 32 64 &c. up to 524,288 Exposure : Seconds. From the Photo-Miniature, No. 56 DIAGRAM XXIII ened by developing. The amount of silver thus made ready was shown to be governed by an exact law, and this law came from the fact that as the different parts of the plate were acted on by light the amount of sil- MODERN DEVELOPING 179 ver to be acted on became less all the time. Thus, at first, the light has all the silver to act on, then some part of this is changed, thus leaving less, and so on till all the silver has been changed, and no more can be done. As is the custom of modern scientific men, they set this forth in a diagram. They drew a horizontal line, and divided it into lengths to represent time of ex- posure. At the left end of this line they drew another at right angles to represent the effect of the light in changing the silver. Then, by means of their tests with plates, they could show just how much silver was affected at each differing length of exposure. This diagram showed the facts, and from it the effect of exposure could be studied. They made many such diagrams and found that all agreed in certain general features. The points indicating how much silver was affected by each length of exposure were connected by a curved line drawn through them, and this showed to the eye just how the changing of the silver proceeded. If you examine the diagram, you will see that at the starting point, left hand lower corner, there is no time of exposure, and no silver; then the curve seems to rise rapidly, both time and silver increasing. Then the curve rises at a steady even rate that makes it almost a straight line; then it droops, turns, and begins to go downward. This means that the changing of the silver at first proceeds increasingly, then regularly, then lessens, and finally decreases. But this agrees with what was already known — namely, that the effect of exposure is at first too slight, then remains about right for a time, then is overdone, and finally reverses its action. Photog- raphers call these different stages: Under-exposure, 180 PHOTOGRAPHY FOR YOUNG PEOPLE right exposure, over-exposure, and reversal. The curve shows us that the second stage, or right ea posture, is longer than the others, and this enables us to get good negatives if we can only stop before over-exposure be- gins. It is the length of this stage that gives plates latitude. Now let us see if we cannot guess at the reasons for the shape of the curve. At first the light has plenty of silver to act on, and rapidly affects what is on the surface; as it goes deeper the light is obstructed by the particles already acted on, and also has less material to affect ; so it acts more and more slowly until it has been all through the film; then it probably begins to undo its work, causing reversal. It will be noticed that in the diagram the lengths of exposure (marked on the horizontal line at the bot- tom) double at each mark, while the amounts of silver Persity Transparency Opacity Value (on the per- ſ e n dicular 1 DJ fo 1O #. increase 2 [D] ića zoo regularly in- stead of doub- 3 [III] zºo 1,ooo ling. This is made so be- 4 CDIT] Zoº, 10,000 cause the light arza, so orz. works m or e DIAGRAM XXIV a n d m O re slowly, and has to be allowed longer and longer times to do a similar amount of work on the silver. To make the horizontal line represent equal increases of exposure would only flatten and lengthen the curve, without changing its character, or showing a different law of action. MODERN DEVELOPING 181 But since transparency and opacity (the lack of transparency) depend on the amounts of silver, we can now see just what the effect of exposures will be on the transparency of our negatives at each step of the process. And during the time of right exposure, where the silver is affected regularly in proportion to exposure, we see that each time the exposure is doubled, silver is affected by one unit more. If we represent densities by little blocks of which one has such transparency that it lets through I's of the light, then it is easy to see that if one block lets through *, of the light, two blocks will let through I's and then * of that, or rºw of the light. Three blocks will let pass ſº of ſº, of ſº, or rººt of the light (Diagram XXVII). So we see that each increase of a unit of destiny, in- creases the opacity or decreases the transparency in geometrical proportion. This will help in understanding this chapter. Now we have to see how much the transparency of the plate is changed to opacity by this change in the amount of silver. The experiments showed that each time the silver affected by light was increased by one unit, the opacity was doubled, so long as the exposure was kept within that part of its action where the curve is nearly straight — as it is during the “right exposure " period. Practically this means that at first the light acts too much on the plate where the light is strongest, and too little where it is weakest ; then, as the action of the light slows down on the best lighted parts, the others catch up somewhat and act in true proportion for a while, affecting the silver according to their strength. If we shut off the light during this time 182 PHOTOGRAPHY FOR YOUNG PEOPLE the plate is rightly exposed because the silver has been affected in the proportion to the strength of the lights of the image. But if we go on further, the strong lights become weaker in their action, the Weaker lights catch up, and the plate is too equally affected all over — i. e., over-exposed and spoiled. The effect of over-exposure is generally to give the negative (on the print) the appearance of lacking con- trast, having the high lights too gray, and the dark spots not dark enough. Sometimes a negative which you have over-exposed will be thin and transparent, so that you may be deceived into thinking that it has been under-exposed. But the reason that it is thin is because you have under-developed it. Seeing the image flash up quickly and the plate blacken over in the developer, you have probably, as most beginners do, taken the plate out sooner than usual. The de- veloper, therefore, has not got below the surface of the emulsion and its deposit is thin. Such is the general result of the Hurter-Driffield experiments, namely, that there is a time of ea posure during which the strengths of the lights are truly rep- wesented by such changes in the silver compound as to Anake the transparency of the plate, when developed, ovary in right relation to the lights upon it. The next question was the developing of the plate so as to make a negative that would show just the transparencies the lights had given it. The experimenters developed plates that had been un- der-exposed, rightly exposed, and over-exposed. Then they tested the amounts of silver darkened by the de- veloper. It proved that no matter what was done, it was impossible to bring out in a plate any different MODERN DEVELOPING 183 relation of tones than the one governed by the ex- posure made. This they illustrate by supposing three pins put through a piece of elastic. If you stretch the elastic, you change f T I the disuance between | | f the pins, but you do | B ſ lation to one another. | | | C | not change their re- So with developing. f I You will increase or | | decrease the differ- ences between the DIAGRAM XXV various tones, but you will not change their relation to one another. You may make a negative including a wide or a narrow range of tones, but you cannot make wrong relations right. A simple illustration will make this clear to every photographer. If you take a negative and make prints from it, you can make your prints very dark, or very light — but you do not change the relation of the tones toward one another, unless you much under- expose or over-expose and spoil the print entirely. If the negative is a good one, too, there is one right amount of printing to represent the natural scene as truthfully as possible. So in developing. By shorter or longer develop- ment (or by weaker or stronger developer, which is the same thing), we may change the negative from one that is thin to one that is dense, or the opposite; but we cannot change the relation of the tones one to an- other equally all through the series. To put the principles of the new method in a few words: Long development increases contrast, but 184 PHOTOGRAPHY FOR YOUNG PEOPLE contrast only increases till the development has acted entirely through the silver compound, or until “fogging ” begins. Warmth hastens, cold delays de- veloping. Detail in a negative depends entirely on exposure, and the developing cannot bring out more than is there already. After developers begin to act, it is useless to alter them. Slow or fast, they will produce the same re- sult. Restraining a developer is not of any use after detail once begins to show, since it only makes de- velopment slower without making the result different. Long development by making a plate denser may fit it better for certain kinds of printing or for enlarging. Short development may make the plate softer in its contrasts, and thus suit the subject better, or fit it for contact printing. From these conclusions come certain modern ways of developing negatives, all dependent upon the time of developing and the temperature of the developer used. One of these is known as the factorial system. It was devised by Alfred Watkins, and is based on the observation that the time for correct development is always to be found by noting how long, after a plate goes into the developer, it takes to show a trace of the image's appearance. This differs greatly according to the developer used, and the temperature of the solution. But whatever the period may be, the time of complete development is a certain number of these periods. Thus if a trace of the image appears in 18 seconds, and the developer is (say) metol, then if we multiply by 30, we shall have MODERN DEVELOPING 185 30×18–540 seconds as the correct time to develop that negative. This number 30 is metol’s “factor” always. Had we used rodinal (another developer) the factor would have always been 40. If the solutions had been stronger or warmer, the image trace might have shown more quickly; but that changes the total time of development without chang- ing the factor. In other words, by using the factor we need not think of the temperature or strength of developer. These have their effect in changing the time of ap- pearance, and affect the development in that way. On the other hand, in tank or machine developing, we fix the time and the temperature beforehand, and use the developer that is directed. Consequently we do not need to know the factor, which we must know if we do not fix time and temperature. All this comes down to a few simple ideas, which we may easily remember. First, development is a scientific matter that depends on chemical facts. These facts are the exposure, which determines the question of how the negative is to represent the image received ; the developer used, the temperature of the solution, the time for which it is applied. If you use the factor system, you simply need to know how quickly the action of the developer first shows, and then multiply by the factor given to know when to stop. If you use the tank system, you must arrange the time according to the temperature and strength of the developer used, and then apply it to your plates ac- cording to rule. -- If you use the old system, you must keep your eye 186 PHOTOGRAPHY FOR YOUNG PEOPLE on the plate as it develops, and do your best to guess when to stop. And this is not said sneeringly, for it is the plain truth, since by the old methods success was a matter of experience and individual judgment. One regrets that the old way is so difficult, for the pleasure of seeing the images come out was very great, and very educational. But it seems undoubtedly proved that the modern methods produce better nega- tives, whatever the exposures may have been. In fact it is claimed that the uniform developing is best whether you get exposure right or not, bringing out all there is in the negative, and making what there is in it truer to nature's scale of lighting than it can be made by the most solicitous tinkering. As to the choice of a developer, the experts agree that it is merely a matter of whether one prefers a quick or slow development. Pyro, however, gives the negative a slight yellow or brown tinge at times, and thus acts as a stain as well as a developer. Bromide added beforehand, keeps the image from appearing so quickly, but otherwise does not change the result ma- terially. In the factorial system two developers, pyro and amidol have different factors when differently mixed in solutions; but these things are given in the tables. It should be said that not all photographers are ready to accept the new conclusions; but the evidence for and against the theory has been most carefully ex- amined, and the great weight of opinion is in favour of the new as against the old. At all events, young photographers cannot fail to welcome a method that will enable them to secure good results by regular rule, instead of one that says to them, “It is all a mat- MODERN DEVELOPING 187 ter of long experience. Just keep on spoiling plates, and after a while you’ll probably get the hang of the thing.” That was not encouraging to say the least ! The practical ways of applying the new methods are seen in the developing machines and tanks, that are filled with the solution of developer, and then moved to keep the solution in motion for a given time. But one word of warning : If you use the new methods, remember that they are scientific, and you must fol- low the directions as exactly as possible. You must always have fresh developer, a thermometer, and an accurate time-measure. Otherwise you will do better to stick to the old methods where you can keep your eye on your plate. CHAPTER XVII FURTHER REMARKS ON DEVELOPING — AFTER TREATMENT OF NEGATIVES Value of correct methods — Following directions — Rocking in devel- opment — Development without rocking — A few notes on devel- opers — Pyro — Metol – Hydrochinon — Getting familiar with one or two — Fixing safely – How to wash and to dry negatives — The question of varnishing — Defects upon inspection — Weak and strong negatives — Fog — Intensifying and reducing : why not advised — The tabloid system — Local reduction — Retouch- ing — Spotting out — Destroying negatives — Preserving nega- tives. IT must be remembered that the whole purpose of correct methods in development is to get correct neg- atives, truly representing nature. Consequently, if you do not want correct negatives, these methods are to be changed accordingly. Thus, for example, if you wish to copy a line drawing, you will want black lines — great contrast; and you will therefore develop all the contrast possible. Or if you want a figure to stand out against a soft background, you may help that effect by developing the plate in that place locally; in which case you might prefer the old style of developing. But if you know how to develop cor- rectly, it is easier to make these changes since you are working from an exact starting-point. Likewise, you may develop to suit some particular style of printing, or to suit your subject. This can be done by chang- ing the factor in the factorial system, remembering 188 FURTHER REMARKS ON DEVELOPING 189 that long developing increases contrast and gives den- sity, while shorter developing gives softness, and a thin negative that prints more quickly. Every package of supplies — chemicals, plates, papers, and all apparatus – tanks, printing devices, — and the many handbooks — photographic booklets, almanacs, annuals and so on, will supply you with plenty of special advice. The main object of this book is to give such a general understanding of the principles that you will be able to judge for yourself what is important, and to see reasons for the rules given. Naturally enough the makers of plates, films, and chemicals give the best methods for using their own goods; and it is, advised that you note carefully the directions given, even if you find reason for changing them in certain particulars. The manufacturers must give directions that will suit even the most ignorant beginners, and so sometimes err on the side of over- caution. Besides, you will wish to make your own solutions, and so on, or to vary the amounts given ; and this must be done with knowledge. In developing, nearly all the handbooks advise the worker to rock the tray while the plate is in the developer. As a rule this is wise, as it keeps new solution applying to each part of the plate, dislodges any little impurities that might settle on its surface, keeps the developer evenly mixed, and also removes the chemical products of development from the plate surface. Consequently, most workers adopt the rule. But there are advantages in not rocking the tray, if you understand the matter. When light strikes the emulsion on an unexposed plate, which contains 190 PHOTOGRAPHY FOR YOUNG PEOPLE silver-bromide, the compound is broken up, and bromine set free. This bromine in contact with an alkaline developer, forms a bromide again — which is a restrainer of the developer. Rocking the plate mixes the bromide all through the solution. But if the tray be left motionless, the bromide remains where formed, and is most plentiful where the lights are strongest. Consequently it tends to restrain the developing of the higher lights, and thus give the duller lights time to develop more evenly, producing soft negatives. The method used is to put a plate into a very weak developer in a pan, and give a long slow motionless development under a cover that can be raised without jarring the tray — as a big pasteboard box-cover which will not touch the tray, but rest on the table around it. After about half an hour, the plate may be examined in the tray, but must not be moved until development is done. This method is said to make beautifully soft nega- tives, but the developing solution should be highly diluted, as in what is called “stand development,” say with six times the usual amount of water. And this sort of developing is of course expert work. As to the choice of developers, it has already been noticed that modern workers find this really a matter of their convenience. The most frequent developers are pyro, metol, hydrochinon, eikonogen, and less often used are amidol, ortol, tolidol, rodinal. There are so many that only professional treatises attempt to describe them all, and no amateur is likely to use more than a very few of the best known. Pyro, perhaps the one entitled to first place, all FURTHER REMARKS ON DEVELOPING 191 things considered, is a feathery white powder, a strong poison, with a tendency to stain your fingers and your plates a brown shade. The action of pyro, according to the experts, differs greatly according to its strength in solutions, as to which a table is given in the chapter of formulae. Here we will say only that its tendency to stain is prevented by mixing it with sulphite of soda. Pyro, properly managed, Will do almost anything in developing plates, but the impor- tant thing is to be sure to get enough density in your plates by long enough developing. Metol is an excellent developer, with the very serious fault that it poisons the skin of some persons, the effects differing with the person and the con- ditions. Most workers who take pains to keep their fingers clear of the solution will escape unpleasant re- sults, but if you find your fingers are injured by it, it will be wise to choose another developer. Hydrochinon (or hydroquinone) seems to be used most often with other developers. It is often called “quinol,” as in the “metol-quinol” compounds, the well known “M-Q’” tubes containing this. Like pyro, it brings out the surface image quickly, and you should not let this induce you to shorten development for density. The use of metol-quinol is especially recommended by the makers of gaslight and other de- veloping papers, while pyro is very apt to stain, if used for making prints. The best course in regard to the use of developers is to make a choice of one or two, and then study the books about these until you know all its characteris- tics. Now it is well established that the same results, generally speaking, may be obtained from each of 192 PHOTOGRAPHY FOR YOUNG PEOPLE them, and there is no excuse for changing from one to another in the hope of special advantages. By using the same developer under different circumstances you will learn to take advantage of all its good qualities, and to adapt it to your changing needs. But your care with the developing will avail little unless you fix your negatives thoroughly and rightly. Yet the matter of correct fixing is not difficult. With plates, you will use the regular “Hypo ’’ bath (hypo being an abbreviation of “hyposulphite of soda,” for which the right name chemically is sodium thiosulphate), either plain, or made acid by the addition of alum, acetic acid, and sodium sulphite — the last being added to keep the sulphur from being precipitated. The only safe rule is to leave the negative in the hypo bath until all the white disappears, and then as long again. But a few rules will help to make your fixing right. Use fresh hypo, it is very cheap; rinse plates clear of developer before fixing; slight rocking helps fixing; the plain hypo bath becomes discoloured, the acid bath remains clear till exhausted ; keep hypo solution cool; do not let films stick together in the fixing bath. After fixing, wash out all hypo by rinsing and draining your plates over and over, say eight or ten times. The draining is quite as important as the rins- ing. This is done by putting the plate into a tray of clean water for about two minutes, then setting it up to drain while you pour out the water and wash out the tray. Then another two minutes soaking, and another draining, and so on. In running water, the hypo will be washed out thoroughly in from one to two hours. This is a bore, of course, but it is the only Courtesy of American Photography “SUNLIGHT on SURF * - - An effective picture made from a very simple scene. and the lighting give it interest. It is proof that the rule “not to photo- graph against the sun” may often be broken to advantage. ing would have made this a “moonlight” picture. The composition Dark print- FURTHER REMARKS ON DEVELOPING 193 way to be sure your negative will not spoil. Films may be pinned to a board, and floated face downward in a bath. Hypo is heavier than water, and will be removed by its weight. The drying of negatives should be done as quickly as possible without heat, since the grain of the image coarsens slightly by long drying. A current of dry air is the best drier, and an electric-fan is an excellent helper. Do not put drying plates or films too near one another, as this tends to delay drying. Keep them in an even temperature if possible. For artificial drying, plates may be mopped with soft cotton, immersed in alcohol for three or four minutes, and then taken out after the alcohol has replaced the water. Spirit alco- hol is best for this purpose. After the alcohol bath the plate will dry in fifteen or twenty minutes. This method cannot be used for films, and is not so good as ordinary drying for plates, being, as Bayley’s “Com- plete Photographer ” says, not so clean looking. The same authority advises against warnishing nega- tives, as the process is a bother, seldom necessary, and prevents the subsequent working upon the negative to reduce or to intensify it, which may save an otherwise faulty negative. When your negative is dry, you will for the first time be able to know how far successful your work has been. But this can be tested certainly only by making a print, since the eye-judgment of negatives is often somewhat misleading, the trans- parency of the plate to the eye and to the printing light being different things. But certain matters will make themselves evident at once, such defects as clear or dark spots and streaks, mottling and blotches. Most of these come from lack 194 PHOTOGRAPHY FOR YOUNG PEOPLE of cleanliness, such as dust and impurities, and a list of them will be found in the last chapter. General Weakness of the negative may come from under-ex- posure or under-development, or weak lighting may be the cause. Under-exposure is known by lack of detail in the Shadows, or absence of all except highly lighted portions of the picture; under-development by general lack of strength throughout; weak lighting by lack of strength in the highest lights though there is detail in the shadows. But a weak negative with detail in shadows may also be caused by over-ex- posure, with under-development, or development in too cold or too weak a developer. The trouble comes usually from being afraid of developing too long, if the image comes up quickly in the developer, or from being afraid to stop development soon enough if the image has come up slowly. Remember that the same development is best for under, correct, or over-ex- posure. It will in the first case bring out all there is in the plate; in the second case, it is of course right; in the third, it may increase density and make slow- printing negatives, but it will give you the detail and contrast you will otherwise lack. Too much contrast in a negative if not caused by an exposure so short as to give only higher lights, may come from harsh lighting with under-developing, or from short exposure with too long a development, that makes the high lights too dense. Fog, or a general dullness of the negative, may come from too much light in the dark room, from too long a development or too warm a developer— both of which will affect the white edges of the plate as well as the picture; or from light in the camera leaking through FURTHER REMAIRKS ON DEVELOPING 195 some opening, or diffused by a dusty lens, which will not fog these edges. With cleanliness, fresh cool de- veloper, proper lighting in the dark room, a light-tight camera and holders, and correct developing, there should be no sign of fogging. To remedy weakness in a negative, the process called intensification may be used, though no after-process is likely to make a poor negative as good as a good one would have been. There are a number of formulae given, many of them requiring the use of chemicals that are dangerous to handle. The intensifier given by the Seed Dryplate Company is as follows: INTENSIFIER After fixing and washing thoroughly, soak in Mercuric Chloride . . . . . . . . 120 gr. Potassium Bromide . . . . . . 120 gr. Water . . . . . . . . . . . . . 12 oz When the image is white throughout, wash thoroughly and place in Sodium Sulphite, 1 to 8 of water. The darkening action takes place steadily and slowly. Wash fifteen minutes in running water to free from Sulphite. There are also sold preparations for the purpose by various dealers, and it will be best to use these follow. ing directions very carefully because the processes are delicate. When a negative is too dense, the process of “re- ducing” is resorted to, and for this the following formula is given by the Seed Company: REDUCER A. B Water . . . . . . . . . . 1 oz. Water . . . . . . . . . . 32 oz. Red Prussiate of Potash . . 15 gr. Hypo . . . . . . . . . . 1 oz. Add A to B. Immerse plate in solution and watch closely. Action 196 PHOTOGRAPHY FOR YOUNG PEOPLE is best seen when solution is poured over negative in a white tray. Remove plate from solution when reduction is quite complete. After reduction wash thoroughly. - Where contrast is too great, a reducer that will act most strongly upon the higher lights is required. From the same source as the two preceding formulae comes this one : TO REDUCE CONTRASTY NFC ATIVES A Permanganate of Potash . . 24 gr. Water . . . . . . . . 1 oz. B Sulphuric Acid . . . . 24 drops. Water . . . . . . 