quadgram

This is a table of type quadgram and their frequencies. Use it to search & browse the list to learn more about your study carrel.

quadgram frequency
the quadrant of altitude211
the number of degrees99
the elevation of the88
p m p m85
the place of the85
the superficies of the80
the meridian of the77
the degree of the77
the length of the76
the center of the75
m p m p75
the hour of the68
one and the same68
elevation of the pole65
s s s s63
the complement of the60
of the quadrant of58
place of the sun55
hour of the day53
the distance of the52
the shadow of the51
the index of the51
superficies of the dyal50
the sine of the50
index of the hour50
the day of the49
the end of the48
the axis of the47
the height of the47
the measure of the46
the poles of the45
the point of the44
the declination of the44
the middle of the43
degree of the ecliptick43
day of the moneth42
early english books online42
number of degrees of41
to the tangent of41