1 oz. For use 1 dram . . . . . . . . . . . A 2 dram . . . . . . . . . . . B 8 oz. . . . . . . . . . . Water This solution works rapidly, reducing the high lights without ap- parent reduction of shadows. \ Those amateurs who desire to go fully into the sub- ject of intensifying and reducing are advised to get the Photo-Miniature, No. 74, called “Intensifying and Reducing Negatives.” The subject is one requiring more space than can be given to it except in special treatises, especially as the kind of process to be used in any given case depends much on the particular neg- ative. It is rarely that the young photographer will have negatives that are both defective and valuable enough to be worth the trouble of either of these treatments; and the chemicals employed are not such as may be handled carelessly. Perhaps the simplest way of meeting the difficulty will be to use the “Tabloid' chemicals made by Burroughs, Wellcome FURTHER REMARKS ON DEVELOPING 197 & Company, New York City. These come in little hard tablets securely sealed in glass tubes, and after the solutions for intensifying and reducing have been used, they can be thrown away, and the graduate and trays thoroughly rinsed. If a portion of the negative is a little too dense, it can be somewhat reduced by rubbing in a circular mo- tion with a tuft of absorbent cotton — a little box of which costs a few cents at a druggist’s — dipped in alcohol. If the negative is too thin in portions, it is sometimes remediea by attaching a bit of damp tissue paper at the back to the four corners or edges with paste, and then after it is dry strengthening the thin parts by shading lightly with a pencil, or a thin wash of red water-colour, or by “retouching ” on the film- side. To retouch the negative, is an art in itself, but it can do no harm to know enough of the matter to remedy plain defects in your negatives. A retouch- ing varnish may be made by dissolving 60 grains of resin in 2 ounces of oil of turpentine, and a bit of soft rag just touched to this may be gently rubbed on the film where you wish to work. Then with a pencil, very sharply pointed, lightly mark where you wish to increase the density of the negative — or, in other words, to lighten the print. Practice on an old neg- ative first, and be content to remedy the worst faults first, taking up others as you find you have the skill. Transparent spots, “pin-holes,” or scratches on the negative made by care'ess handling, may be remedied by painting them out with one of the various brands of “spotting out ’’ medium, or “opaque’” — a pasty material, usually red in colour. This, of course, makes a white spot on your print; but this is far bet- 198 PHOTOGRAPHY FOR YOUNG PEOPLE ter than a black spot, for you can then, with dilute India ink and a brush, or perhaps with only a pencil, touch up your print so that the spot will not show. With P. O. P. you will not be able to do much by this method, but on gray papers it is very satisfactory ; on prints toned to various colours you have of course to match the colour with paints. It may not be known to every amateur that when you wish to destroy a negative, there is nothing simpler than to put it into very hot water, which will melt the film, and leave clear glass. As to celluloid films, though they can be burned, this should be done very cautiously, a single one at a time, as they burn almost explosively. To keep glass negatives, the best way is to put them into the partitioned boxes made for the purpose. If you do not care to do this, keep them upright in tin cracker boxes, or in the pasteboard boxes in which the plates come. Lay them film-side to film-side with clean bits of wrapping paper between each pair, and in a dry place. Manila envelopes are sold in plate sizes by all dealers in camera supplies, and these are ex- cellent and handy. Examine them now and then, and remove any that may spoil. If a little hypo should crystallize on the surface, and the plate is found in time, it may sometimes be saved by a thorough washing, as at first, and re-drying. With a needle set in a holder, you may scratch at the edge of the film any date or number or inscrip- tion. Film negatives are by far the best for storing away. CHAPTER XVIII PRINTING — METHODS AND PROCESSES The print the final object — Choice of process — Which are perma- nent —Ease of working — Number of processes — What they de- pend on — Silver papers — Plain Salted paper — Albumen-coated papers — Gelatine-coated paper—How they compare — Bromide paper, for prints and enlargements – Gaslight papers — Their fitness for amateur work – Papers that depend on iron salts— Blue prints – Platinotypes — Advantages of the platinum process — The Kallitype — Bichromate papers — The Carbon process — Reversing the image — Gum-bichromate process — The Ozobrome process — Which the amateur is likely to use — Advantage of choosing the simplest — Value of handbooks and photographic periodicals. As the negative does not represent nature, it is only a step to the print, and only good pictorially as it will make a satisfactory print. So, when we have carefully avoided all the rocks and the shoals that surround our course from nature to negative, we have only reached the beginning of another channel, and perhaps one more difficult to navigate — the chan- nel leading from negative to print. But there is a difference. There are many courses leading from negative to prints, and accordingly we have to make a choice among them, a choice that should be largely decided by the sort of negative we have secured, and also by the sort of print we wish to make from it. The two depend somewhat upon one another. Some negatives are better fitted for one kind of paper and process, others that might fail with one 199 200 PHOTOGRAPHY FOR YOUNG PEOPLE paper Will give good prints with another. Yet in general it is true that with a clear, strong negative you may get a good print whatever the process, while a weak negative, though doing better under one proc- ess than another, will require shrewd, skillful hand- ling with any. A question requiring consideration also is that of permanency. If your picture is to be kept for years, you must choose the sort of print that will surely last — and of these there are not an embarrassing number, though most prints if carefully and cleanly made will last for many years. Still another thing to think about is the question of ease and simplicity in working, especially because simple processes are most likely to be carefully and correctly carried out. Even without the minor modifications, there are a dozen ways of making prints, and each has its pur- poses and advantages. This whole chapter could easily be devoted to almost any one of them without exhausting its interest. Consequently we cannot hope to do more than give you a first acquaintance with each, to help you to choose among them. Five of the best known processes make use of silver, three of iron, and the other three of bichromate of potassium. The papers depending for their action on silver con- sist of paper coated with a chloride (or iodide) of silver held in a film of gelatine, of collodion, or in the paper itself. The last of these three, known as plain salted paper or plain silver paper is the earliest of them, and the simplest. It is usually made by the amateur for himself since it is merely a matter of coating the paper (any suitable sort) with solutions of nitrate of silver PRINTING – METHODS AND PROCESSES 201 and chloride of sodium, or ordinary salt. A formula for it will be given in the chapter of processes. If an iodide of silver be made, the paper will need develop- ing. With the chloride of silver, it can be printed readily, and toned with gold or platinum, like the papers bought ready-made. The process is simple, cheap, and said to be reasonably permanent — an ex- cellent process for those who do not live near supply houses. If the same chemicals are used with an albumen (white of egg) coated paper, there is a gain in detail, a glossy instead of a dull or “matt' surface, and the paper keeps better while unprinted. The albumen also keeps the image at the surface, whereas in the plain salted paper it sinks into the fibre. Albumen papers may also be prepared with a dull surface. The old-fashioned family photographs were mostly on albumen papers. The process of making the albumen prints is longer than some more modern methods and has no great advantage, either in brilliancy or keeping qualities. Substituting gelatine for the albumen to give sur- face, but using still the same chloride of silver, we get the modern “printing-out papers” (often abbreviated to P. O. P.), though the Photo-Miniature, No. 7S, tells us that the surface of the paper is first prepared with baryta to give smoothness. If collodion be used for holding the silver chloride, we have another variety the two being “gelatino-chloride,” and “collodio- chloride.” An example of the first is “Solio,” of the second, “Aristo, Jr.” These papers are in general use where fine detail is required, especially in photographs meant for reproduction, as plates, and for taking first 202 PHOTOGRAPHY FOR YOUNG PEOPLE proofs of negatives. In order to be permanent they must be carefully made and thoroughly washed, and even then their lasting may be doubtful, and they are not used where permanency for years is of great mo- ment. Usually glossy, they are also made with the matt surface, and may be toned with gold or platinum so as to give brownish or blackish tones. Bayley in “The Complete Photographer” says, “Al- bumenized paper is practically obsolete. Gelatino- chloride paper must be dealt with at only ordinary temperatures (for fear it will blister or melt). e - With collodion P. O. P. . . . the film is quite insoluble, hot or cold.” Two of the kinds of papers using silver compounds require developing. One of these is “bromide" paper, coated with gelatine — with bromide of silver much like that used in making dry-plates, and needing very similar treatment. Like the plate, bromide paper shows ordinarily no trace of the image until the de- veloper brings it out; and it must be handled in ruby light only except when exposed for printing. In fact, it may be considered a “dry-plate” on paper. It prints not only in contact with the negative, but also is used in making enlargements, the image being pro- jected on it from a lantern or from a camera used as a lantern, or by letting outdoor light pass through an opening and then through a negative so as to project the picture on the paper. There are various methods of developing and toning, so as to give different colours and shades to bromide paper, and the prints (carefully made) are said to be permanent. The other class of developing silver papers is what is known as “gaslight” papers, such as Velox and Photograph by Mr. Henry E. Corke A “ FIRElight " Photograph Made by daylight entering through a low opening. (See note in Appendix.) The portraits of persons light- ing pipes, often seen, are made in a similar way. PRINTING — METHODS AND PROCESSES 203 Cyko. The Photo-Miniature already quoted and an- other of the series call these “washed chloride” pa- pers. “Welox” was the first of them, being invented by Dr. Leo Baekeland in 1894, but the exact process of manufacture is a secret. They are very sensitive to light in printing, and yet can be safely handled in subdued daylight or in artificial yellow light, as if they were very slow dry-plates. This style of paper seems especially suited to the amateur, being simple, con- venient, and being made in many varieties of surface, substance, and style. The prints, rightly made, seem to be permanent as a rule, but this is not absolutely established, since there has hardly been time. Cer- tainly, they are safe enough for all average amateur work, and make a beautiful variety of prints. Three kinds of papers depend for their sensitiveness upon the ferric oxalate — a salt of iron. The best known of these is the “blue-print,” which, except for its colour, would come into universal favour. The result of mere printing and washing is permanent and unchanging, so the prints are most excellent for filing away as records, either of your negatives, or of the facts they contain. A very few subjects suit the colour — sea-pictures, for example; but there is some- thing about the tint that is unpleasant to the eye if seen often or too much at one time. There are methods of changing the colour, but they are said to be uncertain in result and in permanency. Besides, When you make the blue-printing a troublesome, long process, you might better use a better method. The Platinotype is also, at the beginning, an iron paper. The paper is coated with ferric oxalate, and a Salt of platinum. After printing till the image shows 204 PHOTOGRAPHY FOR YOUNG PEOPLE faintly, the paper is treated in a warm solution of Oxalate of potash which causes the image to reduce or deposit the platinum from the platinum salt, giving a platinum image. The Photo-Miniature, No. 78, says: “In simplicity of manipulation, and beauty of result, as well as in permanency, the platinum process is not surpassed by any other printing process known.” The objection to it is its expense. Platinum is a rare metal, and is constantly rising in value because the demand for it in electric arts and for many other pur- poses is increasing. Consequently, while it can be used for good and valuable prints, it is not to be used reck- lessly. Platinum paper, or “platinotype paper,” as it is sometimes called, does not give quite the “snap,” or contrast and sharpness of detail that makes the gas- light papers, such as Velox and Cyko, so popular. Nor is it, in some respects, quite so easy or convenient to print and develop. It has to be printed in daylight, though not in the sun ; and even in the so-called “cold bath" process, the manufacturers recommend one to maintain the temperature of the developer at 60° to 90° Fahrenheit. But if it lacks the contrast of Velox, it possesses a far greater beauty in the richness and softness of its shadows, and in a quality of “depth,” by which we mean that it makes us feel that we are look- Žng into the scene. It records, also, many shadings too delicate to show on other papers, such as light clouds in a sky which on the gaslight papers would appear as a white blank. It has one other advantage — it lies quite flat without curling. It shows at its best in prints larger than 4 x 5 in size, and for portraits is the ideal paper. PRINTING — METHODS AND PROCESSES 205 The paper is usually of a dull surface, but glossy platinum papers are made. The prints are black but are toned to the sepia brown, to red and to blue by various treatments. Some platinum papers may be de- veloped by mere exposure to a jet of steam, a simple and fascinating method. Altogether, the amateur is advised to print his very best negatives carefully upon a platinum paper for preservation, being sure to make the washing in the acid solution thorough, and to use fresh and dry paper. Thin negatives may be used for platinum printing, if printed just right, but the best are those with well- balanced contrast. Those who like fancy tones will find a number of processes for them given in the special handbooks on Platinotypes, but it is doubtful whether any of them are an improvement upon the simple straightforward, black-and-white method of de- velopment. For coloured prints with sure permanency, use the carbon process, and keep the platinotype at its best. 3- The third iron process is that known as Kallitype. It is (or rather was — for it is now seldom used) printed on a paper prepared (usually by the amateur himself, since it does not keep) with ferric oxalate and silver nitrate chiefly. The printing shows an image in yellow, which is developed in various ways, and fixed with hypo. A process for Kallitype recently recommended by James Thomson (Photo-Miniature, No. 69) advises that a good paper (Whatman's or “Scotch linen ledger") be sized with gelatine, sensitized in a solution he gives, and then printed to show deepest shadows only, de- Veloped in a nitrate of silver solution, and fixed in 206 PHOTOGRAPHY FOR YOUNG PEOPLE weak hypo. This is said to give prints equal to platinum ; but the process is more troublesome if cheaper, and also stains the finger-nails. Mr. Bayley, the English photographer, throws doubt on the per- manency of the Kallity pe process in some forms, but it may interest some amateurs. There remain three forms of printing that depend on an entirely different principle — that of the change of a gum treated with bichromate of potash under the action of light from a soluble to an insoluble condition. In these processes paper, or some other substance, is coated with dyed gelatine, then made sensitive by dipping into the bichromate solution, and dried. The paper is then printed under a negative, but shows no image. The light makes the gum insoluble in propor- tion to the lighting. Next, the film on the paper is transferred, reversed, to another support, so the printed surface is beneath. Now, by Washing with warm Water, 105° to 115° Fahrenheit, the gum is melted wherever it is untouched by the light, and least melted where it has been most lighted. The result is to leave more gelatine where the light was strong, less where it was weak — making a print in the coloured gum. The name “carbon ’’ comes from the fact that car- bon (such as the pigment lampblack or India ink) may be used as the pigment to colour the gelatine, and if used makes a perfectly permanent print. The earliest carbon prints were printed from the back through the paper – but in 1864 Sir Joseph Swan devised the method of transferring the film so as to bring it with the unprinted side upward. Of course the print developed with the printed side uppermost would have been melted from its support. The present PRINTING — METHODS AND PROCESSES 207 process makes the whole method simple, if somewhat long. The carbon-tissues, or prepared papers, come in a great variety of colours, either sensitized or not. If sensitized it should be fresh, only a day or two old to be at its best. The sensitizing is not difficult, nor are the other processes, while the results are declared to be unexcelled by any other, if the possibilities are taken into account. Carbon prints may not only be of any colour, but may be transferred to any substance — such as glass, china, wood, metals. If printed from glass negatives they will be reversed, but from films they may be printed so as to come out right, by print- ing through the film back — that is, with the smooth side against the carbon paper. The printing does not give a visible image, but there is considerable latitude, and one may print a negative of the same general density on a printing-out paper at the same time, and this will be a guide to the unseen result on the carbon ; or one may go by some actinometer or light measurer. The so-called Gum-Bichromate process is similar in its principles, but needs no transferring of the print, and the third process — the Ozobrome — is also one of the same sort. But the Ozobrome process is unlike any other in the fact that the prints are made, without light, by putting a bromide or gaslight print into contact with the Ozobrome tissue (of various colours) in a special solution. Then the tissue is devel- oped like a carbon print, either by itself, or on the bromide print. The process is a new one in this coun- try, and seems valuable because it will enable ama- teurs to make large prints on the Ozobrome tissue, simply by making a bromide enlargement from a 208 PHOTOGRAPHY FOR YOUNG PEOPLE small negative. Both allow of much modifying of the print, which recommends them to experienced workers; but they are not likely to be used except by experienced workers. All three of the bichromate processes use a solution that is dangerous to handle except with the utmost care, not only because it is poison taken into the mouth, but also may be absorbed by a cut or sore on the fingers. If used, the worker should remember this, and see that the skin is un- broken, and that the hands and nails are thoroughly cleansed from it. The young photographer will find that the ordinary and best known processes — blue print, printing out and gaslight papers, and the platinotype will give him all the variety he needs, and will also teach him the possibilities of other processes. To master these should be his first task, and when he has learned them, he will have graduated from such a book as this to the special books on each method of printing. It is wisest to learn the few best processes thoroughly before attempting the more unusual; and having learned the simpler methods, the others will be quickly understood. To those named above should next be added the making of bromide prints and enlargements, and then the carbon process — which will make the amateur a well equipped worker. - The making of positives is only the printing of a negative upon a new plate, the new unexposed plate being put into the printing-frame against a negative, precisely as if it were a printing-out paper. Exposure is made to a very weak light, and will be very short, unless special plates meant for making the positives PRINTING — METHODS AND PROCESSES 209 are used. Lantern-slides also are made in the same way. Positives, transparencies, and lantern-slides are all simply prints on sensitive plates instead of paper. Plates specially made for these purposes are usually of slow speed, and directions for exposure come with them. The development is varied also to suit the re- sult desired. In fact, space will not permit our giving here more than the most general rules; nor is it necessary. Un- less we should equip ourselves with knowledge greater than that of all the experts employed by manufac- turers — a task that might puzzle a photographer's congress — we could not do better than to copy for you the directions given by manufacturers and dealers in the printed matter accompanying their wares. This will come to you unsought, and you have only to fol- low intelligently the advice given, never modifying rules unless you understand their purpose. For any special work, such as enlarging, copying, making lan- tern-slides and so on, you will do well to buy the hand- books on your special subject. The cost of them will be repaid many times by the time, labour, and money they will save you. It is also well worth while to take at least one good photographic periodical, so as to know what is doing in the world of photography. The experience of the best workers is given to the world, and nearly all the photographic journals are edited with constant remembrance of the needs of the beginner and the not too skilled amateur. The publishers of such magazines, too, can usually supply you back numbers containing articles on special sub- jects which may have appeared in them, if you write for information on any particular point. Not only for 210 PHOTOGRAPHY FOR YOUNG PEOPLE their special articles on processes are the periodicals of value, but for their advertisements as well, from which you may learn of new contrivances for the assistance of the photographer, new printing papers and plates, on which you will want to keep posted, as improve- ments are always being made. CHAPTER XIX LIGEIT AND ITS ACTION What is light? — How it acts — The ether and its waves — Different effects — Light of the sun — Relation of electricity and light waves—What causes them — Electricity changed to heat and light — Different ether waves, and how they are separated — The prism — The spectrum, how its different parts act — How light rays act on various substances — Chemical effects — Examples in fading or bleaching — Experiments by the old alchemists — Nitrate of silver — Horn-silver — Earliest making of light-prints. WHAT light is we do not certainly know. Its ef- fects are known, and scientific men have studied its action, and the laws that it obeys until they have worked out a theory or guess what light must be. So, though we do not know any exact answer to the ques- tion “What is light P’’ we can say a great deal in reply to the inquiry: “How does light act, and by what laws is it gov- erned P” The idea that is believed to be nearest to the truth may be thus simply put : Throughout all the universe, so far as we know anything of it, there is a something called the “ether.” This is named from a Greek word meaning “air,” since we think of this ether as filling all space much as air is in the space close about our earth that we know best. But the ether is thought to be in every way a finer, lighter, thinner, less gross sub- 211 212 PHOTOGRAPHY FOR YOUNG PEOPLE stance than air ; it is thought to extend through all substances, and to possess remarkable properties. Just as air can be set into motion, and just as it has motions great and small, from the grand rushes of great masses of air which we call the “winds,” down to the smaller motions of air that are caused by sounds which we call “ vibrations,” so there are differ- ent sorts of motion which we believe are caused in the ether when it is disturbed — that is, when a portion of it is moved from its place, pushed, or shaken, or set into vibrations, as water is moved and made to form waves, or air is moved in pulsations. In the ether it is thought that there are set up by disturbances different kinds of motions, some irregu- lar, others regular, just as in the sea we find ripples, regular waves, regular great motions like the tides, and occasional disturbances, like earthquake Waves, for example, which move large bodies of water at a time irregularly. To the regular motions, or waves, believed to be set up in the ether we have given certain names accord- ing to their effects. The effects were known to us long before any one thought of explaining them by imagining ether waves, for those effects are heat, light, and electricity. It is thought that when the waves move in one fashion heat is caused ; when the waves move more quickly, what we know as heat be- comes changed into light; other regular waves cause the effects that we call electricity. These last are very like light waves but are much longer. Nearly all of the work that man does in the world is brought about by causing these movements in the ether. By means of friction or chemicals or fire al- LIGHT AND ITS ACTION 213 ready alight we start heat waves, as in making a fire, or increasing one. We use these heat waves to give us power and motion, as in the steam-engine. We may change this power or motion into electricity by set- ting our steam-engine to turn a dynamo; and then, having caused the form of ether waves known as electricity, we change them, perhaps by putting such a substance as carbon under their action, and so produce that other ether-motion which we know as light, as in the incandescent light. It is an every-day matter to change heat to power, power to motion, motion to electricity, electricity to light, or heat, or power. And by experiment it has been shown that light and electricity obey so many laws in common, that it is believed they are different forms of one action. Light, then, is one of the forms of ether motion. We can, of course, know nothing directly except by our five senses; and since everything comes to us only by sight, hearing, touch, taste, and smell, we can never be certain that there is such a thing as this ether, since it must be changed to motion, heat, light, sound, or electricity, to reach our senses. We do not get at or know the ether except in these forms. But men have found that if they think of the ether as existing they can understand many laws by which it acts; and so can explain and control the action of heat, light, and electricity. Let us accept the idea of the moving ether, then, to explain the action of light. From the sun, from the electric light, from the candle, from the reflected light of the moon, from the firefly, from phosphorus, come ether waves we call “light.” Their speed in moving from point to point 214 PHOTOGRAPHY FOR YOUNG PEOPLE has been measured; the laws of their motion have been studied out. s It is believed that when these motions in the ether proceed in certain wave lengths the effect is what is known as light. According to Clerk Maxwell, when the ether vibrates in from 400,000,000,000 to 700,000,000,000 waves a second, the sensation of “light” is caused. When the waves of ether are from a few hundreds or thousands up to 200,000,000,000 a second we call its action “elec- tricity.” But we must not think these are the only ether waves, since at both ends of the spectrum the effects of others have been traced, and exhaustively studied. Some of the things that may set the ether in motion so as to give out light are chemical action of one substance on another; friction, or a rubbing of one substance against another; and electricity, which consists of ether waves that can be shortened into other waves and thus become waves of light. In the sun, to us the chief source of light, it is thought that there is enormous heat, possibly caused by the contracting of the great mass of the sun into smaller dimen- sions; and that in this heated sphere there is intense chemical action among the gases of which it is made up or which surround it. But whenever the ether waves are of the right length and speed, they take the character of what we know as light waves, and may be recognized either by the eye, or by their effects upon different substances. We have seen how the electric waves, when caused to travel in waves of less length by putting into their way something which retards or shortens them, be- LIGHT AND ITS ACTION 215 come heat or light waves, and are therefore led to think that electricity, light, and heat, are really the same sort of action when at different speeds. There- fore it is not hard to understand that since one kind of waves pass into another kind, as electricity into light, this change from one wave length to another is not always made abruptly or instantly. But there is a succession of waves, each somewhat shorter than the one before, when the wave length is shortening; and also a succession of waves each longer then the preceding one, when the wave length is lengthening, as when light changes to heat. Suppose, for example, we put into an electric-circuit made of copper wire a piece of carbon, which it is harder for the electric waves to go through than through the wire. When they first reach it, the waves are very greatly slowed down, so much that they become heat waves and the piece of carbon be- comes warm to the touch. If the current is strength- ened, or the carbon becomes hotter, the waves get through more easily. As the waves gain a higher rate of speed, the carbon grows hotter and hotter and some of the waves escape into light waves — that is, we say the carbon becomes luminous, or “red hot.” When still further heated, the waves are more rapid, and the carbon becomes white hot. In this state it may begin to combine with the oxygen of the air, or, in simple language, to burn up. In the sun, it is supposed that there are different kinds of action among the heated gases, and that from these different kinds of action come ether waves of various speeds. Each one of the different sorts of ac- tion in the sun is sending off ether waves through 216 PHOTOGRAPHY FOR YOUNG PEOPLE space, and so we should suppose that these ether waves are of different speeds and lengths. Some of the waves are at the right rate to become light waves. But not all these light waves are alike. If, then, we can find out a means of separating one set of light waves from another, we can find out what sorts make up the sun's light. Sir Isaac Newton has done this for us, and shown us how to repeat his ex- periment. Into a dark room he admitted through a small hole a ray of sunlight. In the path of this beam of sun- light he put a three-sided piece of glass known as a prism. This had a thick and a thin edge. In going through the prism the ether waves were interrupted and bent from their paths; that is, they were “re- fracted,” which means bent or broken aside as we have explained in talking of the lens. The waves that travelled quickest were the most bent; those that were going more slowly were the least pushed from their path; and upon a screen were received the different light rays that made up the sunbeam, each striking on a different place according as each was more or less bent from a straight line. Then it was seen that instead of being made up of one kind of light, the sunbeam contained many rays that differed from one another in colour and were spread out in a patch work band in which the eye could see a succession of brilliantly coloured lights in a certain regular order. At one end of this band was a bright violet, at the other end a bright red, and between these, passing delicately one into another, were other coloured bands, making up the following list: red, orange, green, blue, LIGHT AND ITS ACTION 217 indigo, violet. It was also seen that by their direction the colour most changed from a straight path was the violet, while the least turned from its course was the red. In other words, the quickest rays were those that we know by the name violet, and the others were slower in regular order until at the other end of the band, or spectrum, were the slow red rays. It was also easy to show that when these coloured rays were all brought together again, by means of mirrors or prisms, they gave a beam of white light. Once having caused the rays that made up the sun- beam to separate themselves one from another, it was easy to place a screen to stop all but any one of them, and then to see which one of the rays acted most pow- erfully in giving any effect known to be caused by the whole sunbeam. The rays were carefully studied, and it was found that each had its specialty ; that is, pro- duced certain effects of sunshine more than others. Most powerful of all in chemical action were the violet rays, and certain rays that were not visible to the eye, but were beyond the visible violet rays, and were called the ultra-violet rays. For the visible spectrum is not all of it; there are rays at each end, beyond what we see. The study of the spectrum is of course, as you may guess, a whole science in itself; but so far as it has to do with photography the important thing to remem- ber is that the changes with which photography has most to do are caused most intensely by the violet rays and, generally, by all those nearest to that end of the spectrum, and that the weakest rays for photog- raphy are found at the other end of the spectrum, that is, where the red rays are. This, for example, ex- 218 PEIOTOGRAPHY FOR YOUNG PEOPLE plains at once the use of the red glass of the dark- room lamp : it is a substance that lets the red rays pass easily and slows down the other rays of light un- til they too come out as red rays. When the ether waves known as light strike upon different kinds of surfaces, they act in different ways. Some of the rays are reflected; that is, they are turned aside and into a new path, and it is by means of these reflected rays that we see, and it is these reflected rays that come into the camera. Some of them are slowed down so as to be changed from light rays into heat, as is very evident to us where the direct sunshine rests upon any surface. Thus we see that the light rays have two effects which are so easily understood that they have always been noticed. A third effect is so much slower in its action, ordi- narily, that we do not think of it so often nor under- stand it quite so well until it is studied. Still, we all know that if a person, on a bright sunshiny day, is out in a boat exposed to the direct sunlight for some time, he will be aware that the light is brightly visible and that the sun's rays are warm, and he knows also that there will be a third effect produced in time. The sun will change the colour of his skin, darkening it. This is not exactly the same as “sunburn,” which means the redness of the skin coming from the warm- ing effect and from bringing the blood to the surface, but it is what we know as “tan.” This darkening of the skin is the effect of a chemical action of the Sun's rays— that is, of the sun's ether waves — and by chemical action is meant the changing of the nature of substances so that their properties are entirely dif- ferent. YIGHT AND ITS ACTION 219 For example, if we take any given substance, like sugar, and break it, grind it, powder it, dissolve it in water, let it crystallize again into its old shape, and so on, we change its form, but without changing its properties. If, however, we burn a lump of sugar in a closely covered receptacle so that no part of it can escape even in vapour, we shall find that it has been changed in its properties, caused to separate into simpler substances which can then be combined into new things having none of the properties of sugar. This is a chemical change, for burning is only a chem- ical process in which the oxygen of the air is allowed to act upon the other chemical elements that make up whatever in the sugar will unite with oxygen — that is, will burn. Now the action of the sun is of this nature upon some things — it changes them chemically. And it is hardly too much to say that, sooner or later, strong light acts chemically upon all substances, sometimes less, sometimes more. In fact a recent scientific work on photography says that wherever light is absorbed by a body work must have been done on that body — or some change in it caused. We can see this action very quickly upon some dyes, for example, when they have been used in wall-paper. Often it will be found, on moving a picture, that the part of the paper which has been hidden from the more direct action of the light is different in colour from that exposed to the di- rect light. We say that uncovered paper “fades more,” but really this means that there has been a chemical change in the pigment used in staining the paper. Upon some substances this action is very quick, upon others so slow as to be almost imperceptible. 220 PHOTOGRAPHY FOR YOUNG PEOPLE The bleaching of clothes in the sunlight is another example of the sun's chemical action. An old book in speaking of this says that it was for a time thought that this change was the effect of heat, but by putting cloths coloured with a dye that faded quickly in the Sun, into an oven much hotter than the sun's rays it was found that very often no change at all was pro- duced. Another little proof mentioned is the fact that Wax which is whitened by sunlight, darkens when heated. But most of the changes that were noticed in the old times were rather slow. The most important of all these changes is that seen in the leaves of trees, which under the action of sunlight ab- sorb carbonic acid from the air, and then give off Oxygen. Without light this cannot be done. In the case of one metal, however, the action was quick enough to excite men's curiosity. Many years ago, in the beginning of chemistry, it was believed that it might be possible to find a mag- ical substance which would change cheaper and com- moner metals into gold or silver. This caused the old chemists to make many experiments about dissolving gold and silver in acids. Silver would dissolve readily in nitric acid and make a clear and colourless liquid. If, then, this liquid was left alone, it would evaporate or disappear, and would leave behind it white crystals. These were a new chemical form made up from part of the nitric acid and from the silver. These crystals were called “ nitrate of silver.” By making an experiment with this new substance it was found that it would dissolve readily in water, and that anything wet with the solution would, when exposed to light, turn to an intense brown or black. LIGEIT AND ITS ACTION 221 This solution is still used for marking clothing — being called “Indelible Ink’” — which is melted nitrate of silver, having a little gum added to give it sufficient thickness not to “run” in the cloth. Here then was something that quickly darkened when exposed to the light. But the same metal, silver, formed also another compound upon which light would act quickly, and this too was soon discovered. In a German mine there was found a kind of silver ore that when first picked up was nearly colourless and transparent. In fact it was called “horn-silver,” be- cause it looked not unlike clear pieces of horn. When exposed to the sunlight it very rapidly changed to a violet tint, the change occupying only a few minutes. This rapid change in the ore of silver could not but be noticed. When it was seen that light turned nitrate of silver and some other silver compounds to a darker colour, it was but a simple step to place upon paper that had been wet with nitrate of silver solution, objects that would cut off the light from parts of the paper, and in this way leave the paper to be darkened except where they had rested. A leaf, for example, placed flat upon such a piece of prepared paper and out in the sun would keep the nitrate of silver below it from turning dark; and when the paper was taken to a less strong light and the leaf removed, there would be a picture of the leaf's outline in white. But although we shall see that many uses were made of this knowledge, so long as the printed picture could not be left in the light without turning to the same dark all over, the process was of little use. Con- sequently, search began for some way of keeping the 222 PHOTOGRAPHY FOR YOUNG PEOPLE printed pictures from changing ; but for a long time no way of making a lasting difference between the two parts of the paper, the printed and the unprinted, was known. The only way of preserving them was to keep them shut up in portfolios or in dark cup- - boards. CHAPTER XX THE BEGINNINGS OF PHOTOGRAPHY Who invented photography 2–What photography includes—The work of many minds — The camera obscura – Da Porta's account — The chemist Schulze — Experiments on silver compounds — Scheele's researches — Wedgwood and Davy make silver prints in the camera — Niépce makes heliographs – His process — Daguerre joins with Niépce — Story of Daguerre's life — His experiments with Niépce — The use of iodide of silver — Discovery of a means of developing the image — The daguerreotype explained. MR. ALFRED WATKINS, the celebrated photographer and inventor, in a recent address said: “There has been much misdirected inquiry on the question, “Who discovered — or invented — photography P’ Almost as truthfully might it be asked, ‘Who discovered Wind- sor Castle P’ Our present practice of photography has been evolved, like all branches of science and industry, through the labours of countless workers, each adding at least one stone to the edifice of knowledge. Here and there stands out the name of a worker of surpass- ing genius or application who has contributed a founda- tion, a story, or a whole wing to the building ; and in giving due honour to such a name we are apt to forget how dependent he was on the work of others.” This witty and sensible paragraph should be borne in mind by all amateurs in order to prevent their giving too much honour to some of the noted workers in the science and art of photography, while robbing others of their rightful share of fame. Just as the great 223 224 - PHOTOGRAPHY FOR YOUNG PEOPLE castle at Windsor is due to a vast number of workers, so is the process that gives us photographs to-day. Not only is it useless to ask who invented it, but it is equally foolish to ask who made the first photograph. The answer to such questions depends entirely upon what is meant by them. “Photography” means a great many things, and each may be thought of by it- self, or in connection with all its fellows. Each of these things has existed in many forms; and as it ex- ists to-day, it usually is a combination of a number of inventions and discoveries. We can tell, sometimes, what man made the discovery that was the first step toward some part of photography, but that first step was very rarely a complete one. We will suppose that any one of us sets out to take a photograph, and has to begin at the beginning by getting together the things needed. First, then, a camera is bought, whether simple or elaborate, cheap or expensive. This consists of a box, a lens, and ways of exposing plates or films. Secondly, comes the sensitive plates or films. Then, thirdly, there are the developing chemicals, and the apparatus and chemicals for making a print. 'Fourth, there is the apparatus for the dark room — the lantern, the trays and so on. These ready, an exposure is made, the plate de- veloped, fixed, washed, and dried. Then the print is made, finished and handed over — a complete photo- graph. All this proceeding is photography. And before the art could be practiced, there had to be invented the camera, with its devices; the plates, with their chem- ical treatment; the print, with the way of making it lasting. THE BEGINNINGS OF PHOTOGRAPHY 225 No one man invented the whole process. Perhaps the nearest to the inventor of a complete process Was the Frenchman, Daguerre, and yet what he invented was only a very small part of one process. The art of photography grew up by steps, slowly made, gradually set right. First came the camera, then came the ways of getting a clear image into the camera; then the mak- ing of this image lasting ; then a way of making this lasting image so it could be used to print copies of itself. Each one of these steps was an invention, or often the combined inventions and discoveries of many men. So it can be seen that it is hardly fair to call any one or two or three men the inventors of photography, or discoverers of its methods. In a very recent and delightful book on photography," it is told how in tropical countries, where the sunlight is so bright and houses were made with few openings so as to be cool, the people must often have seen from the very earliest times, the forming of pictures in the darkened rooms by a ray of light coming in through a narrow chink. Among the earliest civilized nations, such as the Egyptians, the forming of these pictures must have been noticed ; and so we find in the very oldest authors, descriptions of such appearances. Aris- totle, who seems to have had all the knowledge of his time, and who lived nearly 2,300 years ago, tells us that the spot made by the ray of sunlight coming through a very small hole of any shape is always more or less circular. This any one may prove for himself by cutting square, triangular, or irregular holes in a * Bayley’s “Complete Photographer.” 226 PHOTOGRAPHY FOR YOUNG PEOPLE bit of paper, and letting the sun shine through them. If the holes are not too large, all the spots of sunlight will be round. The lights under a tree, for example, on a sunny day, when the sun is high in the sky, will be seen to be round. Further, Aristotle noted that during an eclipse, when the sun was changed in shape, the spots, too, changed to the shape of the sun at the time, which showed that the spots were images of the sun. Euclid, the geometer, some generations later, used to show how the sun made its own image through a small crevice. Of course, we know that the crevice acted like the pinhole lens, already explained. All this shows that the general idea of the camera was understood in very ancient times; but the first real box or camera made for showing the images was possibly made about fifty years before the dis- covery of America. Next we find an account of such a camera written by the great artist, Leonardo da Vinci. In 1558, however, is found the first clear and exact account of the camera written by an old Italian philosopher. Born about 1543, in Naples, Giovanni Battista della Porta from his youth up devoted him- self to philosophy, to experiment, to publishing what science he could gather, and, strangely enough, also to the writing of plays. At the age of twenty-six he published a book in which, among other things, he described the camera obscura, saying that if a small opening is made in the shutter of a dark room, images of external objects—that is, of the view — will be shown on the opposite wall in their true colours. And he further adds that if a convex lens (a lens thick in the middle and thin at the edges) be put in the opening and the image is received on a surface at the right THE BEGINNINGS OF PHOTOGRAPHY 227 distance from the lens, the picture will be made so clear that a person standing on the outside of the window may be known in the image. But the using of a lens in this way had already been told about by another writer. Porta made an apparatus for showing these images, and he also pointed out that the eye is such a camera obscura, though he seemed to think that the images were formed on the pupil instead of at the back of the eye as we know them to be. It would hardly seem from this that Porta invented the instrument. It may be well here to remind the reader that camera obscura is only Italian for “dark room.” The image shown by the camera was upside down, and this had led very early to the adding of a mirror so inclined that the images could be viewed right side up. When the device had been improved, it was ar- ranged so that it consisted of a dark room, on top of which was a revolving opening that could be turned toward any direction of the view. In this opening was a lens that made the image clearer and brighter and sent it to be received upon a table placed in a room below, where it could be conveniently viewed. It will be seen that by putting a flat white surface such as a piece of paper, upon a table, the scene would be received upon this and could be copied at leisure by an artist. It was not an uncommon thing before the improvement of photography, to build these camera observatories upon points that afforded a good view of the surrounding country, and it was a popular amuse- ment to observe from within the scenes that came through the lens. The idea of using these images as a help to drawing 228 PHOTOGRAPHY FOR YOUNG PEOPLE came to many, and artists and astronomers found the camera image a great help in sketching. The camera, with its lens, was carefully studied, and was well un- derstood long before there was any idea that the pic- tures made by it could be made lasting. So we may say that the camera was ready for use as soon as the chemists found out how to make it take pictures. The principles of the action of the camera obscura were set forth in full by the great astronomer Kepler, and there were many forms of the apparatus, some for use, oth- ers for mere amusement. It was also known at a very early date that the human eye was a camera, receiving inhages in the same way, and governed by the same principles. All this was known before there had been any step toward making the camera images perma- nent, though some fanciful writers had suggested the possibility of doing this. In telling of the effects of light, we have spoken of the discovery of horn-silver, and of the sensitiveness to light of certain silver compounds. The nitrate of silver may have been known to the Egyptians, and was described in the seventh or eighth century by an Arabian chemist, who speaks also of certain dyes or pigments made from silver. The first mention of sil- ver as producing dark stains was in 1546, by George Bauer, who also says that a certain silver ore changes to a darker tint. But the earliest statement that horn- silver darkens, is in a book by Fachs, in 1567, and there is no clear understanding of the cause until the work of Schulze. The first chemist to make sure that it was light that darkened the silver was Johann IIeinrich Schulze. He accidentally mixed nitric acid in which a little sil- THE BEGINNINGS OF PHOTOGRAPHY 229 ver had been dissolved, with chalk, and noticed while working by a window that the compound darkened to a purplish red where the sunshine rested on it, and only there. Following up this hint, he put the same mixture into bottles, and covering them with paper in which openings were made, he was able to print the shape of the openings upon the contents of the bottle. He also proved by a series of experiments that it was the silver that caused the change. He published his experiment in 1727, and Mr. Bay- ley thinks that the later English experimenter, Wedg- wood, got his suggestions indirectly from Schulze's account, through another Englishman, Dr. William Lewis. Lewis made many experiments with the silver nitrate, showing how it was darkened by light, and also with other chemicals. Dr. Lewis's experiments were told of in a book published in 1763. Before this, in 1757, the Italian chemist, Beccari, had studied the chloride of silver, and proved its darkening to be due to light. Nine years later than Lewis's book appeared a work on “Discoveries relating to Light, Vision and Colour,” by Dr. Joseph Priestley, describing Schulze's discoveries, and mentioning also those of Beccari, and Lewis's book; and only a short time before (1770), John Dollond, an English optician, had explained how it was possible to make an achromatic lens — a discovery made by Chester More Hall, an astronomer, some time earlier, and one that was to prove most essential in photography. Another step was taken by Carl Wilhelm Scheele. About the time when the Revolution broke out in America, this German chemist became much interested in the action of light upon horn-silver, and following 230 PHOTOGRAPHY FOR YOUNG PEOPLE Beccari, he made a great many experiments to find Out not only how sunlight acted upon this substance, the chemical name of which is chloride of silver, but also he tried the effects of the different parts of the spectrum upon the chloride to see which one acted most rapidly. - There is little to record about this chemist's life ex- cept the appearance every now and then of deep treatises written by him and telling the results of his experiments. There is, in the encyclopedias, a long list of valuable facts he learned in his quiet life in the laboratory. To him is due the proof that air consists of two gases, the invention of a valuable dye, the ex- plaining of the souring of milk, and the discovering of glycerine. Not only did he discover numberless things, but in each case he studied completely the ac- tion of each body he discovered. - In short, he was a great genius, who, in a brief life, made discoveries of priceless value to mankind. He was the first to find out that the rays most powerful in blackening silver were the violet rays. Such inves- tigations were carried still further by other chemists, and it was not many years before it had been shown that nothing seemed to have the same quick sensitive- ness to the action of light possessed by silver or its various compounds. We cannot note the various dis- coveries, but will record that in 1800 and 1801 Sir William Herschel discovered heat rays beyond the red rays, and J. Ritter discovered the invisible rays beyond the violet, and proved their action on silver salts. There is a claim that about 1780 a French professor named Charles made silhouette profiles by casting the shadows of his pupils' heads on paper prepared with THE BEGINNINGS OF PHOTOGRAPHY 231 chloride of silver; yet the evidence is very slight; and there is also a statement that Lord Brougham sent to the English Royal Society in 1795 a paper suggesting that ivory rubbed with nitrate of silver might retain camera images, but neither of these ideas led to any practical result — which is the important matter. During the years when these investigations were carried on, there was in England a number of friends interested in such discoveries, and often meeting and corresponding. Dr. Priestley, the discoverer of oxy- gen, and author of the book on “Discoveries relating to Light,” was one of them ; the father of Charles Darwin (whose brother married a daughter of Josiah Wedgwood) was another; James Watt, inventor of the steam-engine, and Josiah Wedgwood, the famous maker of pottery, were also included in it. Mr. Bay- ley tells us that a former assistant to Dr. Lewis came as secretary into the service of Wedgwood, and was employed partly in educating Thomas Wedgwood, his son. This was Alexander Chicholm (or Chisholm, or Chisolm). Undoubtedly this assistant knew of Lewis's experi- ments with nitrate of silver, having been thirty years in Lewis's service, and through him Wedgwood (Thomas) became acquainted with its properties, and began to experiment with it. It is hardly to be doubted that Tom Wedgwood also knew of Priestley's work, since his father was a subscriber to it, and Tom corresponded with Dr. Priestley. About 1802 came out a paper by Thomas Wedgwood with notes by Sir Humphry Davy, then an assistant lecturer in the Royal Institution. This paper told how to copy paintings on glass, and to make profiles by 232 PHOTOGRAPHY FOR YOUNG PEOPLE the “agency of light upon nitrate of silver.” In this paper Wedgwood claimed the invention of the method. What he had really done was to combine the knowl- edge that nitrate and chloride of silver would darken in the light, with the use of the lens and the prism, as told about in the works of Priestley and others. It was natural that those who knew the beauty of the little images formed in the camera, and who knew that light could print the outlines of objects laid upon paper wet with nitrate of silver, should see what beautiful results could be secured if the images made by the camera obscura could be caused to print them- selves upon paper, and thus save the artist his trouble in copying the scenes the camera showed. But at first Wedgwood did not make much progress in this. Thomas Wedgwood soaked paper or white leather in the nitrate of silver solution, and then printed upon it images of ferns or pictures in outline. Davy, in his notes, remarks: “Nothing but a method of preventing the unshaded parts of the delineation from being col- oured by exposure to the day is wanting to render the process as useful as it is elegant.” In making his experiments Wedgwood had tried also to fix upon his prepared paper or leather the images made in the camera obscura; but though he was able to get traces of the light's action, it was only by making very long exposures, and even then the traces were faint and showed probably only the bright- est lights. When the same experiment was tried with images cast by the sun through microscopic objects, and thence through a microscope upon prepared paper or white leather, better success was met with, probably TEIE BEGINNINGS OF PHOTOGRAPHY 233 because the light was more concentrated. But the experimenters had no very great success, and could not preserve the images except in the dark, though they tried by prolonged washing to leave only the blackened or metallic silver in the paper. Conse- quently until more knowledge was gained, little could be gained. Meanwhile, others were likewise working on the same problems, though they did not always approach them from the same direction. The next step in ad- vance was taken in trying to improve upon certain printing processes in lithography — which is the method whereby a drawing made on soft stone can be used to make prints in ink. The next noted experimenter was Joseph Niépce, a Frenchman, born in 1765. He became interested when about forty-eight years old (1813) in lithography, mainly with the idea of reproducing certain line-en- gravings. In order to save himself the trouble of copying these, he tried to make them transparent by oiling or warnishing them, and putting them upon metal plates covered with different substances, in the hope that the light shining through the transparent engravings would print an image that afterward could be engraved by the use of acid. He seems to have tried a great number of different substances, including some silver compounds, but was most successful with a kind of resin. This was bitumen, or asphalt, which he spread on polished metal plates. Exposed to the light under an engraving or drawing, this bitumen was so affected that where the light had acted the bitumen was hard to dissolve, while the parts protected by the lines of the engraving could be dis- 234 PHOTOGRAPHY FOR YOUNG PEOPLE Solved away by the use of a chemical — the oil of lavender. When a plate so covered with bitumen had been ex- posed to the light and then had been put into the oil of lavender, those parts of the plate that had been struck by the light were still covered by the bitumen, and therefore looked brown, while the parts protected by the lines of the drawing had been dissolved away by the oil of lavender and so the lighter metal showed through. Thus he had made a plate on which the original drawing was reversed in colour, black lines showing white, white places showing brown. It was not a quick process, since even in direct sun- light the printing time was from four to six hours; and when the same process was tried in order to fix the images of the camera obscura, the necessary time of printing was immensely increased. When once he had succeeded in getting these re- versed pictures, he tried all sorts of experiments with them, among other things putting them in acid which bit into the plate where the bitumen did not protect it, making a sort of an etching, or engraving, in which the white lines were changed to lines engraved upon the metal. These plates when engraved, after the bitumen had been removed entirely (which could be done easily by heat, or friction) could be used to print from exactly like plates cut with lines by an engraver. One of these plates still exists, and a print of it is reproduced in the Photo-Mānºature for March, 1904. Niépce also used his processes in attempts to fix the image in the camera obscura, using paper to receive the image. It is also said that he used chloride of sil- THE BEGINNINGS OF PHOTOGRAPHY 235 wer in certain of his experiments; but the process he brought to the most successful results was that with , the bitumen on metal plates, either by direct printing or in the camera. And the same general method is to-day in use for modern photo-engraving, and a similar one in making carbon prints. - * In writing an account of his process for an English friend, Niépce mentions that he is indebted to a certain M. Daguerre, of Paris, for the suggestion that glass could be used instead of metal, and that the lines etched on glass could be filled with ink, causing the drawing to be visible when the glass plate was backed with white paper. Louis Daguerre was a painter living about nine miles from Paris, a scientific man “much esteemed for his goodness and geniality of character,” as an old writer puts it. Daguerre was born about ten miles from Paris in 1787. His father was crier to the local court in Cormeilles, his mother a villager. The boy was educated in the public schools, and had a strong taste for drawing. He went into an architect's office, and learned to make tracings, but in 1803 entered the shop of a scene painter. He was engaged to make panorama paintings, and invented or planned a Diorama, a circular building around which pictures were shown to spectators on a turning platform. He introduced the idea of lighting these pictures from the front, and then from the back — so as to bring a new picture to view by looking through the first. He also showed his own paintings in art exhibitions. It was in 1824 that he began his experiments with the camera, using chloride and nitrate of silver, as Wedgwood had done. Two years later he began to 236 PHOTOGRAPHY FOR YOUNG PEOPLE Work with Niépce, and went into partnership with him in 1829. An old book on “The Camera and the Pencil,” by M. A. Root, tells how, in 1825, at the end of a lecture by a distinguished French chemist, a lady came to ask a question, saying, “I am the wife of Daguerre, the painter. For some time he has let the idea seize him that he can fix the image of the camera. Do you think it possible P. He is always at the thought, as he can't sleep at night for it. I am afraid he is out of his mind. Do you, as a man of science, think that it can ever be done, or is he mad?” The great chemist, Dumas, said: “In the pres- ent state of knowledge it cannot be done, but I cannot say that it will always remain impossible, nor set the man who seeks to do it down as mad.” As this was fourteen years before Daguerre's process was pub- lished, Root well says that it gives us some idea of what the discovery cost him. These two investigators, Niépce and Daguerre, used, among other things, iodine to darken the surface of their plates. By letting the vapour of iodine — a substance first extracted from the ashes of seaweeds, discovered by Courtois, and investigated by Humphry Davy (who reported Wedgwood's work and assisted in it) — act upon the surface of a silver plate, a com- pound formed of the iodine and silver was left upon the surface of the plate. Like other silver com- pounds, this was sensitive to light after a long ex- posure, far too long to make portraiture possible. But, owing to a most remarkable accident, Daguerre made a discovery that at once gave him a quick proc- ess by which visible images could be formed upon Courtesy of T. M'. Smillie, U. S. National Museum * . .” -- - - Monument to DAGurr R.E. In the grounds of the National Museum, Washington, D. C. TEIE BEGINNINGS OF PHOTOGRAPHY 237 the iodide. Daguerre had been exposing some silver plates coated with the iodide, but had not made long enough exposures to get an image he could see. He put the plates away in a closet where he kept chemic- als, and upon examining them at a later time was astonished to find that both showed a visible image. This, he reasoned, must have been caused by Some of the chemicals in the closet; and with the ingenuity of a genius he patiently went to work to find out which chemical had caused the images to appear. One after another he took out of the closet a chemical at a time, putting a fresh plate like the first into the closet after each time a chemical was re- moved ; but when be thought he had taken out all the chemical substances he found that visible images were still produced. At length he discovered upon the floor a dish hold- ing quicksilver, which he had hitherto overlooked. Knowing that quicksilver is very ready to evaporate, giving off vapour even when slightly warm, he tried the experiment of allowing the vapour of the slightly warmed quicksilver to rise against the surface of the silver plate coated with iodide. “To his intense de- light,” says Dr. Vogel in his “Chemistry of Light and Photography,” “an image appeared, and the world was enriched by one of its most beautiful dis- coveries.” This process discovered by Daguerre consisted, as will be seen, of the following steps: A polished silver plate was “fumed,” that is, exposed to the vapour of iodine. The vapour made with the surface of the silver a chemical union, producing the chemical substance, iodide of silver. This iodide is sensitive to 238 PHOTOGRAPHY FOR YOUNG PEOPLE light. On being exposed to the light, say in a camera, no image is at first seen; but if the plate be then placed over a dish of mercury, and the mercury slightly warmed so as to give off a vapour, the mercury particles combine with the iodide of silver more or less as the iodide has been more or less acted on by the light, and so produce a darkened image made up of the combining of the mercury with the iodide. Fortunately for Daguerre, there had been dis- covered before this time at least two-chemicals that would wash out of the plate those silver compounds that had not been affected by the light, without dis- turbing the parts that had been so affected. When the unaffected silver was washed out, of course the pictures could be exposed to daylight without injury. Of these substances we shall say something in the next chapter. We must also reserve for that chapter an account of the work of Fox-Talbot, whose re- searches and inventions led most directly to modern ways of making photographs. CHAPTER XXI FROM THE DAGUERREOTYPE TO THE DRY PLATE Seeking to fix the images — Daguerre uses salt – Herschel dis- covers hyposulphite of soda to be the best fixer — Objection to the daguerreotype — Morse and Draper work together in America – Fox-Talbot's invention — He makes real silver prints from nega- tives — Draper's work — He uses the “chemical focus ” — The first portrait — Summary of the work of invention — Niépce St. Victor introduces albumen — The use of collodion — Scott- Archer's wet collodion process — The seeking for a dry process — Dr. Taupenot's gelatine plate — Bennett heats the emulsions — Dr. Maddox's gelatine plate — The making of emulsion— Monckhoven adds ammonia — “Modern photography ’’ begins — The Petzval lens — Dr. Vogel. To make the nitrate of silver prints last, Sir Humphry Davy and Wedgwood tried long washing in water, but without success. Niépce, on the other hand, had found a way of making sun-prints that would last, but these were his bitumen plates. He could not fix his silver prints. Daguerre was the first to find a solution that would “fix” silver prints by washing away the parts not made insoluble by light. IIe used a solution of ordinary salt — chloride of sodium. In 1839, Sir John Herschel, the English astronomer and chemist — who lived until 1871 — showed that hyposulphite of sodium was a far better solvent, and Daguerre at once adopted this substance, which has been used ever since. It was discovered in 1799 by 239 240 PHOTOGRAPHY FOR YOUNG PEOPLE Chaussier, and Herschel had described its effect on the silver compounds in 1819. The Daguerreotypes were very beautiful pictures even from the first, and the process was rapidly im- proved. The improvements were needed. For after the first Wonder and delight over the new process, serious ob- jections to it appeared. The pictures were very deli- cate, being ruined by the slightest touch, and if ex- posed to the air they soon were spoiled. A chemical treatment due to a Frenchman named Fizeau made them more permanent. A mixture of hypo and of chloride of gold was poured upon them and evap- orated by heat. This left the gold on the image, mak- ing it both clearer and more lasting. Put under glass, and viewed at the right angle, the pictures were beautiful as works of photography, but the long exposure necessary caused portraits to be un- satisfactory. In his “House of the Seven Gables,” Nathaniel Hawthorne points out the defects, saying that the faces were “hard or stern '' and the sitters “conscious of looking unamiable.” This in view of the twenty minutes' exposure sometimes required does not seem unnatural. The cost of the pictures was ex- cessive — from five dollars up to twenty-four, the lat- ter price being charged for Daguerre's own work. But many workers helped to improve the processes. Dr. Goddard, of Philadelphia, and another Goddard, an Englishman, both treated the plates with bromine fumes, and a Frenchman, Claudet, used chlorine ; both these treatments made the plates more sensitive, and reduced the necessary exposure to from five minutes to one minute — or even less in the best light. Yet FROM DAGUERREOTYPE TO DFY PLATE 241 even at this time — 1840 and 1841, the very long ex- posures were often necessary where lenses were im- perfect or conditions were unfavourable. Daguerre's process had been made public early in January, 1839, in return for a pension of 6,000 francs ($1,200) to Daguerre and 4,000 to the younger Niépce. But in 1839, Professor Morse (of telegraph fame) had visited Daguerre and seen some of his pictures. Re- turning to America, Morse met with Professor John W. Draper, who had for many years been interested in the study of light and its chemical effects — using chemically prepared or “sensitive ’’ paper for the pur- pose. Draper had repeated the experiments of Wedg- wood and Davy, and had especially studied the work of Fox-Talbot, an Englishman whose researches upon photography had been carried on several years before Daguerre's process was published. Talbot was an amateur, born in 1800, and died in 1877. He was educated at Harrow, and Trinity College, and being rich could afford to give his time wholly to the scien- tific studies that interested him, and in them he spent his life. Talbot's experiments began in 1834, but he had not published his work when Daguerre's invention was announced. Three weeks after this announcement, Faraday showed some of Talbot's prints, and on Jan- uary 31, 1839, Fox-Talbot read a full account of his process before the London Royal Society. Talbot made prints on paper, ſirst salted and then soaked with nitrate of silver, and fixed them in iodide of potassium and salt. He also devised a method of de- veloping — possibly taking the general idea from Da- guerre — by using gallic acid. This process was 242 PHOTOGRAPHY FOR YOUNG PEOPLE finally known as “Talbotype,” though patented as the “Calotype ’’ process. It was rapid as compared with the Daguerreotype, and was also a means of making prints, rather than a positive picture. Professor Draper repeated Talbot's experiments, and tried to shorten exposures by usi, ºnses of wide aperture and short focus, and in 18.9 he learned of and tried Daguerre's process with success on buildings and other outdoor objects. Then, with a lens of five inches diameter and seven inches focus, he attempted a portrait — dusting the sitter's face with flour, and arranging his camera so that the plate would be at the chemical focus of the rays. After certain fail- ures, he succeeded in photographing a sitter— mak- ing the first photographs of a human being from life. At this time the Daguerreotype process was used for making landscape and still-life pictures and required from twenty to twenty-five minutes' exposure. Pro- fessor Morse was at work during the same time, and declares that he cannot say whether “he [Draper] or myself took the first portrait.” After a while they worked together, Morse, as an artist, taking especially the artistic side of the work, and charging his sit- ters for the portraits. There are other claims as to the earliest photo- graphic portraits, but the weight of evidence seems to favour that of Professor Draper. To sum up a little, now that we have reached the first portraiture, we may remember that the achro- matic lens — a necessary step — came from Hall and Dollond ; Wedgwood printed with nitrate of silver in the camera ; Daguerre found out the printing with iodide on a silver plate, and developing with mercury FROM DAGUERREOTYPE TO DEY PLATE 243 and fixing with salt; Fox-Talbot printed on paper with silver salts, developed with gallic acid and made negatives ; Herschel taught the fixing of the image with hyposulphite; Draper probably made the first portrait. But it should he said also that the developing with nutgalls (gallic acid) is due to Reade, an English clergyman, who published a method in 1839, and that Fizeau and the Goddards used the chlorides and bromides of silver to make plates more sensitive. To Herschel is due the use of the terms “positive ’’ and “negative.” About this time also, 1844, a worker named Claudet suggested the use of red or yellow light in the working room to prevent spoiling the plates. So great were the advances that had been made in the years from 1839 to 1850. In 1851 came a process that really gave the begin- nings of the marvellous modern photography. The Talbotype had been printed through paper, and often showed the paper's grain ; and this led to waxing it to make it more transparent. Herschel had suggested the use of glass-plates, but his method did not prove prac- tical, until a relative of Niépce, Niépce de St.Victor, saw the need of some substance to hold the silver salts to the plate, and introduced in 1847 the use of albumen and starch for that purpose. His process was pub- lished the next year, and improved and extended by two other Frenchmen — Blanquart-Evrard using paper coated with the albumen for printings, and Le Gray using collodion (a solution of pyroxyline, a kind of gun-cotton) to replace the albumen in the plates. The inventor of collodion was a Boston medical student, John Parker Maynard, who in 184S advised its use as 244 PHOTOGRAPHY FOR YOUNG PEOPLE a medical plaster, and gave the substance its name from the Greek word “kolla,” glue. Then an English- man, Scott-Archer, made the collodion process certain and practical. He was a sculptor, and studied photography to pre- Serve records of his work. Between 1847 and 1850 he tried the calotype and the daguerreotype, but soon improved on these processes by using collodion and his methods soon took the place of both. Archer's method was to dissolve cotton-wool in nitric and sul- phuric acids, making “pyroxyline.” This was washed and dissolved in ether and alcohol, making collodion. To this was added iodide of potassium and potassium bromide, and the mixture poured on a glass-plate and allowed to set. The plate is then sensitized in silver nitrate, put into a holder (still wet) and exposed in the camera for “from one moment to a quarter of an hour.” It was developed in gallic acid, acetic acid, and water, and fixed in hypo. This is the “wet collodion ” or wet-plate process. It gave most delicate and beautiful negatives, or if preferred a positive could be had by making a short exposure, and whitening the negative in bichloride of mercury. The plate so treated was then backed by a black background, and gave an effect like the daguer- reotype, but more lasting and very much cheaper. When such a picture was covered by another glass plate, the “ambrotype" was formed,— a kind of pic- ture very well known years ago, say from 1854 to 1807. The wet-plate process is still used in making plates for lantern-slides, delicate negatives for reproduction, and wherever the finest detail is needed, as in astro- nomical work or scientific photography. The claim is FROM DAGUERREOTYPE TO DFY PLATE 245 made that it still produces the most beautiful of nega- tives. But though the wet-plate process may be looked upon as the first step in modern photography, it was not convenient to have the silver-bath always ready. Consequently many efforts were made to unite the silver with the collodion coating, and then to dry the plates without their losing sensitiveness. A French- man, Dr. Taupenot, was the first to succeed, though many improvements designed to keep the plates moist were tried before the really dry-plate was devised. Taupenot coated the sensitive plate with albumen, dipped it in silver nitrate, and found that the dried plate would keep its sensitiveness for six weeks or two months. To this process the main objection was the plates required about six times the exposure of the wet plates. There were many preservatives suggested, — such as sugar, beer, pyrogallic acid, but it is not necessary to describe the many processes, for the im- provement that was to be most successful took another course. This was the making of an “emulsion ” — a mixture containing all the chemicals and substances necessary to coat the plate. Many tried, but the earliest to succeed were Sayce and Bolton, of Liver- pool, who formed an emulsion containing bromide or iodide of silver, which was quickly so improved as to become most valuable. This was early in the sixties, and they used a collodion mixture. Then in 1871 a Dr. Maddox substituted gelatine for collodion, and thus introduced the gelatino-bromide process, and this proved to be a great advance though it required the efforts of a number of workers to find out just What was needed to make perfect dry-plates. 246 PHOTOGRAPHY FOR YOUNG PEOPLE Harrison, in his “History of Photography ’’ says that in an exhibition of photographs held in 1876–7 in Edinburgh, 709 exhibitors used the wet-plate and 105 the dry-plate process. In 1878, however, Charles Bennet, an amateur, showed gelatine negatives in Lon- don which were so good and produced by so short an exposure that he was asked to explain his method. He published his process, and showed that his results came from having heated the emulsion from two to seven days, which greatly increased its sensitiveness to light. Then another worker, Stuart Wortley, shortened the time and increased the temperature; George Mansfield boiled part of the emulsion for ten minutes, and then added the rest. Still another, Dr. Monckhoven, added ammonia to the emulsion and gained the sensitive silver bromide without heating. Thus, by 1880, says Mr. Bayley, “gelatine dry-plates were fairly on the market, exposures had been reduced to fractions of a second, and modern photography had ‘ arrived.’” The change was to make photography over, to trans- form it from a pursuit possible only to a few devoted professionals and amateur chemists to a universal helper in the affairs of mankind. The wet-collodion process, though producing exquisite results, required for outdoor work a cumbersome equipment including “a tent, a nitrate bath, a good supply of water.” The longer exposures caused the plate to dry, and spoil the picture, or, in cold weather, to freeze. Thus though there were many amateurs in the years from 1853 to 1858, they found their path a rocky one, and Harrison tells how “stains of inky blackness [from the nitrate solution] on the hands and clothes soon earned for the FROM DAGUERREOTYPE TO DFY PLATE 2.47 infant science the appellation of ‘the black art,’” and caused the disfavour into which photography as an amusement soon fell. In 1857 the Duke of Parma used visiting cards on which a little photographic por- trait took the place of his name, and Disderi, the pho- tographer to Napoleon the Third brought out soon after the little card pictures known as “Cartes-de- visite,” a name very familiar to a past generation. The wet-collodion process was “smelly,” dirty, troub- lesome, and required the most elaborate care. The pic- tures were excellent, but could be made only by ex- perts. Whereas by the dry-plate process, while the expert can still produce the finest results, every person can make good pictures, with little time and little labour, and without elaborate apparatus or a great battery of chemicals in a specially prepared dark I’OOII] . Besides all this, the bringing in of the dry-plate en- abled photography to become automatic, so to speak. It was no longer necessary for the photographer to re- main with his camera. The exposure could be made mechanically, and thus the camera could be left in position for the shutter to be operated by a wild ani- mal touching a cord, a thermometer or barometer that made an electric contact, a clock that at a certain hour released the shutter and so on. One of the men who contributed greatly to the ad- Vancement of photography was Professor Petzval, of Vienna. He saw that the daguerreotype and the wet- plate processes would be greatly aided by lenses bet- ter than those in use, and in 1841 worked out the problem set him, inventing a sort of lens known by his name. The Petzval lens gave good central defini- 248 PHOTOGRAPHY FOR YOUNG PEOPLE tion, and could be used at a very wide aperture (f/3 or f/4), being consequently exceedingly rapid. It was an excellent portrait lens, and its faults were such only as made it unsuitable for landscape photog- raphy, for it lacked mainly in even lighting, depth of focus, and astigmatism. Another photographer, whose work is of increasing importance, is Dr. Hermann Vogel, of Berlin, the dis- coverer of means for making plates sensitive to the red and yellow rays. His method was to stain the film which made it respond to the rays that otherwise would not affect it or would affect it very slightly. This was in 1873, but the full importance of his work was not appreciated for many years, though it was to become the foundation for the photography of colours, both in their true values when rendered by white, black, or gray, and also in their true tints — as is to- day done by several different processes, and as will be increasingly done in the future. All these process im- provements led also to improved apparatus. CHAPTER XXII A GLANCE AT MODERN PHOTOGRAPHY Dry-plate photography slowly developed — The first ‘‘ detective ’’ cameras — The earliest “Kodak” — The roll film —The daylight film — Improvements in printing — Combination prints–Wignet- ting — Enlarging — Chromophotography — The cinematograph — Uses of the ‘’ moving pictures” — The coming of new developers — The photographing of colours — Orthochromatic photography — Dyeing the plates — The colour-screen — Importance of Ortho- chromatic photography in making prints in colour. WITH the coming of the dry-plate, that was ob- tainable every where, would keep indefinitely, was easy to use, and rapid enough for taking objects in motion, modern photography began. Yet the very rapidity of these new plates was at first a cause of their unpopularity. The older pho- tographers simply could not believe in the short ex- posures. They were used to the wet-plate process, had learned to time their exposures accordingly, and for a long time would greatly overtime the new dry- plates and thus either fog them or get very thin im- ages by failing to give long development. Besides, they would develop by a yellow light that was not safe enough for the new and more sensitive plates. Consequently, during the years from 1874 to 1880, photographers were learning the use of the dry-plates, and changing from the collodion to the gelatine plates, while the experimenters were constantly improving the new methods. But by 1880 the new dry-plates 249 250 PHOTOGRAPHY FOR YOUNG PEOPLE were ready for general use, and had in most cases taken the place of the wet-collodion plates. In the next ten years, a number of manufacturers had put excellent dry-plates upon the market. In our own country Cramer and Norden of St. Louis, and John Carbutt of Philadelphia, were pioneers, and both the Cramer and the Carbutt plates have been well known ever since. When ready prepared plates were thus available, many were induced to take up photography, and there was a demand for small, portable cameras. From the amusing notion that these would be especially valuable to detectives in securing portraits of criminals, or at least that they might be so used, the earliest hand-cameras were designed to be unobtrusive black boxes, or were even made to look like books, luncheon cases, or other harmless objects that (it was believed) would deceive the unwary law-breaker. The first practical camera of this sort was invented (according to the Americana Cyclopedia) by a German named Schmid, and introduced by the E. & II. T. Anthony Company of New York, and their example was soon followed by many others as the number of amateurs increased. About the same time with the portable box-camera, John Carbutt brought out plates which were upon cut pieces of celluloid instead of glass, and, being unbreakable and light, were especially adapted for the hand-camera. The next marked improvement was the introduction by George Eastman, in 1888, of the first “Kodak.” The name was a coined one, without meaning, but has been accepted by the dictionaries as well expressing in sound the little “snap-shot ” camera. The earliest kodak was a narrow, square-fronted, oblong box that A GLANCE AT MODERN PHOTOGRAPHY 251 contained a long roll of sensitized paper sufficient for taking one hundred pictures. This idea of taking negatives on a roll of sensitive material was patented in England in 1854, but the roll seems to have been made of cut sheets gummed together. Then in 1871 came an improvement in the roller idea, by a Hungarian engineer named Warneka, who added several ways of judging how much of the roll had been wound up each time. But the Eastman roller device was superior in all respects to all that had been devised before it, and so succeeded. Within a year celluloid took, in the kodak, the place of the paper, the little cameras became very popular, and were in the hands of tourists every- where. The main improvements since then have been the introduction of “ daylight "rolls of film, protected from the light by ends of black paper which wind about the rolled celluloid and its coating, the adapting of the extension camera in the place of the more bulky box-form ; the various “magazine cameras” holding glass plates or cut films so they may be brought one by one into the place for exposing; the introduction, very recently, of the film-pack, which is a removable paper-box magazine holding cut films, and the many methods of developing without need of a dark room. Of the different devices for regulating length of ex- bosure – the shutters, diaphragms, and so on, we have already spoken. But some note must be taken of the improvements in printing methods, before speaking of the sorts of work possible to modern photography. The plain silvered paper as used in the earliest days was followed by the albumen papers that gave a surface image, and one of finer detail; then came the “aristo,” a highly glossy paper with a chloride of 252 PHOTOGRAPHY FOR YOUNG PEOPLE silver coating; and both of these papers are of course still in common use. In fact, most of the modern processes can be traced to earlier forms, of which they are improvements, and the general nature of them has already been described. But we may note the be: ginnings, as given by Harrison’s “History of Pho- tography,” of certain devices in the making of prints. He gives the first “combination printing,” as exhibited in 1855, in Glasgow — a landscape photograph into which a figure had been printed from another negative. Three years later Otto Sarony patented a combination process by which parts of negative films were to be united to make a new negative — a thing afterward done by cutting up paper-negatives. Tejlander, in 1857, printed portions of many negatives on a single photo- graph by masking parts of the paper with black velvet, and work printed from five, nine, and various num- bers of negatives masked, was shown in England by H. P. Robinson. The addition of clouds in landscape photography began in the fifties, and is much prac- ticed, the clouds being added by a second printing (the sky being masked during the first), or being painted in some light resisting tint (such as India ink) on the landscape negative. “Wignetting ” is a means of causing a print or nega- tive to be softened, shaded, or lost around the edges. It was described as far back as 1853. It can be done in the camera or in the printing frame. In the camera vignetting is caused by interposing between the object photographed and the plate a screen or mask which is cut to allow part of the object to be plainly and clearly focussed, and to interrupt the light rays beyond the clear portions of the picture. The screen or mask is A GLANCE AT MODERN PHOTOGRAPHY 253 out of focus, and has a saw-tooth or fringed edge. It may be put in front of the lens, or inside the bellows of an extension camera. In making a print, the vignetter is supported a few inches from the glass side of the negative, and allows part of the image to print clearly while the rest shades off to white. Adjustable vignetters, which may be arranged to make any shape of hole, are sold at photo- graphic supply stores; but it is quite easy to cut your own vignetter for any particular negative from paper — using light tissue to get grayish ef- fects ; or to shut out light en- tirely, the black paper in which plates and printing paper are wrapped. When printing with a vignetter, it is sometimes well to keep the frame in motion, so as to avoid all possibility of the vignette edges showing clearly. AN EASILY MADE A vignette on a black back- VIG NETTER ground may be made by first printing the picture, and then masking the central portion while allowing the rest to be fully printed out. Enlargements were made in 1875 by Valentine Blanchard, who threw an enlarged image through a negative upon sensitive paper, thus making a trans- parency, or positive. This was used to print a negative which was made transparent by waxing, and from the second negative were made enlarged prints. With the ability to obtain instantaneous photo- graphs came devices for taking a great number of pic- 254 PHOTOGRAPHY FOR YOUNG PEOPLE tures in quick succession, so as to give the history of an action or movement. Then followed other devices for Showing such photographs in rapid motion, so as to reproduce the action. In the Smithsonian Institution Report for 1901 is a history of these arts — “chrono- photography ’’ being the name given them. The earliest mentioned is an invention of an astronomer named Jansen who in 1873 made a camera in which a circular plate turned so as to take successive pictures of the planet Venus while crossing the sun. Other inventors had seen the possibility of taking such pic- tures of objects in motion as far back as 1857, 1861, and 1864; but photography was not able to do the work at so early a date. In 1878, Muybridge, of San Francisco, took by means of a row of cameras (12 or 24) a set of views showing the gaits of the horse in motion, and also of other animals. Anshūtz, of Vienna, followed the same method with the quicker gelatine plates, soon after- ward. In 1882, Dr. J. Marey, a French scientific worker, arranged a revolving shutter that made ex- posures at measured times, each.on a different part of a sensitive plate. Next came the “photographic gun" which took the pictures on a revolving plate, and a camera which turned on a pivot so as to follow a mov- ing object, and then of one into which a moving mir- ror reflected the images. But in 1887, Marey, owing to the invention of kodak paper film, was able to use a moving strip for taking the pictures; and when transparent films were made, these pictures could be both taken and exhibited by means of the lantern when changed to positives. Many imperfect forms of apparatus were devised, but none was satisfactory un- A GLANCE AT MODERN PHOTOGRAPHY 255 til Thomas A. Edison found a way of causing the mov- ing film to be viewed at just the right intervals, and brought out his “Kinetoscope ’’ in 1894, enabling one spectator to see the motion pictures—as in the “slot machines' now so well known. But a French in- ventor, Lumière, brought out the next year his “Cine- matograph,” which was a clever machine for catching, moving and releasing the film at the right rate and without injuring it. Marey tells also of later improvements upon the motion picture machines adapting them to various purposes. But he points out that when run at the natural rate of speed, the motion-picture does no more than repeat what the eye has seen. By running the films more slowly, quick motions (as, trotting of a horse or flying of a bird) may be understood and studied ; by running them more quickly (as, repeating in a short time a series of pictures taken at long inter- vals) we may get a clear idea of processes usually slow — as the changes of an insect in its metamorphosis, the growth of a plant, or even the putting together of a great piece of mechanism or the erection of a building. Thus slow motions may be hastened, quick ones made slow. In this way all motion may be studied, and its laws understood. The article from which we quote gives many useful applications of chronophotography. Though they may not seem now to be within reach of the amateur, yet they are more nearly within his power than even the simplest processes were only a few years ago. What would Wedgwood, Herschel or Daguerre have thought of a modern “watch camera,” fitting the vest- pocket and capable of making a dozen or two perfect Q. 256 PHOTOGRAPHY FOR YOUNG PEOPLE negatives, each in an instant, and each capable of enlargement P Of course we need not explain all the tricks and dodges used in making “motion pictures,” since they depend mainly on the fact that the instrument can be stopped, and any desired change made in the scene photographed. But we may make the suggestion that motion-photographs ought to be largely used in educating the young, since by means of the cinemato- graph almost any phenomenon or happening or proc- ess may be exhibited in the class-room. The move- ments of the planets of our solar system might readily be thus exhibited. The chemical side of photography has kept place with the improvement in the making of plates and the devising of cameras that will take advantage of the quickness of plates. Niépce, it will be remembered, developed by dissolving bitumen by oil of lavender; Daguerre used the vapour of mercury; pyrogallic acid brought out the images in the calotype process and on the collodion wet-plate. Ferrous sulphate was also used in the collodion process. Then came “alkaline” development, in which ammonia aided the action of the pyro ; and this in turn has been often replaced by carbonates of potash and of soda — which have a similar effect. Ferrous oxalate was suggested as a developer in 1877, and in 1882 it was found that sodium sulphite tended to prevent pyro from becom- ing brown and staining the plates. In 1889 came what are known as the “coal-tar developers ”— such as eikonogen, metol, Ortol, and so on, of which more has been said in speaking of the chemistry of pho- tography. ºth - *- - Courtesy of American Photography A Night Scene Such a picture can easily be made, giving an exposure of twenty to thirty minutes, using the snap-shot stop. The long shadows give a good appearance of depth and reality to the picture, an effect always obtained when the light is low. High-noon sunlight causes “flat" or shadowless lighting. & A GLANCE AT MODERN PHOTOGRAPHY 257 Especially modern are the processes that give us prints or negatives in natural colours, and those that try to interpret colours in the right relations as felt by the eye. The reader will see that here, in a sentence, are a number of subjects. These are the taking of a negative or positive in natural colours; the making of prints in colours; and the making of correct colour- value prints. We shall speak of each in turn, taking up first the question of making correct colour-value prints. This, from two Greek words for “right" do60s (Orthos) and “colour” zoöua (chroma) is called orthochromatic pho- tography, or sometimes “isochromatic,” or “equal” colour photography. We have already spoken of the weak action of the red and yellow rays on the plo- tographic plate, and strong action of the violet and blue rays. From this it results that ordinary photo- graphs do not show things in the same relation of light and shade that the eyes see. To correct this to some extent is the object of Orthochromatic photography. Dr. Vogel discovered in 1873 that by staining the plates with various dyes (yellow and red) they became less sensitive to the stronger rays, and so gave better representations of the brightness or darkness of things as the eye sees them. This idea was followed up by many workers, and various dyes were tried, one of the most valuable being eosin — a derivative from coal-tar. This was applied in 1882–3 to the gelatine bromide plates, and they were made commercially in England, while in 1886 Carbutt of Philadelphia made such plates in America, and others soon followed. Many different dyes were used, either in the emulsion or for soaking plates afterward. Amateurs will find many 258 PHOTOGRAPHY FOR YOUNG PEOPLE directions given for making plates orthochromatic, but it is easy to buy the plates ready made. But no dye was found that could prevent the violet and blue rays from doing more than their share in affecting the plate — that is more than they should do when com- pared with their effect on the eye. Consequently work- ers put before the lens a coloured glass or “screen " which, letting the others pass, held back the too active rays or obstructed them. The glass or screen is some- times called a “ray filter.” It stopped the non-lumi- nous violet rays, and left the eye-affecting rays to af- fect the plate. But of course this greatly decreased the light action, and so made longer exposures necessary when a screen is used. Without a screen the plates should be ex- posed according to the general colour of the subject, remembering that the orthochromatic plates are more sensitive to red or yellow, and less to violet, blue, and chemical (ultra-violet) rays. Consequently for yellow and red subjects or subjects lighted by yellow or red lights (as at sunset or in the early morning) ortho- chromatic plates need slightly less exposures. In yel- low or red lighting the use of the screen is not neces- sary, as the light has a similar effect. With a screen, the colour of the screen has to be taken into account. Follow the maker's directions, and use the screen recommended for each particular brand of orthochro- matic plates. A screen may require from twice to twelve times the usual exposures, or even more ; but in dully lighted landscape work the greens will be more effective when the screen is used, and it is valu- able in taking pictures showing white clouds or distant mountains against a blue sky. Of course where it i A GLANCE AT MODERN PHOTOGRAPHY 259 desirable to take pictures in which there is much red and yellow (as with flowers or fruit, or brilliant cos- tumes) the screen will help to give right values, and where the blue light is too strong — as at the sea- shore — Orthochromatic plates with screens will give many delicate effects. In the dark room, remember the sensitiveness of the plates, and also be more careful to use the developers as recommended by the maker, who knows what these special plates require. The worker with ortho- chromatic plates must, in short, remember that he is to proceed under entirely new conditions, and should prepare himself beforehand by careful study. Modern science has provided the photographer with means of making plates sensitive to many different colours, and even, it may be said to all colours with some ap- proach to correctness, and to use these means careful study of the manuals on the subject is requisite. It must be said also that sometimes a yellowish or red- dish object will seem to affect a plate when the light is reflected from it, even though the ordinary sort of plate is used. The question of orthochromatic pho- tography is most important, however, not to the usual amateur, but to the professional makers of colour- plates. Their work opens a new subject and may be included in another chapter. CHAPTER XXIII COLOUR WORK AND OTHER APPLICATIONS OF PHOTOGRAPHY Coloured prints from photographs — The three-colour process — True coloured negative — The Lippmann process — The Joly or Mc- Donough process — The recent Lumière process — A single-nega- tive method — What it accomplishes — Photography by ultra- violet rays — A glance over the field of modern photographic work — The amateur's recreations — Serious branches of photo- graphic work. CLOSELY connected with the question of making plates equally sensitive to the rays of different colours is the producing of prints in varied colours. But pho- tography has to do with the making of the plates from which the prints are printed rather than with the coloured pictures themselves. For the ordinary coloured prints produced by photography owe their colour entirely to being printed in coloured inks on the printing press. Photography in this, the ordinary “three-colour process,” largely due to Ives, of Phila- delphia, is used only to make three plates each of which is separately printed in a single coloured ink — usually a red, a blue, and a yellow. The three plates are so taken that each takes account of one colour in the scene photographed. Three photographic nega- tives are made by using coloured screens. Each screen shuts off all but one kind of light rays. Thus one ad- mits only red, shutting off blue and yellow ; another only yellow ; a third only blue. The negatives are 260 COLOUR WORK 261 the usual sort, but each records only one kind of light. Then by a process based on the same general principles as were used by Niépce, these negatives are made to yield printing-plates. Then by three printings in three colours one upon the other is produced a coloured print that may bear a resemblance more or less close to the natural colouring. Success in this depends on choosing the right colours for the three inks, printing them in the right strength, and printing accurately. Exact reproducing of natural colours is of course in- possible. Pigments are not lights. No blue tint can represent the colour of a bright blue sky, no white paper the brilliance of a white cloud, no black ink the blackness of darkness. The younger reader here may ask how it is possi- ble that with three colours we can reproduce all of the innumerable other colours seen in nature. This is be- cause the three colours we choose are what scientists call the primary ones. They are approximately red, green, and violet blue. What we know by the words brown, purple, pink, Orange, and many other names, are in reality only a combination of the three primary colours in various proportions. So that what we call brown or pink in nature, may be photographed so as to separate it into its three component primary colours; and when we print, we use inks that repre- sent the primary colours, and combine them again into the colours of the scene. Generally, printers use for their work red, light yellow and sky blue inks, and with these they get wonderful results; but they are not, strictly speaking, the true primary colours. Three transparencies can be made by the same method of photography, and lights of three colours may 262 PHOTOGRAPHY FOR YOUNG PEOPLE be sent through them to unite on a screen, making an image representing all three colourings; or by carbon printing and other methods the three plates may also be united. Yet none of these plans will give more than a suggestion of natural colouring. Sometimes cameras are so made as to take the three negatives at once, each through the right sort of colour filter, the right exposure for each plate being regulated by diaphragms of different sizes. With three such negatives on films, the three films might be coloured and put together to make one lantern slide. But how- ever it be used, the three-colour process is not “pho- tography in natural colours,” nor is it an approach toward the discovery of that long-desired art. There are certain ways of taking photographs in colours, but they are all, at least excepting the very latest, exceedingly difficult and uncertain. The one that belongs especially to the laboratory is what is named after its inventor, the “Lippmann Process.” But first we may briefly repeat what Abney in the Ency- clopedia Britannica records about early experiments toward true photography in colours. In 1810 a Dr. Seebeck of Jena received the image of the spectrum on moist chloride of silver and succeeded in getting traces of the natural colours; in 1839 Herschel saw similar results on the chloride, and both Daguerre and Fox-Talbot found red was sometimes reproduced on their plates; in 1840 and 1843 Robert Hunt produced the spectrum colours to some extent on paper dipped in nitrate of silver and then in sodium fluoride, and the print lasted over two months; Hunt also made other experiments with similar success. Then in 1848 Becquerel, the French chemist, prepared a silver plate COLOUR WORK 263 with a very pure silver chloride by means of a voltaic battery, and then gently heated it. Upon such a plate, the spectrum was photographed in colours, and “col- oured images of brightly dressed dolls were also ob- tained.” These images, however, like the first nitrate of silver prints, could not be “fixed,” and had to be kept from the light. Niépce de St. Victor in 1857 repeated and improved on Becquerel's method, but could not make the pictures permanent. In 1868, Poitevin made prints in colours on paper prepared with silver chloride, and after wash- ing exposed to sunlight for a moment, and then treated with bichromate of potash and copper sulphate and dried. Under a coloured transparency, this gave a coloured print. Poitevin said it could be fixed by the use of sulphuric acid. Other investigators secured similar results, but the authority from whom we quote states that the resulting tints on the paper prints were merely records of the different sensitiveness of the compounds used, not the effect of differently coloured rays of light — as in the case of the Becquerel daguerre- otypes, which is a “true colouration by the spectrum.” The Lippmann process is based upon the wave-theory of light, and depends upon the principle that the light waves may be reflected after passing through the sen- sitive film. When so reflected by means of a mirror (sometimes a receptacle filled with quicksilver), the re- turning waves interfere with the coming waves. The result of this action is to make stationary instead of travelling waves (as Professor Lippmann declares). These waves, he tells us, act in the substance of the film, instead of merely going through it, and “impress 264 PHOTOGRAPHY FOR YOUNG PEOPLE their structure on the film,” or throw it into such a condition that when the silver particles are formed under the action of the developer they lie in a set of planes that in some way correspond to the waves made by different coloured rays — that is waves of different length. , ' , Whether or not this is an explanation (and we con- fess that it conveys no very clear 'ea to ourselves), the result is to produce a plate that, after it is devel- oped and viewed by reflected light, reproduces the col- ours to the eye. Gabriel Lippmann, the inventor of this process, is a French professor born in 1845, and distinguished for his work in science. The method of photographing in colours was announced in 1891, but has not been greatly used, although special apparatus for viewing the plates has been devised, and they may also be projected on a screen by a rightly arranged lantern. It is not a process at present that is likely to come into popular use, though an interesting one as proving the theories about light rays and their wave-action. In 1894 Professor Joly of Trinity College, Dublin, invented a method by which one negative is taken through a screen ruled with very fine close lines of orange, yellowish-green and blue. Then a positive is made from the negative, and viewed, when lighted, through a similar screen, whereupon the colours of the original scene are reproduced to the eye, though the negative is the usual colour of ordinary negatives. The theory of this process is not unlike that of the usual three-colour process except that in the Joly plate the colours are produced by putting the three colours close together instead of one over the other. Indeed the COLOUR WORK 265 coloured lines are put so close as to give the eye the effect of their overlapping. The negative is taken through these lines, each line shutting off all but its own colour. Thus, where a red surface comes, the negative is imprinted strongly or thickly under the red lines, not und “hº others. Then a positive being made, becomes thin Just where the negative was thick, and so this red su -º- portion is thin just opposite the red lines. Now if the positive be viewed by means of a similar screen over it, these thin portions over the red lines show red, while the other colours are blocked out where the positive is thick. So we see a red light- ing where the red surface made the positive thin. It makes no difference whether the positive be viewed by light on it or through it, as in one case we look through the screen and see its red, and in the other case we have light coming through the red to us. The blue and yellow lines act in the same fashion. There is in the human eye something like this ar- rangement. It is believed that the retina upon which we receive the images that come through the eye-lens contains a number of the ends of nerves. These nerves are sensitive to colour waves, each nerve to one of the three main colour-sensations, red, blue, yellow (though, strictly speaking, the sensations should be considered green, red, violet). Thus when we look at a red rose, the red-sensitive nerves are affected where the image of the rose rests, the other nerves in that space being less excited to action. This Joly process was improved by McDonough, an American. Credit for the idea underlying the three- colour, the Lippmann, and Joly processes, is largely due to a French worker, Louis Ducos du Hauron, who 266. PHOTOGRAPHY FOR YOUNG PEOPLE in 1869 outlined the principles governing them. At a much later date this inventor devised a camera that took upon three plates the negatives necessary for the three-colour process, and also contrived that the posi- tives could be viewed through the same camera so as to give the effect of a single picture in colour. There is still another process to be described, which is the most recent of all and seems to be more likely to come into general use among skilled amateurs. This is the “Lumière Process.” In a photographic journal for August, 1907, it is stated that the “new Lumière autochrome plate is on the market in Europe, and will be soon sold in America.” By this method a single plate is exposed as usual and can then be de- veloped into a positive in natural colouring, and a permanent picture, a transparency, thus made of any scene. This new process depends upon the structure of the new plate. The plate is prepared first by spreading upon a sticky surface starch granules of exactly uniform size and dyed in the three primary colours, orange, green, and violet. These are so small that 20,000 will cover an inch of surface, and are put in a single layer, none overlapping. A black substance was at first used to fill up all spaces, so every ray of light must come through the stained granules, but this is no longer required. Then the film is so flattened by great pressure that the grains have flat faces, top and bottom, and will not act as lenses. This, when varnished, is the foundation for the photographic emulsion, and the plate so prepared looks nearly white, like a fine ground glass. Next an emulsion is put on this foundation — one that is “panchromatic,” or sensitive to all three colour- COLOUR WORK 267 rays when used with a special yellow screen that goes with these plates. This emulsion is very thin and of bromide-collodion. Exposure is made glass-side fore- most — so that the light comes through the starch- granule foundation before reaching the emulsion. The necessary exposures vary from one-sixth second in bright sunshine with a quick lens (at f/6) to twenty or more seconds and upward. After ex- posure there is a peculiar development. In the Joly process, it will be remembered, the object is attained by making a positive so that the light can come through in the places where the negative was dark. In the Lumière process, the negative itself is changed to a positive. First the darkened portions are developed as usual. The developing is in darkness. Next the plate is “reduced ” (by potassium permanganate and sulphuric acid), which removes the silver that has been darkened. The plate is now developed once more (with amidol), which darkens the emulsion that before was not dark. The plate is then intensified, cleared, and after being rinsed, fixed, and dried. The accounts of the process given by experts in Europe say that the pictures produced are of marvellous beauty and brilliance, and very true to nature. The Lumière brothers, the inventors, are said to be per- fecting means for making prints from the negatives, but that is not yet done. The plates can be kept some time before exposure, and the resulting pictures are said to be permanent. A German authority says that the process in its results far surpasses all others, and is confirmed by English and American workers who have tried the plates. The plates are naturally very expensive, $2.50 for four plates 5×7 in size — or ten 268 PHOTOGRAPHY FOR YOUNG PEOPLE dollars a dozen, but no doubt will be made more cheaply. It must be said that these are not all the means of making coloured pictures by photography, but the principles can be understood from these, the most im- portant, and the leading processes. The reader will be ready to admit at least that the progress in colour- photography since 1873 has been very great, and that the outlook for the future seems hopeful, even though the art of taking actual photographs in colours — the fixing of the actual colour image — has not yet been achieved. Another recent photographic triumph is the taking of photographs by means of the invisible rays, and thus securing photographs of objects so minute that the ordinary visible rays will not show them. Visible rays are of longer wave-length than the ultra-violet or invisible rays, and so when used in microscopic work interfere with one another. By using the ultra- violet rays, the waves are shorter, do not interfere with one another, and so bring out things the eye cannot separate. These short waves do not affect the eye, but they do affect the photographic film. They will not pass through ordinary glass lenses, and so Quartz lenses are used ; they are not visible, and so focusing has to be done by using a fluorescent screen of uranium glass which makes them visible; the Ob- jects examined must be mounted on quartz and cov- ered by the same mineral. But when all this is done, the ultra-violet microscope will show things of only half the size of those before considered the smallest visible, and will also tell us much of structures trans- parent to ordinary light, but showing differences of COLOUR WORK 269 constitution in the ultra-violet photographs. To the microscope also has been applied the Lumière colour process, so as to take natural colour pictures of the most minute objects. Modern photography covers so many branches and is applied so widely that we cannot expect to do more than give the reader the merest hints of the many subjects in which the camera has given mankind new eyes. By its use the invisible is seen, as in astronomy, where the plate records more than the eye receives; in microscopic work, as has been set forth ; in instanta- neous pictures of objects in rapid motion; in the use of other rays than those the eye knows; in submarine and surgical photography, where the camera may be made to act apart from the operator; in natural his- tory work, by automatic shutters; in scientific record instruments actuated by clockwork — and so on end- lessly. Not only is the record different from that of our vision, but it is permanent and accurate. Not only is it complete, but it may be made large or small at will. The camera aids every art, science, trade and pro- fession, and its field extends daily. The amusements of the amateur at one time, give rise at a later period to most useful improvements available in practical life. There is a little book called “Photographic Amuse- ments,” written by Walter E. Woodbury, author of an “Encyclopedic Dictionary of Photography.” This is a collection of “novel effects obtainable with the camera,” and serves to show how ingeniously the powers of photography may be applied. There are Suggestions in the volume for using in connection with 270 PHOTOGRAPHY FOR YOUNG PEOPLE the camera a number of adjuncts. Thus from the mir- ror we may get multiple images; by using odd-shaped reflecting surfaces, distorted views are secured ; by interposing screens we may produce caricatures, show- ing a big head on a small body, or a portrait on a bust- pedestal; by under-exposure of one image, followed by full exposure of another, are produced “spirit” pictures; by photographing wall-paper laid on a floor from a suspended camera, it may be made to repre- sent a wall, and all sorts of accidents made to take place, since a figure lying down seems in the plate falling through space. Other possibilities are silhou- ettes, taken against stretched tissue-paper, with short exposures and long development ; distorted photo- graphs on plates set at various angles in the camera, or taken through vertical or horizontal slits; “moon- light ° photographs taken in full sunlight (with the sun in the picture) by means of a very small stop and too quick exposure with under-development; the tak- ing of snow crystals or frost-markings in winter, and so on through every sort of ingenious modifying of the usual conditions. - The means of making these odd pictures will be very quickly picked up by any amateur who will be- come familiar with the right methods of picture-mak- ing. To avoid errors, you must know what causes them ; and, knowing how they are caused, it is not a difficult matter to make errors on purpose. For ex- ample, many so-called “freak pictures” are shown. In them we may see a man playing checkers with him- self, or a woman holding a book on which a tiny im- age of herself is standing. Such effects are produced either by exposing part of a plate at a time, or by Copyright, 1996, by A. B. Phelan A SpecimeN of Photographic IxceNUITY Courtesy of Photo-Era Magazine A Duplicate Port RAIt - - (A description of this process is given in the Appendix) COLOUR WORK 271 having a black space come in the part of the view where you want to introduce a second figure. The second exposure uses either a second part of the plate, or puts a lighter figure against the black background, to affect the unaffected portion of the plate. Pinhole photography, night photography and com-. posite photography, are matters of another sort, each a branch well worthy of the most careful and serious study. But each would require a separate treatise, and the reader who is interested will find many de- lightful handbooks available to him. When you begin to study special subjects like these, you will need to seek out the works devoted especially to them. CHAPTER XXIV SOME HINTS ON THE CHEMICAL SIDE Chemistry and its language — Meanings of the symbols and formulae – Acids and bases — Salts — Other compounds — Important ele- ments — Light and the silver salts — Chemistry of developing— Chemistry of fixing – Intensifying and reducing — Warning to the amateur — Some text-books on chemistry — Photography an art of expression. THE language in which chemical facts are recorded is simpler than it looks. The elements (those sub- stances which cannot be simplified or changed) are expressed by their initials, either one or more ; and these initials are to be learned or known by looking at the Table of Elements (see last chapter). Opposite each will be found its “atomic weight' — that is, the weight in which it combines with other elements. It always combines at this weight or a multiple of it. Where the letter alone is written it means just so many parts of that element as is expressed by the atomic weight. Thus the atomic weight may be con- sidered as the smallest possible amount of the substance that will enter into a chemical compound. The num- bers represent the weight of each substance as com- pared with hydrogen — the lightest of all. Thus iron is 56 times as heavy; gold, 196 times; platinum, 1974 times, oxygen, 16 times. Water is hydrogen and oxygen, two parts of H, one of O, or “H.O.”— the one chemical symbol we all remember. But any quantity of water must then consist of 2 weights of 272 SOME HINTS ON THE CHEMICAL SIDE 273 hydrogen to 16 of oxygen, 2 volumes of hydrogen to 1 of oxygen. Thus, in 2,000 pounds of water there would be (in round numbers, and leaving fractions for school hours) 222 pounds of hydrogen and 1,776 pounds of oxygen. And this will show how we can always calculate how much of any chemical by weight is in any compound, since we know from the formula how much weight (in atomic weight) goes to one part of the compound. Silver nitrate (as used by Wedgwood and the rest of us photographers) is, for example: AgNO3. If we put down the atomic weight we shall have : Silver (argentum, Ag.) = 107.93 Nitrogen (N) = 14.045 Oxygen (O) three parts = 48. 169.975 Say 170 for ease of calculating. Then, in 170 pounds, ounces, grams, or tons, of nitrate of silver there would be (nearly) 108 parts of silver, 14 of nitrogen and 48 of oxygen. And, in the same way, you can take any chemical compound and by translating the symbols and attaching the atomic weights, you will have the receipt for the compound. Chloride of sil- wer is AgCl — or 108 parts silver and 35 of chlorine; and no matter how much or how little of these com- pounds you have, they are made up of these relative quantities and relative weights. The elements when combined from various com- pounds, and according to their behaviour the elements are considered as “acid-formers ”or “base-formers,” though some form both acids and bases. An acid and a base are so named because they differ greatly in 274 PHOTOGRAPHY FOR YOUNG PEOPLE their action ; acids contain hydrogen, bases contain a metal; and when an acid acts on a base, the hydrogen and the metal exchange places. The acid then usually becomes neutral — or neither acid nor alkaline, and the hydrogen unites with the oxygen of the base and there is water formed. The acids therefore contain hydrogen exchangeable with a metal or the metal from a base. The bases contain metal combined with hydrogen and oxygen, and treated with acid exchange the metal for hydro- gen. The acid acting on a base gives a neutral sub- stance called a salt, and also causes water to be formed by the uniting of the Oxygen and hydrogen. The chemist considers all elements that will replace hydrogen in an acid to be metals. As to names, acids end usually in ic, as nitric acid, sulphuric acid, hydrochloric acid, tartaric acid. But if there are two acids formed from an element, the One with less oxygen ends in ous. Thus there is nitrous acid, and nitric acid – with these formulae HNO, and HNO, - the nitric having in each molecule (or smallest possible portion) one more atom of oxygen. In the same way sulphuric acid is H.SO, ; while sul- phurous acid is H.S.O. If in an acid there is still less oxygen, the prefix, hypo (Greek “under’), indicates this, as in hypochlorous acid ; if there is an acid con- taining more oxygen than in the best known acid the one known to have most oxygen has the prefix “per” (Latin for through or “very ") as in perchloric acid. Thus (taking our illustration from Remsen's “Intro- duction to Chemistry ") from chlorine we have “chloric, chlorous, hypochlorous, and perchloric acid " — but in each case the acid is merely a compound of SOME HINTS ON THE CHEMICAL SIDE 275 chlorine with various atoms of hydrogen and oxygen — in other words with the elements of water. With these explanations you will be able to see the reason for the names of acids. The bases (among which are the substances called alkalis) combine with acids and neutralize them, form- ing what are called salts. Thus bases and acids com- bine and change into substances unlike either, and we have already said that this comes about when the hy- drogen of the acid changes places with the metal of a base. Thus if nitric acid acts on silver and dissolves it, the nitric acid exchanges its hydrogen for Silver, and the IINO,--Ag produces AgNO, or silver nitrate. The salts have this ending, ate when formed by the acids ending in ic. When formed by acids ending in ows, they have the ending ite — as in sodium sulphite — formed from sodium by sulphurous acid. Thus our old friend “hypo’’ is “hyposulphite of sodium,” as it is formed by the action of hyposulphurous acid on sodium. The bases, being compounds of metals with hydro- gen and oxygen are known as hydroxides — as potas- sium hydrocide (caustic potash), and caustic soda is sodium hydrowide. Each metal can (theoretically) yield a base when treated by an acid, and thus we have nitrates, chlorates, sulphates (instead of sulphur- ate) according to the acid used. Prefixing the name of the metal, we have the compound — as silver nitrate, copper sulphate, and so on. The elements with which most of us have to deal are not more than two dozen, and it will not take very long for the amateur photographer to know something about their properties, and about the compounds used 276 PHOTOGRAPHY FOR YOUNG PEOPLE in photography. The ending “ide’” means simply “compound of ’’; thus compounds of bromine are known as bromides, of sulphur as “sulphides,” of oxygen as “oxides.” With so much of chemical talk to make the “hard words” more familiar, we express the hope that the young photographer will soon be driven to regular works on chemistry — as he will sooner or later be glad to know fully the chemical facts that explain the reasons for his work. The more important elements to the photographer are gold, silver, platinum, iron, copper, mercury, zinc, lead ; sulphur, phosphorus, chlorine, bromine, iodine ; boron, calcium, carbon, hydrogen, magnesium, nitrogen, owygen, potassium, sodium. Of these, four will form salts directly with a metal, and so are called “halogens” (from the Greek hals and gen) or “salt-makers.” Cyanogen (a group of a carbon and a nitrogen atom — with the symbol CN, though not a compound, is found in various com- pounds, and these are called “cyanogens”) is also a halogen. These halogens are important in photography. Now when a silver salt (as a bromide or chloride of silver) is acted on by light, it is believed that the mole- cule of the salt is separated into its atoms. The light waves agitate the atoms. Originally composed of two atoms of silver and two of the halogen (silver bromide is Ag, Br, and silver chloride is Ag,Cl), the light de- composes the compound into a sub-bromide by liberat- ing a bromine atom if the compound be silver bro- mide, or makes a sub-chloride from silver-chloride by liberating a chlorine atom. It is just as if the com- pound were four bathers holding each other's hands – the two brothers Bromide and the two brothers Silver, SOME HINTS ON THE CHEMICAL SIDE 277 and a big wave pulls them a little way apart, so that they either lose their hand-clasp or loosen it. Now, being already somewhat separated, the group is composed of the two brothers Silver, and one brother Bromide— the other Bromide brother being by himself, thus: But besides the separation of B, the waves have greatly weakened the union of the group, and either of the S brothers may easily be de- tached (for being held by chemical attraction, the one atom B cannot strongly hold more than one atom S). Consequently when we put the developer at work, we have a compound ready to break up, and form new compounds. Pyrogallic acid mixed with an alkali, such as sodium carbonate, has a strong affinity for oxygen. It takes oxygen from water (II.O), leaving the hydrogen free to take part in the breaking up of the halogen. Thus the new chemicals added and produced in the water attract, the bromine atoms. First they take away the free atom, and then the other, from each group. This leaves the silver atoms by themselves — or reduced (or simplified) to metallic silver. Thus the developer continues the sep- aration begun by the light waves, and produces in the film metallic silver. Pyrogallic acid has the formula: C.H.(OH), and is chemically called a “tri-hydoxyl-benzene’’— hy- droxyl meaning the group OH, and the benzene being the C.H., (in which Ha-HOH, replaces H.). The carbon compounds, among which pyrogallic acid is classed, are too complicated for any but technical books. We need only remember that they can develop 278 PHOTOGRAPHY FOR YOUNG PEOPLE plates by taking the halogens away and leaving the silver. After we have developed the plate, we must take away the part of the haloid salt, the silver compound, unchanged by light and developer. This is done by the hypo bath. Hyposulphite of sodium is Na2S2O3−5H2O. The latter part of this formula, 5H2O, means simply that the crystals contain five parts of water held in them. Another name given by chemists to hypo is thiosul. phate of sodium. “Thio’’ is from the Greek 0siov (theion), sulphur, and the term indicates that the salt is the result of the action of thiosulphuric acid on sodium; and thiosulphuric indicates an acid in which some of the oxygen of sulphuric acid has been replaced by sulphur atoms. Whatever the theory, our useful “hypo ’’ has the ability to dissolve the silver salts if they have not been broken up by light waves, or de- velopment. But there must be a strong solution of hypo, or there will be formed in the film an insoluble chemical instead of a soluble one. This insoluble double salt is Ag, Na,(S.O.), and it will remain in the film in spite of Washing, and may afterward discolour it. So use fresh, strong hypo. Rightly used the hypo forms the double salt: AgNaS,O, and this will be washed out by water, leaving the film free from any compound that will injure it. But before this double salt is washed out it is invisible, being transparent. Hence we leave negatives in hypo till the white dis- appears, when we know that the bromide of silver has been changed to these double salts, and then as long again, so that they may be dissolved out and cleared away. Be careful to fix thoroughly, and then wash thoroughly, if you want permanent negatives. SOME HINTS ON THE CHEMICAL SIDE 279 The chemistry of intensifying consists in either changing the colour of the silver deposit, so as to make it more resisting to the rays of light ; in making the image more visible to the eye by adding to the deposit something else, or substituting something else for it. Thus using mercuric chloride (HgCl), it forms with the silver a double chloride of mercury and sil- ver, and then this is stained (by ammonium hydrate) a deep brown — which resists the light rays. There are also methods of adding more silver to that already deposited. By means of platinum and gold combina- tions — gold chloride and platinum tetrachloride, for example — the silver is made to combine with the chlorine, is then removed, and leaves the gold or the platinum in its place. But for these methods, which are complicated, it is fair to refer the reader to the text-books. Before leaving the subject of the negative two more things must be noted. The first is the tendency of a chemical action to continue when once started — as seen in the burning of wood, the rusting of iron, the crystallizing of a dissolved substance from a solu- tion. Advantage is taken of this in increasing develop- ing action when once begun — as in the use of chem- ical developers after light has acted either on plates or printing papers. The second is the operation of reducing a negative. Chemically this is done by the use of agents that combine with the silver making new compounds that are soluble, and may be washed out. Thus ferrocyanide of potassium changes the silver partly to a mixture of silver and ferrocyanide; the latter being soluble is washed out leaving the silver in a state when hypo will wash it out. Other iron 280 PHOTOGRAPHY FOR YOUNG PEOPLE compounds are used for reducing, as perchloride of iron with citric acid, and reducing agents also used are sulphate of copper, and potassium permanganate. The amateur who means to try any of these intensi- fying and reducing methods should be sure to know something of the powerful chemicals used. For it must be impressed on young photographers that a great many of the agents used in the various processes are active and powerful poisons. Photography is no place for carelessness or bungling. The making of prints introduces a whole new class of chemical facts and proceedings. But into these there is no room to enter. Generally speaking, the desire to know the details of the processes, and the reasons why the chemicals act as they do, should send the amateur to the various text-books on the subject of photographic chemistry. A very excellent one is Abney’s “Treatise on Photography,” and another is Harrison’s “Chemistry of Photography.” On special subjects, the reader will find the various numbers of “The Photo-Miniature ?' most helpful; an especially useful one being “Chemical Notions for Photog- raphers” which tells about the qualities and uses of all the most useful compounds. You will not, of course, expect to know the whole subject even generally ; but you can easily follow out the main facts of the processes you choose for most of your work, and thereby learn what is right and wrong in them, and wherein to make changes. In this chap- ter the purpose has been only to give you some little introduction to the subject in order that you may be invited to go further by yourself. The last chapter of this book contains certain tables SOME HINTS ON THE CHEMICAL SIDE 281 and rules that may be found useful, but the more serious worker is strongly advised to buy each year one or more of the Photographic Annuals, which con- tain excellent helps and discussions and tables upon every subject the photographer may need. In closing the author desires to be considered only as one who has tried to direct amateurs to better knowl- edge than he ever hopes to possess of the great science and art of photography. The expert often knows too much to be the best helper for those who are making their way among the elementary principles, whereas the learner who has not long ago travelled the same path remembers the stumbling blocks and the blind trails that perplex. Above all things remember that photography is an art of ea pression, and like other arts of the kind de- pends for its final, true value upon what the artist is trying to express. Much of your earlier work must be accidental in its results, but the amateur who learns to know the possibilities of lens, camera, and print, will have little ambition if he does not desire to become rather the master than the slave of these wonder- Working marvels of modern science. THE END Appendix WEIGHTS AND MEASURES UNITED STATES STANDARDS From the “American Annual of Photography,” 1907 LINEAL Inches. Feet. Yards. Rods. Fur's. Mile. 12 inches = 1 foot. 12 = 1 3 feet = 1 yard. 36 = 3 = 1 5.5 yards = 1 rod. 198 = 16.5 = 5.5 = 1 40 rods = 1 furlong. 7,920 = 660 = 220 = 40 = 1 8 furlongs = 1 mile. | 63,360 = 5,280 = 1,760 = 320 = 8 = 1 VOLUME–LIQUID 4 gills = 1 pint. Gills. Pints. Gallon. Cub. In. 2 pints = 1 quart. 32 = 8 = 1 = 231 4 quarts = 1 gallon. FLUID Gallon. Quarts. Pints. Ounces. Drachms. Minims. 1 = 4 = 8 = 128 = 1,024 = 61,440 1 = 16 = 128 = 7,680 1 = 8 = 480 1 = 60 16 ounces, or a pint, is sometimes called a fluid pound. TROY WEIGHT Pound. Ounces. Pennyweights. Grains. Grams. = 12 = 240 = 5,760 = 373.24 1 - 20 - 480 = 31.10 1 - 24 = 1.56 Precious metals are sold by Troy weight. 283 284 PHOTOGRAPHY FOR YOUNG PEOPLE APOTHECARIES” WEIGHT ft) gr. Pound. Ounces. Drachms. Scruples. Grains. Grams. 1 = 12 - 96 F: 288 = 5,760 = 373.24 1 - 8 — 24 = 480 = 31.10 1 F 3 = 60 = 3.89 1 = 20 = 1.30 1 = .06 The pound, ounce, and grain are the same as in Troy weight. AVOIRDUPOIS WEIGHT Pound. Ounces. Drachms. Grains (Troy). Grams. 1 F 16 - 256 - 7,000 F. 453.60 1 — 16 - 437.5 - 28.35 - 27.34 == 1.77 Chemicals are sold by avoirdupois weight. 1 ounce avoirdupois = 437% grains Troy or Apothecaries'. METRIC SYSTEM MEASURES OF WOLUME Names. Kiloliter or stere Hectoliter Deckaliter Liter Deciliter Centiliter Milliliter Names. Millier or Tonneau Quintal Myriagram Kilogram or Kilo Hectogram Dekagram Gram Decigram Centigram Milligram No. of Liters. Wine Measure. 1,000 264.17 gallons. 100 26.417 gallons. 10 2.6417 gallons. 1 1.0567 quarts. 1-10 .845 gill. 1-100 .338 fluid Oz. 1-1000 .27 fl. drn. WEIGHTS No. of grams. Avoirdupois Weight. 1,000,000 2204.6 pounds. 100,000 220.46 pounds. 10,000 22.046 pounds. 1,000 2.2046 pounds. 100 3.5274 ounces. 10 .3527 ounce. 1 15.432 grains. 1-10 1.5432 grain. 1-100 .1543 grain. 1-1000 .0154 grain. º COINS AS STANDARDS By the use of coins as weights in a balance (made APPENDIX 285 ut of a stick and two little disks of cardboard) chem- ical solutions can be made up accurately enough for most photographic processes. WEIGHT OF COINS (In Apothecaries' System) Standard dollar 412; grains Half-dollar 192 '' and a little over. Quarter-dollar 96 ‘' & & $ & 4 & Dime 38 { { { { { { { { * { 5-cent (nickel) 77 ( { { { { { { { 1-cent (copper) 48 ‘‘ Five-cent nickel, 2 centimeters diameter, weighs five (5) grammes. 1 gramme = 15% grains. MEASUREMENTS Half-dollar, 1% inches in diameter; Tâ⺠inch in thickness. Quarter, ! ... “ * { Iłºw º - 1 4 * { { * { { 3 2 { Dime, 2 Ö To () () For liquids, an ordinary drinking-glass holds about four ounces when half-full, and about 9% a pint, full. EXPOSURE TABLE OF COMPARATIVE LIGHT VALUES BY REV. DW IG HT W. SMITH. “American Annual of Photography,” 1907. While there is a wider range in timing the ex- posure of a dry plate than is generally supposed, yet it is well known that there is but one correct interval for the best results with a normal developer. To best approximate that interval at all available hours of the day and year requires some attention and experience. It will be seen in this table, that in January, the light value for noon is given as 1.7, while at 4 P. M. the ex- posure would necessarily be more than five times that 286 PHOTOGRAPHY FOR YOUNG PEOPLE duration. For July, the most rapid as well as longes available light of any month, the light at noon is indi cated by .2 instead of 1.7, and at 3 P. M. more tha twice the time will be required. The first column indicates the hour of the day; th second column the comparative light values in whol numbers and tenths. JANU ARY. FEBRUARY. MARCH. APRIL. 8 10 8 6 8 3 8 2 9 4 9 4 9 2 9 1.5 10 2.5 10 2 10 1.5 10 1.7 11 2 11 1.7 11 1.2 11 1 12 1.7 12 1.5 12 1 12 1 1 1.7 1 2 1 1 1 1 2 2.5 2 2.7 2 1.7 2 1.2 3 4.5 3 3.5 3 2 3 1.5 4 9 4 5 4 4 4 2 5 60 5 20 5 4 6 20 MA. Y. JUNE. JULY. AUGUST. 8 1.7 8 1.7 8 1.5 8 1.7 9 1.2 9 1.2 9 1.2 9 1.5 10 1 10 1 1() 1 10 1 11 .7 11 .6 11 .5 11 .7 12 .5 12 .3 12 .2 12 .5 1 .7 1 .5 1 .5 1 .5 2 1 2 .7 2 1 2 1 3 1.2 3 1.2 3 1.2 3 1.2 4 1, 5 4 1.5 4 1.5 4 1.7 5 2.7 5 2.2 5 2.2 5 2.5 6 15 6 5 6 4 6 5 7 80 7 20 7 15 7 60 SEPTEMBER. OCTOBER. NOVEMBER. I) ECEMBER. 8 2 3 8 4 8 9 9 1.5 9 1.7 9 3 9 3 1() 1 10 1.5 10 2 1() 2 11 1 11 1.2 11 1.7 11 1.5 12 .5 12 1 12 1.5 12 1.7 1 1 1 1.2 1 1.5 1 2 2 1.2 2 1.5 2 2 2 2.5 3 1.5 3 2 3 2 5 3 3.5 4 2 4 2.7 4 5 4 8 5 3 5 6 5 20 5 80 6 10 6 40 6 70 APPENDIX 287 IR. W. K. BURTON'S TABLE OF COMPARATIVE EXPOSURES." From the “Photographic Reference Book '' # = #e a 3, ##= == 3 24 -- : : ſ baQ | W +E P. tſ.< .: Tº 5 rture of lens * ; 2 # = 3 ne ſº #3 & #3: ... : : # # & 3 £U E & “. .- := 2 - T : T. (AED E - tſ. nder E. 5 1 D - º + = ºr 3 := - 3. System and 3 3 # 2, 3 trees. Fº teriors. # = 2 * : * ~ : f System ă T. * : 3 £: |##### 5 §3 3 #. : * = Up to # 7 Up to 5 Ż £3:e * * * Z_i > - a |* 'sec sec. sec. m. s. m. s. h.m. m.s. see. m. s. 1 = f/4 || | | | | | 0 10 0 10 0 2 | 0 || | | | 0 4 8 = f/11.3 3' | } 1 120 1 20 0 16 || 0 8 1% 0 32 16 = f/16 tº 2 2 40 2 40 0 32 || 0 16 2š 1 4 32 = f^22.6 # 4 520 520 1 4 || 0 32 || 5 || 2 || 8 64 = f 32 3 14 8 10 40 1040; 2 8 1 4 103 || 4 16 13s = i is 2 3; 16 |31 go 31 30 316 3 & 21 $33 256 = f/64 º º * 42 to 4240, 832 |416 42 17 4 | } alling # 1 6 Up to 480 Up to 48 8 192 480 5,760 OBJECTS BY W. D. KILBEY From the “American Annual of Photography,” 1907 A TABLE SHOWING THE CORRECT EXPOSURE THAT SHOULD BE GIVEN FOR VARIOUS MOVING The table is made out for a distance from the camera 100 times that of the focus of the lens ; that is, for a 6-inch focus lens at 50 feet, a 7-inch at 58 feet, an 8-inch at 67 feet, a 9-inch at 75 feet, or 12-inch at 100 feet. -º-º-º- 32 Wynne. * These are for bright sunlight in May, June, or July, slow plate = 16 H & D = 32 Watkins 288 PHOTOGRAPHY FOR YOUNG PEOPLE Toward At Right the Angles to Camera. the Camera. Man walking slowly, street Scenes . . . . . . I's sec. 3's Sec. Cattle grazing . . . . . . . . . . . . . T; “ 4's “ Boating . . . . . . . . . . . . . . . . . .'; “ * “ Man walking, children playing, etc. . . . . . 4's “ T}o “ Pony and trap, trotting . . . e º 'º Tº “ 3 #5 “ Cycling, ordinary * * * * * g e & e Tº “ sº a “ Man running a race and jumping . . T} iſ “ #6 “ Cycle racing . . . . . . . . . . . . . . . . 2 #6 “ who “ Horses galloping . . . . . . . . . . . zło “ sło “ If the object is twice the distance, the length of allowable exposure is doubled, and vice versa. RELATIVE BRILLIANCY OF ARTIFICIAL LIGHTS From the “American Annual of Photography ’’ No. l 2 3 4 5 6 7 8 9 1 Sun at Midday, June 21,–1 1 2 Light of Magnesium Lamp (burning 1 gram of powder) 3 1 3 Magnesium Ribbon, 3 mm. wide 14 5 1 4 Electric Arc Lamp 35 11 2.5 1 5 Oxyhydrogen Light 50 16 3.6 1.4 1 6 Gas, Welsbach System 165 53 11 7 10 1 7 In can descent Electric Lamp (24 volts) 1,600 533 115 46 32 10 1 8 Oil of Petroleum Lamp 2,300 766 165 66 46 1 4 1.4 1 9 Stearine Candle 18,000 6,000 1,300 515 360 109 11 7 1 l3y means of this table, the nine chief sources of light above given can be compared with each other as to their relative brilliancy. EXAMPLE.—Compared with the sun, the Welsbach Gas Light is 165 less brilliant, but is 10 times more brilliant than the electric incandescent lamp, and 109 more brilliant than the light from a stearine candle. COMPILED BY MIR. J. W. ELSDEN PO ISONS 1& E M A R KS CII A RACTERISTIC SY M PTOMS ANT II) OTES Ox A LIC ACI ſo, including POTASSI UM OXA LATE AMMONIA POTAS LI SO ) A MElt CURIC CH LORIDE ACETATE OF I, EAD CY ANI DJ. ( , F POT Ass IUM B1 CIT ROMATH, C, F POTAS- SJ U M TNITRATE ( , F SILVER NIT 1: 1c AC II) FH Y DROC Fr LC, RI ( ' A CID SI I I, ſº I I I I It I ( ' A " i I) LIYDIto FLU Olt I C A CID ACE IODIN F. PYROG A Lilo I, ty. Applied 1 dram is the smallest fatal (19se known. Vapour of am nonia may cause inflatu Illation of the Jungs 3 grains the Smallest known fatal dose. The sub. acetate is still more pois0110 uS. a. Taken internally, 3 grains fatal. b. Applied to wounds and abrasjons of t lie Skin. (t. Taken internally. to slight abra- Sious of the skin. 2 drams have been ſatal. Inhalation of the funes has also been fatal. *4 ounce has caused death. 1 (1 ran ) has been fatal. !2 ounce has caused death. tro A CID, concentrated, has Variable in its action ; 3 grains have been ſatal. 3 grains sufficient to kill a dog. Hot, burning sensation in throat and Chalk, whiting, or magnesia sus- stomach ; vomiting, cralups and pended in water. Plaster or Liu ſubneS8. mortar can be used in emer- gency. Swelling of tongue, mouth and ſauces: Vinegar and water. often ſollowed by stricture of the esophagus. . Acrid, In, etallic taste, constriction and White and yolk of raw eggs with burning in throat and stomach, tol-, milk. In emergency, flour lowed by nausea and vomiting. | paste may be used. Constriction in the throat and at pit of Sulphates of soda or magnesia. stomach ; Cranlpy pains and stifliness Enuetic Of Sulphate of zinc. of abdomen ; blue line round the gll n.) S. Insensibility, slow, gasping respira. No certain remedy cold effu- tion, dilated pupils, Spasmodic clo-, sion over the head and neck sure of the jaws. most eſlicacious. Sun arting sensation. Sulphate of iron should be ap- plied immediately. Irritant pain in stomach and vomiting. Emetics and magnesia, or chalk. Produces troublesome sores and ulcers. Corin mon salt to be given imme- diately, followed by emetics. Powerful irritant. | Corrosion of windpipe, and violent Bicarbonate of soda, or carbonate inflammation. of magnesia or chalk, plaster of the apartinent beaten up 111 Water. Similar to hydrochloric acid, though In ore violent. as powerful an effect as the mineral acids. Acrid taste, tightness about the throat, Vomiting should be encouraged v Odin iting. and gruel, arrowroot and starch glºven freely. Resembles phosphorus poisoning. No certain remedy. Speedy - - - emetic desirable. - - - −x-Txpre-op-porsors-rrºr-rrrrrºrPºs = i 3. 290 PHOTOGRAPHY FOR YOUNG PEOPLE TABLE OF THE SYMBOLS AND ATOMIC. WEIGHTS OF THE ELEMENTS - ATOMIC NAME SYMBOL WEIGHT Aluminum . . . . . . . . . . . Al 27.5 Antimony (Stibium) . . . . . . Sb 122.0 Argon . . . . . . . . . . . . . A 39.9 Arsenic . . . . . . . . . . . . As 75.0 Barium . . . . . . . . . . . . Ba 137.0 Beryllium (Glucinum) . . . . . Be 9.4 Bismuth . . . . . . . . . . . . Bi 208.0 Boron . . . . . . . . . . . . . Bo 11.0 Bromine . . . . . . . . . . . . Br 80.0 Cadmium . . . . . . . . . . . Cól 112.0 Caesium . . . . . . . . . . . . Cs 133.0 Calcium . . . . . . . . . . . . Ca 40.0 Carbon . . . . . . . . . . . . C 12.0 Cerium . . . . . . . . . . . . Ce 138.0 Chlorine . . . . . . . . . . . . Cl 35.5 Chromium . . . . . . . . . . . Cr 52.2 Cobalt . . . . . . . . . . . . Co 58.8 Copper . . . . . . . . . . º Cu 63.4 Didymium . . . . . . . . . . . Di 145.0 Erbium . . . . . . . . . . . . E 166.0 Fluorine . . . . . . . . . . . . F 19.0 Gallium . . . . . . . . . . . . Ga 68.0 Germanium . . . . . . . . . . Ge 72.5 Glucinum . . . . . . . . . . . G 9.4 Gold . . . . . . . . . . . . . Au 196.0 Helium . . . . . . . . . . . . He 4.0 Hydrogen . . . . . . . . . . . H 1.0 Indium . . . . . . . . . . . . In 113.4 Iodine . . . . . . . . . w I 127.0 Iridium . . . . . . . . . . . . Ir 193.0 Iron . . . . . . . . . . . . . . Fe 56.0 Lanthanum . . . . . . . . . . La 139.0 Lead (Plumbum) . . . . . . . . Phy 207.0 Lithium . . . . . . . . . . . . Li 7.0 Magnesium . . . . . . . . . . Mg 24.0 Manganese . . . . . . . . . . . Mn 55.0 APPENDIX 291 NAME SYMBOL Mercury . . . . . . . . . . . . Hg Molybdenum . . . . . . . . . . MO Neodymium . . . . . . . . . . Nd Nickel . . . . . . . . . . . . . Ni Niobium (Columbium) . . . . . Nb Nitrogen . . . . . . . . . . . . N Osmium . . . . . . . . . . . . Os Oxygen . . . . . . . . . . . . O Palladium . . . . . . . . . . . Pol Phosphorus . . . . . . . . . . P Platinum . . . . . . . . . . . Pt; Potassium (Kalium) . . . . . . K Praseodymium . . . . . . . . . Pr Rhodium . . . . . . . . . . . Rh Rubidium . . . . . . . . . . . Rb Ruthenium . . . . . . . . . . Ru Samarium . . . . . . . . . . . Sm Scandium . . . . . . . . . . . Sc Selenium . . . . . . . . . . . Se Silicon (Silicium) . . . . . . . Si Silver (Argentum) . . . . . . . Ag Sodium (Natrium) . . . . . . . Na Strontium . . . . . . . . . . . ST Sulphur . . . . . . . . . . . . S Tantalum . . . . . . . . . . . Ta Tellurium . . . . . . . . . - . . Te Terbium . . . . . . . . . . . Tb Thallium . . . . . . . . . . . T] Thorium . . . . . . . . . . . . Th Thulium . . . . . . . . . . . Tul Tin (Stannum) . . . . . . . . Sn Titanium . . . . . . . . . . . Ti Tungsten (Wolfram) . . . . . . W Uranium . . . . . . . . . . . . U Wanadium . . . . . . . . . . . V Ytterbium . . . . . . . . . . . Yt. Yttrium . . . . . . . . . . . . Y Zinc . . . . . . . . . . . . . . Zn Zirconium . . . . . . . . . . . Zr ATOMIC WEIGHT 200.0 96.0 144.0 58.8 94.0 14.0 191.0 16.0 106.6 31.0 194.8 39.0 141.0 104.4 85.4 101.7 150.0 43.9 79.4 28.0 108.0 23.0 87.5 32.0 182.0 127.0 128.0 204.0 231.5 171.0 118.0 48.00 184.0 240.0 51.2 172.6 89.0 65.0 90.0 292 PHOTOGRAPHY FOR YOUNG PEOPLE DEVELOPMENT The following excellent instructions in development are reprinted from Cramer's Manual, issued by the G. Cramer Dry Plate Co., St. Louis: Into a tray of proper size pour a sufficient quantity of developing solution to well cover the plate. Slide in the plate, and by a tilt of the tray cause the solu- tion to flow evenly over it. Another way is to lay the plate in the dry dish, face up, and pour the developer over it in one sweep without stopping. A tuft of filtering cotton (kept for this purpose in a saucer of clean water) should be passed gently over the plate to remove any adhering air bubbles. Rock the dish occasionally and keep the plate well covered with the developer, for stain is apt to appear when the plate is exposed too much to the action of the air. Continue development until sufficient density is ob- tained, which can be judged by taking the plate out of the tray and holding it against the red light for a short time. However, the less a plate is exposed to the developing light, the better. If the plate was correctly eaſyosed the high lights of the image will soon appear in the developer, then the half tones and finally the detail in the shadows, and if sufficiently developed, the resulting negative will have all the desired printing qualities, viz.: sufficient density with full detail, and the parts of the plate where the light has not acted will be perfectly clear. If the plate was over-exposed the whole image will appear simultaneously as soon as the action of the de- veloper takes place, and the negative will be flat and lacking in contrast. APPENDIX 293 Lack of contrast may be helped some by carrying the development as far as possible so as to get the greatest density, and after fixing, reducing. The addition of bromide of potassium to the developer after development has begun has but little effect on the quality of the negative, and only slows the development, but its addition to the developer be- fore it is applied to the plate has a restraining effect on the shadows and helps to keep down fog. An under-exposed plate will develop slowly without detail in the shadows, and will not yield as good a negative as one that is correctly timed. The ex- posure should be made over, but if this is not possible, a passable result may be obtained by transferring the plate without rinsing to a tray containing pure water at about 80 degrees Fahrenheit, and after soaking a while, back to fresh developer. Another method is to use a diluted developer which works soft and does not fog the plate. The main object in develop- ing an under-exposed plate is to obtain detail in the shadows. During the necessary prolonged develop- ment the plate must be completely protected against all traces of light. Should the negative, after fixing, be found too intense in the high lights, we have in persulphate of ammonia an effective remedy to reduce the same without losing the detail in the shadows. An attempt to force development by an overdose of alkali will always result in failure. After developing is completed, rinse the plate well, and place it in the fixing bath for the purpose of dis. solving the bromide of silver which has not been acted upon by the light and the developer. After all the bromide of silver appears to have been dissolved in 294 PHOTOGRAPHY FOR YOUNG PEOPLE the fixing bath, leave the plate therein at least ten minutes longer to insure permanency and freedom from stain. | Plates that are left in the acid fixing and harden- ing bath for half an hour, will not soften in the wash water nor show reticulation (puckering of the film) even in warm weather; they will dry quickly and not be so apt to gain undesirable density, provided the fixing bath is in good condition. If the bath is too strong, and not stirred before using, it will cause parallel lines on the negative, due to the differing densities of the upper and lower portions of the bath. All tray developers work best at a temperature of 65 to 70 degrees Fahrenheit. If the dark room is cold, the developer should be slightly warmer or more concentrated. If the dark room is hot, the developer should be colder or more diluted. A concentrated developer works fast and with much density. A diluted developer works slower but with finer detail and is best for short exposures. If the developer is too concentrated or too warm it will produce fog, unless it is restrained by the addi- tion of bromide of potassium solution. If too much diluted, it is prone to produce stain by the long immersion required ; also peculiar streaks. Weak negatives with clear shadows are due to un- der-development or too weak developer. Weak negatives with plenty of detail in the shadows are due to over-exposure or too flat lighting of subject or too weak developer (use less water). Strong negatives with too much contrast are due to APPENDIX 295 under-exposure or too strong developer containing too much alkali. Add more water and use less carbonate of soda or potassium, as an excess of alkali blocks the whites. Too much intensity is the result of the developer being too warm or too strong, or development carried too far. Negatives dried in warm, sultry air assume more intensity than when dried in a cool place with draft. Frilling, softening of the film, film leaving the glass, are caused by too high temperature. When this occurs cool the developer and use fixing and harden- ing bath. For reticulation (puckering of the film) leave the negative in the acid fixing bath for half an hour to harden the film way through. DEVELOPERS FACTORS FOR DEVELOPERs From Watkins on Development, in Photo-Miniature, No. 66 5 Adurol. 10 Ortol. 5 Quinol. 12 Diogen. 6 Imogen sulphite. 18 Amidol (2 gr. per oz.) 7 Glycin. 20 Edinol. 9 Eikonogen. 30 Metol. 10 Kachin. 40 Rodinal. 10 Pyrocatechin. 60 Diamidophenol. PYRO-SODA OR PYRO-POTASH DEVELOPER Grains of pyro Factor Grains bronide Factor peº. without bromide. per Oz. with bromide, 2 12 i 5 3 10 - e # 4} 4 8 • * 1 4 5 6} 2 3 For Watkins' System of Development see Photo-Miniature No. 34 296 PHOTOGRAPHY FOR YOUNG PEOPLE Following are two developers for special purposes given in Cramer's Manual : DEVELOPER FOR LINE WORK (Black and White) Metric. Pure Water . . . . . . . . . . . 30 OZS. . . . . . . 900 C C m Cramer's Dry Sulphite of Soda . . . 2 ozs. . . . . . . 60 grams (Which will test 32° by Hydrometer.) Edinol . . . . . . . . . . . . 150 grains . . . . . . 10 grams Bromide of Potassium . . . . . 100 grains . . . . . . 7 grams Carbonate of Potassium . . . . 23 ozs. . . . . . . . 75 grams Use full strength. This developer, with special contrast plates, pro- duces negatives of great intensity and absolute clear- ness, desirable for copies of pencil sketches, pen draw- ings, line work, etc. TROPICAL DEVELOPER (For hot climates where mo ice is available) Metric. Pure Water . . . . . . . 50 ounces . . . . . . . . 1200 C C m Cramer's Dry Sulphite of Soda. 1 ounce . . . . . . . . 24 grams Bromide of Potassium . . . . 20 grains . . . . . . . . 1 gram Citric Acid . . . . . . . . . 20 grains . . . . . . . . 1 gram For use : To 4 ozs. of the above solution add ten grains dry Amidol; or to 200 cc m of above solution add 1 gram dry Amidol. Before developing place the plate in Water . . . . . . . . . . . . . 60 parts Formalin . . . . . . . . . . . 1 part for about three minutes, then rinse well and place in the developer. Fix in the acid fixing and hardening bath. The following analysis of the elements of a de- veloper, from Cramer's Manual, is also of interest: The carbonates of soda or potassium are added to give the developing agent the alkalinity required for APPENDIX 297 ction, whereas the sulphite is added to prevent apid decomposition and discolouration. Carbonate of potassium is of the same strength as ure dry carbonate of soda. These alkalis may be substituted for one another in ny formula. Two ounces of dry carbonate of soda equal five ounces of crystal carbonate of soda, provided the dry carbonate of soda is really chemically pure. For many years it has been generally believed that an excess of alkali gave softness and detail, and for this reason a largely increased quantity of alkali was used for short exposures, though it was generally known that beyond a certain quantity it caused chem- ical fog. Experiments conclusively prove that when the plate is developed the same length of time, the greater the quantity of alkali used, the more rapid the reduction, and the greater the contrast. Therefore if a negative which is properly lighted and timed, shows too much contrast, reduce the quantity of alkali, or increase the quantity of water until the image shows proper balance. If a properly timed negative lacks contrast, increase the quantity of the alkali, or use less water until sufficient contrast is obtained. Doubling the quantity of water in normal pyro developer reduces contrast because the deposit of silver in the strongly lighted portions of the plate proceeds slower, giving more time for the half tones and shadows to gain their maximum strength. For the same reason, reducing the alkali reduces the contrast between the high lights and lower tones of the negatives. Bromide of potassium is added to the developer to counteract the effect of over-exposure, its action being 298 PEIOTOGRAPHY FOR YOUNG PEOPLE to produce contrast and clearness by restraining the development of the shadows. For this reason the contrast developer to be used for this purpose, con- tains a large dose of it. A very small quantity of bromide of potassium or of contrast developer is of benefit as an addition to fresh developer, if it does not work perfectly clear. One drop of a solution (1 part bromide of potassium in 10 of water) usually being sufficient for two ounces of developer. The following is from the American Annual of Photography: - The tendency of a greater or less quantity of any factor in the developer is as follows: Developer itself (Pyro, Ekonogen, etc.): More—clogs up whites; too much contrast. Less—slow development; lack of brilliancy. Alkali : More—quick development; dense, flat negatives; fog and granulation. Less—slow development; contrast. Sulphite : More—colder tone. e Less—warmer tone; Stain. Water : More—thin in high lights; detail. Less—contrast. Temperature : Should be about 70 deg. F. Higher—intensity; fog. Lower—flatness. APPENDIX 299 The warmer and closer the atmosphere in which the negative is dried, the more intense it becomes. Mr. Alfred Watkins is quoted as saying: “In a paper read before the Royal Photographic So- ciety, I described a comparison of seven developers, namely: pyro, metol, ortol, adurol, hydroquinone, kachin and glycin. All were made up with the same formula (no bromide) and compared under the same circumstances. The result may be summed up : “Effect on speed of plate, very slight and doubtful difference. “Searching out detail, no difference. “Ultimate density power, no difference. “Appearance of image, wide difference. “Speed of working, no difference. “There is one respect in which developers differ. One class of developers (represented by metol, rodinal and weak pyro) causes all the tones to appear very early in the course of development, and density seems to follow with comparative slowness. This class has the reputation of giving thin negatives because users are deceived by the rapid appearance of image and take the plate out too soon. In the second class of developers (represented by hydroquinone, (quinol), strong pyro and adurol) the lowest tones or detail ap- pear slowly, and by the time they are out the high lights have attained quite a respectable amount of density, and density is afterward attained quite rapidly. The usual tendency with these developers is to over-develop and thus get too much contrast. “It really does not matter which developer you use 300 PHOTOGRAPHY FOR YOUNG PEOPLE if you take the plate out of it at the right stage of contrast ; for all (variations in bromide excepted) give identical negatives if their action is stopped at the right moment. For general purposes it is more con- venient to use a developer which is neither in the first class mor the second, but intermediate, density follow- ing the appearance of the image at a comfortable rate. It is a peculiarity of pyro that it belongs to the first or the second class according to the grains of pyro to the ounce of developer.” TANK DEVELOPMENT HURTER AND DRIFFIELD'S STANDARD DEVELOPER, FOR TANK USE Pyro . . . . . . . . . . . . . . . . . 8 parts. Sodium Carbonate . . . . . . . . . . . . 40 “ Sodium Sulphite . . . . . . . . . . . . . 40 “ Water . . . . . . . . . . . . . . . . . 912 “ 1,000 No bromide of potassium. Use at 65°. RODAK TANK DEVELOPMENT From Kodak Advertisement Standard. 1 Powder. Temp. 65° Fahr. Time of Development, 20 Minutes. Time of Temperature. Development. 70 degrees . . . . . . . . . . . . . . . 15 minutes. 68 “ . . . . . . . . . . . . . . . 17 65 “ . . . . . normal . . . . . . 20 “ 60 “ . . . . . . . . . . . . . . . . 25 “ 55 “ . . . . . . . . . . . . . . . . 30 “ 50 “ . . . . . . . . . . . . .. . . , 35 “ 45 “ . . . . . . . . . . . . . . . . 40 “ APPENDIX 301 Standard. 2 Powders. Temp. 6.5° Fahr. Time of Development, 10 Minutes. Time of Temperature. Development. 70 degrees . . . . . . . . . . . . . . . 8 minutes. 68 ‘‘ e e s tº e º e e s a º 9 “ 65 “ . . . . . . . normal . . . . . 10 “ 56 “ . . . . . . . . . . . . . . . . 13 “ 50 “ . . . . . . . . . . . . . . . . 15 “ 44 “ . . . . . . . . . . . . . . . . 17 “ Developer must never be warmer than 70° Fahr. It will be noted that it requires just double the time or development between 65 degrees, the normal tem- Yerature, and 45 degrees when using one powder, and learly double the time when employing double strength eveloper. The variation in the temperature of the atmosphere will make some difference in the results, but not suffi- ciently so to be taken into serious account. At low temperature some difficulty may be experienced in dis- solving the developing powders; crushing the powders very fine and adding slowly to the water while stirring will lessen this difficulty. From a Kodak Pamphlet. It has been fully demonstrated that sea water may safely be used in compounding the developer and for all the processes of Tank or Machine Development, provided only that the final rinsing is in clean fresh Water. TANK DEVELOPER FORMULE From Burke and James's (Chicago) Pamphlet on the Ingento Tank. GLY CIN-STOCK SOLUTION (This developer is especially recommended.) Glycin . . . . . . . . . . . . . . . . . . 120 grains. Sulphite of soda dried (Anhydrous) . . . . 360 “ Carbonate of soda dried (Anhydrous) . . . 360 “ Water e - - º - e - e o - º º - º o - e - 35 OUln CeS. 302 PHOTOGRAPHY FOR YOUNG PEOPLE For 20 minute developer, temperature between 6: and 70 degrees: To each part of stock solution, ad 3 parts water. For one hour developer, temperature between 6 and 70 degrees: To each part of stock solution, add 9 parts water. HYDROCHIN ON -STOCK SOLUTION Hydrochimon . . . . . . . . . . . . . . 90 grains. Sodium Sulphite dried (Anhydrous) . . . 400 “ Sodium Carbonate dried (Anhydrous) . . . .390 “ Water . . . . . . . . . . . . . . . . 30 ounces. For 20 minute developer, temperature between 65 and 70 degrees: To each part of stock solution, add 3 parts water. INTENSIFIERS AND REDUCERS The following formula is given in Cramer's Manual, for reducing negatives which are too dense all over, and lack contrast, owing to over-exposure and over- development: A Water. . . . . . . . . . . . . . . . . . 16 ounces. Hyposulphite of Soda . . . . . . . . . . . . . 1 ounce. (Which will test about 15° by Hydrometer.) B Water . . . . . . . . . . . . . . . . . . 16 ounces. Red Prussiate of Potassium . . . . . . . . 1 ounce. As this solution is affected by light, the bottle con- taining it, should be of amber colour or wrapped in opaque paper and kept in the dark when not in use, Mix for immediate use :- APPENDIX 303 Use in subdued daylight. The negative can be placed in this solution directly fter fixing. If a dry negative is to be reduced, it must be soaked in water for at least half an hour efore applying the solution. To avoid streaks, al- ways rinse the negative before holding it up for ex- mination. As soon as sufficiently reduced wash horoughly. For intensifying negatives, Cramer's Manual gives the following: No. 1. This solution will keep and work well until exhausted. Metric. 16 ounces of Water . . . . . . . . . . . 500 c c m. 120 grains of Bichloride of Mercury . . . . 8 grams. 120 grains of Bromide of Potassium . . . . 8 grams. No. 2. Number 2 should be mixed fresh. 8 ounces of Water . . . . . . . . . . . 250 C C m. 1 ounce of Cramer's Dry Sulphite of Soda 30 grams. (Which will test 60° by Hydrometer.) After the negative is well fixed and washed, immerse in No. 1 until it has become thoroughly whitened, and after rinsing carefully place it in No. 2, leaving it there until entirely cleared. In case sufficient intensification has not been gained, wash for ten minutes, repeat the operation and finally wash well. If after intensifica- tion the negative is too dense it may be reduced by placing it for a few seconds in water 16 ozs., Hypo. 1 oz. | If the negative has not been thoroughly fixed and washed before intensification, stains will ensue. 304 PHOTOGRAPHY FOR YOUNG PEOPLE The following are taken from the American An nual of Photography, 1907: INTENSIFIER (MERCURIC) WITH sodium sulPHITE, FOIR GELATINE DRY - PLATES Whiten the negative in the saturated solution o mercuric chloride, wash and blacken with a solution of sulphite of sodium 1 in 5. Wash well. The reduction is perfect, with a positive black ton REDUCER FOR GELATINE DRY-PLATES Perchloride of Iron . . . . . . . . . . . . . 30 gr Citric Acid . . . . . . . . . . . . . . . . 60 gr. Water. . . . . . . . . . . . . . . . . . . 1 pint PRINTING PROCESSES THE PLATINUM PROCESS The following brief summary of the platinum proc. ess is taken from A. Horsley Hinton’s “Platinotype Printing ” (A mateur Photographer Library). This book contains, besides very full descriptions of methods, instructions for colour-toning of platinum and for glycerine development. The negative and printing-frame having been thor- oughly dried, the paper is exposed in the printing- frame in the ordinary manner until the image is seen mapped out in grey or orange grey tint. It is then placed upon the oxalate bath with a pushing, sliding movement, the bath being about 70° for cold-bath paper, or about 170° for hot bath, the solution being roughly one part of oxalate to four or six of water for APPENDIX 305 old bath, or in the proportion of one pound of oxalate o fifty-two ounces of water (or a slightly super-satur- ted solution) for hot bath. Development occupies but few seconds—more does no harm—when the print is transferred to a solution of hydrochloric acid and water f the strength of one in seventy. After this the prints are leisurely subjected to one or two successive acid baths of the same strength, and then finally washed in water for about fifteen minutes. SPECIAL TONES ON PLATINUM SEPIA TONES From Wilson's Photographic Magazine The use of zinc oxalate for obtaining warm brown tones with ordinary black platinum paper was first suggested by Dr. R. Jacoby. He now states that rich warm sepia tones can be produced by using the fol- lowing developer: Potassium oxalate . . . . . . . . . . . . 200 parts. Ammonium phosphate . . . . . . . . . . 50 parts. Copper Sulphate . . . . . . . . . . . . . 2 parts. Water. . . . . . . . . . . . . . . . . . 1000 parts. The prints should be left for at least five minutes in this, otherwise they lose a lot in the fixing bath. For brown tones, A. Horsley Hinton, in “Platino- type Printing ” suggests a dram weight of mercury bichloride added to three or four ounces of the oxalate developer. Prints are developed and cleared similarly to black prints. 306 PHOTOGRAPHY FOR YOUNG PEOPLE THE GLY CERINE PROCESS From the “American Annual of Photography” The “Glycerine Process,” or the process of develop- ing platinotype prints by application of the develop- ing agent with the brush, is perhaps one of the most interesting and fascinating of photographic processes, owing to its far-reaching possibilities. By this method of developing platinotype paper, many negatives, which have been discarded on account of the dim, flat, non-contrasty results which they yield, may be made to give fair results, carefully printed, and, in the hands of one possessing a little artistic skill, snappy, animated pictures may be obtained. On the other hand, from the sharp and hard negative, soft, sketchy effects may be obtained. There are required for this process: some glass jars; some soft brushes, varying from the fine spotter and the Japanese brush to the 1% inch duster, and several pieces of special blotting paper. Print the paper a trifle deeper than for the ordinary method of developing. Place the print face up on a piece of clean glass (should the print curl so that it is unmanageable, moisten the glass with glycerine), and, with the broad camel's hair brush, thinly coat the en- tire print with pure glycerine, blotting same off in three or four seconds; then re-coat more thickly such portions as are desired especially restrained, or the de- tails partly or entirely eliminated. Now brush or paint such portion of the print as is first desired with solution of one part glycerine and four parts normal developer, blotting the portion being developed from time to time to avoid developing too far. Full strength APPENDIX 307 developer (without glycerine) is employed where a yronounced or deep shade is wanted. [If desired, nother solution, equal parts glycerine and water, may be kept at hand and used where caution is advisable.] When any part of the print has reached the full de- velopment desired, blot that portion carefully with the blotter and coat with pure glycerine. THE KALLITYPE Photographic Times Formula Coat stout but fine grained paper with a solution of Sodium ferric-oxalate . . . . . . . . . . . 6 drachms Water . . . . . . . . . . . . . . . . . . 23 ounces Dry quickly without the application of heat, and print till the deeper shadow portions of the picture become visible. On removal of the print from the frame, immerse into a 1% per cent. solution of nitrate of silver acidified slightly with citric acid, when the picture will develop brilliantly and with all detail. Finally wash in pure water. A yellow tinge may be Washed away with a 5 per cent. solution of oxalic acid. “SALTED,” OR PLAIN SILVER PAPER From the “American Annual of Photography,” 1902 Sensitizing Plain and Albumen Paper.—The usual method of rendering paper of any kind sensitive to light is to float it for a varying length of time on a solution of silver nitrate, having previously salted it, if it be plain paper, with some chloride, usually chlo- ride of ammonium. In practice it has been found that the strength of the silver bath should not fall be. low thirty grains of silver to the ounce of water, lest 308 PHOTOGRAPHY FOR YOUNG PEOPLE the albumen be dissolved; and that, save in exce tional cases, there is no need of a greater strength tha sixty to sixty-five grains to the ounce. The precis strength necessary to produce the best results with any given brand of albumen paper depends upon th amount of chloride used in salting; a paper weak in chloride requiring a weak bath, while one rich i chloride demands a strong one. Formulae for Sensitizing Bath.-For very stron negatives : No. 1. Silver nitrate . . . . . . . . . . . . . . 35 gr. Water . . . . . . . . . . . . . . . . . 1 oz. Print in full sunlight. For thin negatives: No. 2. Silver nitrate . . . . . . . . . . . . . . 80 gr. Water . . . . . . . . . . . . . . . . . 1 oz. Print in the shade. Floating the Paper.—There should be enough of the bath poured in to cover the bottom of the pan to a depth of at least half an inch, and it should have been most carefully freed from all impurities before the sensitizing is begun. Impurities and air-bubbles are the two great enemies of the sensitizing room. Grasp the paper by the two opposite corners, albumen side down, bring the hands together, and lower the convex side to the surface of the bath; separate the hands, and the paper will float on the surface. If it shows an obstinate tendency to curl up, gently breathe upon it. This difficulty may be overcome by placing the paper, the night before sensitizing, in a damp place. Now raise one corner and look for air-bubbles. APPENDIX 309 f any are found, break them with the point of a glass od, and again lower the paper. When it has floated he proper length of time, from one to three minutes eing the usual time, raise it by one corner very lowly, until another corner is free, which is then rasped by the other hand and the paper slowly with- rawn, allowed to drain a minute into a dish, and ung up by one corner to dry in the dark, or yellow ight. Points in Sensitizing.—1. Have the paper damp efore silvering. 2. Before floating ascertain the condition of the ath as to strength and alkalinity. 3. Do not allow the paper to become bone-dry efore printing if you wish to have rich prints. Of ourse, it must be dry enough not to adhere to the egative; anything more than this is not only useless, ut fatal to securing the best results. - Toning Solution. A. Chloride of gold . . . . . . . . . . . . . 1 gr. Water . . . . . . . . . . . . . . . . . 20 Oz. B. Acetate of Soda . . . . . . . . . . . . . 15 gr Water . . . . . . . . . . . . . . . . . 1 oz. Saturated solution of sulphate of copper. When solution is complete, add B to A, and add 10-15 drops of C, allow to stand at least twenty-four ours before using. Tone only until the half-tones re somewhat bluish by reflected light. This bath will keep. Fixing Bath. Hyposulphite of soda . . . . . . . . . . . 4 oz. Water . . . . . . . . . . . . . . . . . 20 oz. 310 PHOTOGRAPHY FOR YOUNG PEOPLE REDUCTION OF BLUE PRINTS BY SAMUEL PURNELL From Camera Craft To secure the best results from a blue-print, a manipulated in the usual way, is more difficult than i: generally supposed. The chief difficulty is to print i to just the proper depth. If under-printed it is of no value ; if over-printed it has heretofore been consid ered also valueless. I have discovered that an over printed blue-print may be cheaply, quickly, evenly and successfully reduced to just the density desired and without any damage to the print. The method employed is so practical that it is advisable to inten tionally over-print all blue-prints, so as to be sure they are printed deeply enough, and afterward reduc them by this process. When the finished and dried blue-print is seen to b too dense, soak it in water for a few minutes. In tray put a pint of water and dissolve in it about a heaping teaspoonful of bicarbonate of soda ; the exac quantity is not material. Immerse the blue-print i this and rock the tray. Do this by daylight. Re duction proceeds at once and rapidly, the speed de pending on the alkalinity of the bath. Just before the print is reduced to your liking, transfer it to an other tray in which fresh water is running. Wash it for about five minutes and then lay the print out t dry. PRINTING ON SILK From the “American Annual of Photography,” 1899 Boiling water . . . . . . . . . . . . . . 80 ounces Chloride of ammonium . . . . . . . . . . 100 gr. Iceland moss . . . . . . . . . . . . . . 60 gr. APPENDIX 311 When nearly cold, filter and immerse the silk for fifteen minutes. Sensitize for fifteen minutes in an acid 20-grain silver bath, and when dry stretch the fabric over cardboard. Print deeper than usual and tone in Water . . . . . . . . . . . . . . . . . . 20 Ounces Acetate of Sodium . . . . . . . . . . . . 2 drachms Chloride of gold . . . . . . . . . . . . . 3 gr. Common whiting . . . . . . . . . . . . . a few gr. “ FAKE '' PHOTOGRAPHY AND SPECIAL EFFECTS FIRELIGHT EFFECTS BY DAYLIGHT (SEE ILLUSTRATION FACING PAGE 202) From an article by Henry Essen.high Corke, reprinted in The Camera The sitter posed on a raised platform, so as to be on a level with the bottom of the window, in this case of ground-glass and about two feet from the floor. The sit- ter should be as near the source of light as possible, so that the lighting may be rather concentrated. All the dark blinds are then drawn, leaving only a patch open about two feet square, just in front of the sitter, where the fire is supposed to be. A fender and hearth-rug are then placed in front of the light on the floor. In some cases it may be found convenient to place a mir- ror, in the “fireplace,” so as to give an extra amount of reflected light upward onto the face of the sitter. A small strip of white paper may be placed inside the fender to look like the white hearth. - It is desirable to use a dark background, composed of dark curtains; these should not be allowed to hang in folds, but should be stretched tightly, or awkward streaks of high light will possibly show on the folds 312 PHOTOGRAPHY FOR YOUNG PEOPLE Exactly the same effect can be obtained in the same Way in an ordinary room and at an ordinary window. All that is necessary is to block up the window with brown paper, from the top downward, as may be re- quired, so as to give an opening of suitable size as low as can conveniently be managed. The sitter is then raised to a level with the opening, using a large din- ing table or boards supported on trestles for the pur- pose. The other arrangements are the same as just described. Alternatively, if French windows are available, they may be used, and there is then no need for a platform. The sitter is posed on the floor, and a large white sheet thrown down outside the windows will be found to throw a bright reflected light into the room. If by any chance the ground outside should be cow- ered with snow, the same effect is secured without the sheet. The exposure should err on the underside, as a rather hard negative is best suited for this class of subject. Of course, the actual exposure will vary according to many prevailing circumstances, but it may be some guide to say that with about two feet of ground-glass, with the sitter about two or three feet from it, using a lens working at f/4.5, about two and a half seconds will be about right with a fast plate. In development the high lights should be allowed to attain sufficient density, and no thought need be taken of the shadows. I should also advise a pyro-soda developer, as with it the high lights are not so likely to clog up as when hydrokinone or such developers are used. APPENDIX 313 DUPLICATE PHOTOGRAPHY (SEE ILLUSTRATION FACING PAGE 270) SEGMENT DUPLICATOR. (Cut reproduced from Photographie Amusements.) This consists of a disk of pasteboard or black material fitting the lens front exactly, with a slice taken off on one side. The proper size of the opening should be determined by experi- ment; it should be just large enough to expose half of the plate. After a photograph has been made on one half of the plate, the disk is turned around so as to expose the other half. Devices of this sort may be bought. LZ ANOTHER DUPLICATOR. (Cut reproduced from the Photo Era.) This is made from heavy cardboard, and the hole should fit over the lens front snugly. It should not be forgotten that the duplicator always 314 PHOTOGRAPHY FOR YOUNG PEOPLE cuts off a good deal of light, necessitating a longer exposure. The following extract is from an article in the Photo Era of September, 1907. The secret of success . . . is to blend or vig. nette the two exposures into each other in such a way as to conceal the place where they come together. This the segment article will not always do, as it is purchased ; but it is easily made right, if large enough to permit of adjustment. The first thing to do is to divide the ground- glass of the camera into four equal parts by drawing a line across its centre when placed horizontally, and another intersecting this, when set up for perpen- dicular views. This will give a dividing-line to work by — a guide for future operations. Next put the duplicator over the front of the lens, und note how much image shows on the ground-glass. [f it gives more than what covers half of the plate it is useless, and should be returned, if possible, to the maker or dealer. If this cannot be done, cement or glue a piece of stiff, black cardboard or heavy paper over the disk, allowing it to extend over the segment one-eighth of an inch. Now see how it works. Sup- pose it does not permit the image to come up to the centre line. Then it will have to be pared down gradually, until the dark side of the ground-glass ex- tends up to within a quarter of an inch of the line. Now turn it around, so that the image is shown on the opposite side of the focusing-screen, being careful to see that both sides bring the two images together in the same way at the centre line. One will likely have now noticed the necessity for care in making APPENDIX 315 this preliminary test. One will have seen the gradual blending of the fully-lighted view, which first began about three-eighths of an inch from the centre line, and gradually lessened until the image disappeared altogether about the same distance beyond the centre. This blending is the crucial point; it either makes or mars the resulting negative. It is absolutely necessary when adjusting the du- plicator on the front of the lens to get the straight edge of the segment perfectly perpendicular or hori- zontal, according to the way one is composing the shape of the picture. Failing in this, one will have a portion of the negative unexposed. This is one of the things that this simple device leaves to the care of the operator, and on his skill in setting it depends the future of his composition. SNOW-STORMS MAXIMILIAN TOCH In the “American Annual of Photography,” 1899 To photograph the snow falling is by no means easy, unless certain conditions are obtained, and even then, it is to be remembered that carelessness in develop. ment will obliterate the flakes. To begin with, it is impossible to photograph the snowflakes against a sky background. . . . Bear- ing this in mind I selected a spot where the back- ground was a row of brick houses, and against which the white flakes stood out. . . . The picture was taken in one-fiftieth of a second, and it came up in the developer as easily as if it had had a second or two. I took five more the same day, but with the exception of one other they were monstrosities. There was one, 316 PHOTOGRAPHY FOR YOUNG PEOPLE of a man struggling against the storm, with a big um- brella, and the flakes were coming down furiously, but, alas! when I developed it his black figure was streaked and spotted with monstrous flakes which were falling between him and the camera, and they were so horribly amplified, that I discarded the nega- tive after the first print. I could have corrected the negative by retouching or by the old-time “fake” of spattering water colour with a tooth-brush, but had I done that, this article would never have been written. I advise every camerist to try snow-storm pictures next winter, but be sure and photograph the scene against a dark background, and get under a shed or an awning, if possible, so that no flakes will fall near the lens and spoil the effect of the picture. SHORT HINTS MISCELLANEOUS FORMULAE, FROM CRAMER'S MANUAL NEGATIVE WARNISH Best grain alcohol . . . . . . . . . . . . . . 20 OzS. Crushed dark shellac . . . . . . . . . . . . . 1 oz. Shake occasionally for several days until dissolved (without heat). Allow it to settle, then decant care- fully from the settlings, and add two drachms of oil of lavender. The negative should be slightly warmed before warnishing. DEAD-BLACK WARNISH Alcohol . . . . . . . . . . . . . . . . . . . 8 OzS. Lamp black . . . . . . . . . . . . . . . . . . 3 oz. Liquid shellao . . . . . . . . . . . . . . . . 1 OZ. APPENDIX 317 FOR RETOUCHING Powdered rosin . . . . . . . . . . . . . . 60 grains. Oil of turpentine . . . . . . . . . . . . . 5 OzS. Moisten a clean cotton rag, and rub over the parts of the negative to be retouched. HARDENING SOLUTION Water . . . . . . . . . . . . . . . . . . 30 Ounces. Formalin . . . . . . . . . . . . . . . . 1 ounce, Immersing the negative a few minutes in this solu- tion will render the gelatine perfectly insoluble, so that the negative can be dried by artificial heat. HOW TO PRINT SUCCESSFULLY FROM A CRACKED NEGATIVE Every one knows that a crack prints a black line bordered by a white line. This crack ran through the centre of the plate, so I made an exposure with the crack horizontal, the heads of the group point- ing upward, and when half printed I reversed the frame, making the heads point downward, thus com- pleting the exposure. In this way I made perfect prints. If what was the white line in the first half of the printing should begin to show darker than the original dark line before the exposure is com- plete, reverse the frame again until this disappears. If the crack shows in the least, it is the fault of the printer. I have not tried this plan with artificial light printing, but should think it will be even simpler by that process, as the time can be divided to a second. 318 PEIOTOGRAPHY FOR YOUNG PEOPLE I consider, however, that the crack should be kept at the same relation to the light in every respect, in the second as in the first half of the exposure. If the crack runs diagonally, I think it will not matter, provided the condition is entirely reversed.— The Amateur Photographer. HOW TO PRINT FROM A WET NEGATIVE Oftentimes a print is wanted in a great hurry ; this happens frequently in newspaper work. Prints can be obtained from wet negatives on gaslight paper by wetting the paper for a few seconds and then placing it carefully on the film side of the wet negative, smoothing it down with the hand to in- sure perfect contact. Make the exposure without the use of the printing frame. After exposure, the negative with the paper still on it should be placed in water, when the two will sepa- rate without harm. The negative should of course have been carefully washed to remove all hypo remaining from the fixing bath.-The Cyko Manual. TEST FOR HYPO IN WASH WATER Permanganate of Potash . . . . . . . . . . 3 grains. Caustic Soda . . . . . . . . . . . . . . . 15 grains. Water . . . . . . . . . . . . . . . . . . 16 ounces. | A few drops of the water to be tested are mixed with an equal quantity of this solution. If hypo is present, the red colour will change to green.—The Cyko Manual. APPENDIX 319 PASTE FOR MOUNTING Dissolve a handful of ordinary gloss starch in just enough cold water to make a thick solution. Pour boiling water into this until it thickens. Set aside to cool before using.—The Cyko Manual. A GUIDE TO FOCAL LENGTH If a print be moved backward and forward be- fore the eyes it will be found that there is a point at which it becomes more stereoscopic than at any other, and the distance of the print from the eye at that point is exactly the same as the original focal length of the lens which took the photograph.- American Photography. TO FIND THE FOCAL LENGTH OF A LENS Make two images of any object of convenient length, so that the difference between the images will be equal to some part of the object, making the position of the ground-glass on the base of the camera where each image is in focus. The distance between the two posi- tions of the ground-glass thus found will be the same part of the focal length that the difference of the two images is of the object. Examples: With two images of a foot rule, let one image be eight inches long and the other four inches. The difference being one-third the length of the ob- ject, the distance between the two positions of the ground-glass will be one-third of the focal length of the lens.—American Annual of Photography, 1899. 320 PHOTOGRAPHY FOR YOUNG PEOPLE TO CALCULATE THE FOCAL FRACTION OF STOPS FOR LENSES Divide the focal length obtained by the above method expressed in inches and hundredths, by the diameter of stop opening expressed in hundredths of an inch.-American Annual of Photography, 1899. TO CLEAN A LENS First spread upon a table a clean sheet of paper; take your lens carefully apart; now dust with camel's-hair brush each lens on both sides; then take a clean gradu- ate, pour in two ounces of distilled water, one ounce of alcohol and three drops of nitric acid (C. P.) mix well, and with a tuft of filtering cotton dipped in this solution, rub the lens on both sides; polish with a clean chamois which is kept for this purpose only, which when not in use, put away in a clean paper bag. After the lenses are all polished, before putting together, wipe out carefully the brass tube; then dust each lens with a camel's-hair brush (never blow on them) and put to- gether. A lens cleaned in this way will keep clean much longer than it would, if simply wiped with a chamois.-‘‘The Art of Megative Making ” (M. A. Seed Co.'s pamphlet). PORTRAITS WITH THE NO. 3 KODAK With a No. 3 Folding Pocket Kodak and Portrait Attachment you should focus as follows: To work at 2 ft. 8 in. set focus at 6 ft. { { ( & 3 { { { { { 8 { { { { $ 4 { { 3 4 4 4 4 { { { { 15 { { { { * { { { 4 { * 4 & { { { { 25 { { { { § { { { 4} { { { { { { { { 100 { { In each case the distance is to be measured from lens to subject.—Aodak Pamphlet. APPENDIX 321 CONTINENTAL STOPS AND THEIR U. S. gº EQUIVALENTS Mr. Edward M. Nelson says: “Photographers are frequently troubled by the Continental nomenclature of the stops, and wish to know the U. S. equivalents for them. The method of finding this out is very simple. All that is necessary is to divide fº by the ratio to be converted, and square the result. Ex- ample: required the U. S. equivalent of f.9 : — & 9 {{ } = {x} = 2.25; the square of 2.25 is 5.06, the U. S. number required. — The British Journal Photographic Almanac, 1907. RULES FOR CHANGING DEGREES IN ONE THER- MOMETER SYSTEM TO ANOTHER C. = Centigrade. F. = Fahrenheit. R. = Reaumur. C. to F. Multiply by 9, divide by 5, add 32. C. to R. Multiply by 4, divide by 5. F. to C. Subtract 32, multiply by 5, divide by 9. F. to R. Subtract 32, divide by 9, multiply by 4. R. to C. Multiply by 4, divide by 5. R. to F. Multiply by 9, divide by 4, add 32. INDEX Index ABERRATION, chromatic, spherical, I40 Achromatic lenses, 229, 242 Acids, in chemistry, 273-275 Albumen papers, 2O I, 243 Alkaline developers, 256 Amateur photography, 4–9 Ambrotype, 244 Amidol, I86 Anastigmatic lenses, 147 Animals, photographs of, I 20 Antidotes to poisons (table), 289 Apparatus, improvements in, 6–8 Aristo, 25 I Aristo, Jr., 20I Aristotle, 225 Art, in photography, 96–IO5 Artificial lights, brilliancy (table), 288 Astigmatism, I42 Atomic weights, of elements (table), 290 Autochrome plates, 266 Autumn photographs, Io9 I4 I ; BASES, in chemistry, 273–275 Beccari, 229 Becquerel, 262 Bellows, the long, 156 Bennet, Charles, 246 Bi-convex lens, 144 Bitumen, 233 Blanchard, Valentine, 253 Blue-prints, 203, 3 IO Box camera, 39 Bromide, 186, 190 Bromide papers, 202 Brush development, 94 Burton, 77 CALOTYPE, 242 Camera, attachments, 42, 152–161; choice of a, 34–42; drill in use of, 47–53; modern forms of 250 ; primitive forms of, 226– 228; setting up the, 65, I 14, II 5, 12 I, I53; simplest form of, I4–16, 23; value of the, vi-viii, I— cºa Image. Cap, the, 158 Carbon papers, 206 Carbutt plates, 250 Chemical action, 218–220, 279 Chemistry, of photography, 29–30, 272-281 Chlorine, 240 Cinematograph, 255 Coal-tar developers, 191, 256 Coins, weights of (tables), 284 Collodion paper, 20I ; process, 243–245 Colour, effect of, 96–98, 99, 169; photography, 260–268 Contrast, principle of, 97–99 Cramer plates, 250 Cross-swing, 156 Curvature of field, 142 Cyko, 2O2 See IMAGE DAGUERRE, LOUIS, 225, 235-238, 24I, 256, 262- Daguerreotype, 235-238, 240–242 Dark-room, the, 54–56 Davy, Sir Humphry, 231, 239 Developers, choice of, 186, 190– 193, 294, 298–300; factors for (with tables), 295–298, 300– 3O2; quantity used, 298; special (tables), 296 Developing, apparatus for, 75; chemistry of, 29, 277–279; in Lumière process, 267 ; methods of 184–190, 232–238, 240–247, 256; papers, 92–95, 202; process of 73, 75–82, 192, 292–295 (with tables), 300–302; temper. 325 326 INDEX ature for, 78, 183–186; time of, 78, 183–186 Diaphragm, the, 49–53, 69, 166, I70–172; markings, 170, 320, 32I Distortion, I4 I Dollond, John, 229, 242 Draper, J. W., 241-243 Driffield, V. C., 176 Drop-front, 158 Drying plates, 81–82, 193; prints, 89 Dry-plate process, 245–247, 249 Du Hauron, L. D., 265 Duplicate photography, 313–315 ELECTRICITY, 212–215 Elements, chemical, 272-274, 275; and their symbols (table), 290 Emulsion, for plate, 245 Enlarging, 253 Ether, the, 2 I I ; waves, 212–216 Exposure meters, 66, 7 I, I 24, 129, 169 Exposures, length of, 41–44, 48, 5 I, 66–73, I22–125, 162–168, I78–183, 194, 292; mechanism regulating, 159; tables for, 285, 287 FACTORIAL system of developing, 184 Ferrotype plates, 91 Film-pack, 38 Films, kodak, 251 ; or plates, 36– 39; varieties of, 37. See also PLATES Finder, the, 42, IOI Fixed focus, 40 Fizeau, 240 Focal length, 164–167, 319 Focal-plane shutter, 159 Focus, depth of, 50–52; fixed, 40; for landscapes, 65; principles of, 44–46. See also FOCAL LENGTH Fog, in negative, I94 Folding camera, 39 Fox–Talbot, 241–243 Freak pictures, 269, 3 II GASLIGHT, in developing, papers, 202–2O3 93 ; Gelatine papers, 201 Gelatino-bromide process, 245 Glycerine process, 306 Goddard, 240 Ground-glass, the, 36, 38, 39 Group portraits, I 17 Gum-bichromate process, 207 HALATION, I 31–132 Halogens, 276 Heat waves, 212 Herschel, Sir John, 239, 240, 243, 262 Herschel, William, 230 Horn-silver. See SILVER COM- POUNDS Hunt, Robert, 262 Hurter, 176 Hydrochinon, 191 Hypo, 79, 88, 192, 239, 243, 275, 278; test for, 31 ILES, GEORGE, vii, 3 Image, fixing the, 24, 27 Indelible ink, 22 I Indoor photography, IO6, IO7, 122– I 32 Intensifying, 195—197; chemistry of, 278; tables for, 302–304 Interiors, I 30–132 Iodine, action on silver, 236–238 Iris diaphragm. See DIAPHRAGM Iron printing papers, 2O3–2O6 Joly process, 264—266 KALLITYPE, 205; table for, 307 Kinetoscope, 255 Kodak, the, 250, 320 ; tank de- velopment, 300–302 LANDSCAPES, distant, 65, Ioſ, I IO- I 14; near view, 65, I I4–I I7 Lantern slides, 208 Lens, the, 16-23; early use of the, 226–228; errors of the, 140–143 Lens-mechanism, 48, 154–158 . Lenses, cleaning, 32O ; different forms of, 42, I32, 143-I5 I, 165, 229, 247; speed of, 52, 148, 164–167 INDEX 327 Lewis, William, 229, 231 Light, action of, I I-I4, 16–23, 24, 28, 32, 5 I-54, 67–69, 86, I31, 177–183, 217–222, 228—238, 248, 257–259, 263, 276; and shade, 97–99, IOS–I IO, II 3, I 15, 125, I 28, 162, 168, 169; artificial (table), 288 ; laws of, 21 1–218; values, I 28, 163 (tables), 285 Lippman process, 262-264 Lithography, 233 Lumière process, 266–268 MADDOX, R. L., 245 Mansfield, George, 246 Maynard, J. P., 243–245 Measures, weights and (tables), 283 Meniscus lenses, 145 Mercury, 237 Metal quinol (M. Q.), 191 Metol, 191, 256 Microscopic objects, photographing, 268 Monckhoven, Dr., 246 Moonlight pictures, 270 Morse, S. F. B., 24 I, 242 Mountain photographs, I I I Mounting, 90 Moving objects, exposures for (table), 288; photographs of, I 18, 172–174; pictures, 253–256 Multi-speed shutter, 161 NEGATIVE, definition of, 30 Negatives, cracked, 317; destroy- ing, I98; the first, 243; fog in, I94; intensifying and reducing, I95–197, 278–280, (tables) 302– 3O4; preserving, 81, 198, 316; retouching, I97, 317; wet, 318. See also DEVELOPING ; PLATES Newton, Sir Isaac, 216 Niépce, Joseph, 233—236, 256, 261 Niépce de St. Victor, C. M. F., 243, 263 ORTHOCHROMATIC photography, Io9 ; plates, 257–259 Outdoor photography, IOG-121 Ozobrome process, 207 PASTES, for mounting, 90, 319 People, photographs of. See POR- TRAITS Perspective, in interior, 130; in landscapes, I I I–II.3, II 7 Petzval lens, 247–249 Photography, definition of, v, Io, 224; history of, 223–248; value of, vi, I-5 Piazza photographs, 127-129 Pinhole lens, 15–18, 139, 225 Plant-life, I 16, 120 Plate-holders, defects in, 62; load- ing, 53–58 Plates, developing, See DEVELOP- ING; drying, 193; essential ele- ments of, 24; or films, 36–39; injuries to, 25–27 ; inventions of, 243–247, 249 ; the Lumière, 266; orthochromatic, 257–259; preserving, 80–82, 198; selec- tion of, 60–62; sizes of, 36; speed of, 167–169; washing, 192 Platinotype paper, 203–205 Platinum process, 3O4 Poisons and antidotes (table), 289 Poitevin, 263 Porta, G. B. della, 226 Portrait lenses, 150 Portraits, IO4, 124-127; the first, 242; group, I I7 ; outdoor, I 17– I2O, with kodak, 32O Positives, 208 Priestley, Joseph, 229, 231 Principality, I I I Printing, in colours, 260–262; in- ventions in, 232–238, 240–247; methods of, 84–87, 92–95, 199– 2O9, 25 I-253 ; papers, 200–209; processes, 31, 83, (with tables) 3O4–3 Io, 318 Printing-frame, 85 Printing-out papers, 201 Prism, the, 18–21, 216 Pyro, 186, 190, 277 READE, 243 Rectilinear lenses, 146–148 Reducing, 195–197; chemistry of, 279-28o; tables for, 302–304 Refraction, 216 328 INDEX Rejlander, 252 Retouching, 197,317 Reversible back, 154–156 Revolving back, 154–156 Rising and falling front, 156 Ritter, J., 230 Rocking, in developing, 189 Roll-films, 38, 25 I ; loading with, 57 SALTS, in chemistry, 275 Sarony, Otto, 252 Scheele, C. W., 229 Schulze, J. H., 228 Science, photography in, 3, 268 Scott-Archer, 244 Seashore photographs, Io9 Seasons, effect of, Io&–1 Io Seebeck, 262 Sensitizing, 309 Sepia tones, 305 Shade, light and, 97–99, IO3–1 Io, II.3, I 15, 125, 128, 162, 168, 169 Shutter-mechanism, 48, 158–161 Silk, printing on (table), 3 IO Silver compounds, action of light on, 24, 177–183, 220–222, 228– 238, 276; nitrate, chemical com- position, 273; printing papers, 2OO–2O3, 24 I-243, 307--3O9 Sky-line, the, I 12 Snow-storm pictures, 315 Solio, 20 I Spectrum, the, 216–218 Spirit pictures, 270 Spring photographs, IO8 Stops. See DIAPHRAGM Subjects, choice of, 64, 96–105 Summer photographs, IO3 Sun, pointing camera at, I I4 Sunlight, action of, 217–222; com- position of, 215–218. See also LIGHT Swing-back, the, 154 Swing-bed, 155 TALBOTYPE, 242-243 Tank system, developing, 184 (tables), 300–302 Taupenot, 245 Telephoto lenses, 150 Thermometers, different, 321 Three-colour process, 260–262 Toning, 87; solution for, 309 Trimming, 89 Tripod, the, 12 I, I52–154 VARNISH, 316 Velox, 202, 203 View camera, 35 Views. See LANDSCAPES Vignetting, 252 Vogel, Hermann, 248 WASHING plates, 80, 192 Water, in landscape, I 16 Watkins, Alfred, 223 Wedgwood, Thomas, 231, 239, 242 Weights and measures (tables), 283 Wet-plate process, 243–245 Wide-angle lenses, 132, 149, 165 Winter photographs, Io9, 315 Wortley, Stuart, 246 GRADUATE LIBRARY DATE DUE -- * *r-servºirs •} * *„ , ! *º» º* **4 *· · · · ·~* I. · * * * t | - & # , . " - ! . w • , ! - **----------- · : ' ′ ', ¿? ??? ! **ș. • • • ***…argae****... , , , , ,; šº-· * № , CN <+ OO CN Cro Cro O O DO NOT REMOVE MUTILATE CARD ==============). *-*=============== ***æs=- =~ *===============æ, {■ *=================== *=~::~~============::= *-*=============−= *--(======,,=, *-*==+==~:=) (-)))…-…-- *-*=æ- *-*===========№s *** →→→=≡: 0,,---, *========æ→→ \,-)-, *-*============== !=w===æ*=======). *-*================= *= *s* →→→→=→ *-*==========№s ======)=)=)-; ſ-)))--~a *(==+==~::~~=====ą !=æ→===--> *-*============ --◄ t-ae-):-) *===========--- **= *======æ-◄ *=?=~=======№ { , ) --• | MAR 16 1021 UNIVERSITY OF MICHIGAN | 3 9015 |||| *ų.* · ·, , ºs ºss!!! ***(Zºº, ** ** •,,。 №. !! %± − × ° aes,§§ſë; • №*...*..* .*,,+.*):*ae ſaeº, ºſ º : ::::::::::::: $('#', 'º'.'); Ķī£.ſ.,·ſºżſſºſ ■ *- *(?:(.*)? (ºſae ·gaeg? & a º · · ·:·º·: - № · · -· №ſº), ·، ، ،- - : #:##ſſae;· ----- -· º,º (...) 、、 、№: - ·§ 3. §- * . .- !, * · ! 8 - · - -- --º ſº ºº , !‘) . ț¢ſº - - '. ~--~--~ , r.º., s.”, ſię:- · - ·· - ( ! !ſ.º aelº. --~~~~ -…--! € º.º.::::::::::::::::: ∞ √°.',- · - -· …- - , , ,•¿{ ·~ - ſ** - ºg ș.ae - ſae șae <!# }', º. ، ، ، ، ^ & - & * • • • - ≡ z º.º. a.º.:? -r, - - · №. !!!? · * №ºrſ-№yº, · · - · · · - ·- „ſaeºſ (ºſº, º - ſaeaeae£ €, , (* § (3): §§ - - - - ·¿º); e ſº: º ¿i.ſººº !ſae". . « ſº: ~--~ - · - · - (* - 3 , !· -• №ºſaeſae:ſaeſº? ¿ • №ºaeaeae; - | * * * - - ſaeſae g.!ſae º - · ſº:ſae€.¿ :', - · ·- -· - · , , , , , º· -§§:ſſä;ſaeſſae; - ∞ √° : *** ſ!!!: ---- ∞, !- ∞ √° * * ·,≤ ≤ 、。 §§§§ 4 × × × & & * „ºg“ (ſyſº ∞ √≥ſºs ∞، ، ، ، !!!! ¿ ššº: •_º.º.; ºſsºſº:- ºsſºſ 8. , , , !Mae ae::::::...', -„¿º| , ، („º,، ،§§ × × × × ×ſaeſ- ſºſiae º� && !º: ****** ș. · º ſa : ---- ∞ √° √° √ ſ ºſ ·~--~ ∞ √° √ ¿?,?,!,:, , , ,'','','','','º' ---- ſae *a| *. -), ±,±,±- · -º;, ·ºgłºſº · · · · -&. · ' * ? ºſſ, ∞:', º - sº [. [. · # *:)*)· ! № ¿? ſaeſae ¿ (ſººſ ** * * * * · ×: * ? ſae , &+, *), § 8 (º.ſ.v.ſ. ∞∞∞ - º_º_ºe.. & 3№ - - *****, , , ; **: ( ) -- · · ſ. » «, ! - - - - Eº-№.3, Hººae ) s º · T · : ? ----- - - -}, - · ·ſe º ºſſ..? ' jºſ:s sººſº ºz.ſ.ſ. ! 8 ¿??¿?, º...”; P.ſ.: ) × × × × × × ×și º 8 * !”)! ſaeºſ¿ &.* 、、 、 。 。 t. ſaes? ... ». * * *ae * # : *… !! 8 $ ¢ © ® , , , ,,,*;; № º ¿.*¿.* £ € ¥° Æ, , , , º Yº & № *…" § (3)*…* ; ; , , , º_° *** , !· º.º.º. ſ.ſ. ºſa ſaei ſae gì º, , , , !ººſſaeiſ º- *** - ºr *« »- - №º's z + : ? - · ، ، ¿? № ---- * * (?:?) ëſ), ſe º.ººº ! ,* ¿ * ( ), e º ºs º, º iſºſae *...!!!!!!!!!! * ¿? *(?:): s ºs ſa, ، ، ، :,: &.….? ¿¿.*; ºſv.); ∞ √°.', ș. a. ſaeſs);ſº;* ■ ■ ■ ■ ■ ■ ■ ſº & ! º ∞ √° ſ√≠ , , , , , £ aes · · * ~„ , , º & & ∞ √ º.º.º.· · $, e º ºeſº.º. ºſº,· ·- ■ ■ ■ ■. , º º) ſae aeſ ) { ∞ √≠√∞ √°. *** (º.ſ. aes, ****...* # : » № º∞ √°. ، ، ، ، ، ، ، :::*(, , , ■ ■ ■ ■ *** y · • × ° ſº * - ſº º º - *- *:', ¿ º ſº; !,!." aegae » º ºg „ſe ∞ √≠√∞ae. ¿¿.* №ſº (4) »,« ≡ *** !!! § * * * ****:º .*,,+.* ſº, №w , !, , , ∈ ¿?,"3":'', ';' - ، ،- · - -· · -- - ·-· - -(*)$. ≡ º.º., ſ.s.· -· ſºſ“, |- - - ∞ √° √≠ ≠ ≠ ≠ ≠ *…s : »- -… - ;*)(.* - ، ، ، ، ، ، s ≠ ≤ ≥ 333· ſº º º - ºg 23 *- » #3 -Éſ.';*$'), '$ $ º- ſºſ §. šº ! sºw_lº. ;ºsſº, aff,º)- - · ✉ ₪º : jºſſae º'r§:ſsä ſae,ºſº º ſº: :: ſe; -, *sº: · t. ∞∞∞∞ √° ſ√≠√∞º ! ·ſºſyº, ¿?! - ·:::::::::::::- ∞ √° √ · - |- º ,'$' *…ºrºſ º, , , º *, ** * * * * ſaes )ſº º …, ¿ºſ· · - ∞ ſ'effºs, - - -...º.º.º.º, , aeſººſ, - R. - · ſae?)", tvºrº, №8 |ºs,'} - ~ - *…-… ¿ ::::...º aeſ; ' * ) ſae.№ſºſ *:)*)*)(-- · w:· · · · -ſaeº. ſ.¿¿¿. ſae?), º aeſ, º ¿??¿? *) ≤ ∞ √°. · ∞∞∞####∞ √ ¡ ¿ $¢ £ € - ، ، ، ، ، ، ، 、、 、、 、 º.º. · º: , , , , , , - aevºſ žºs ºs º aes (º: º - ſae (ſ.º aee ! , , , , º - - ·„”, ſº, º . . ≤ . . ), º - -gaewºººººº!!!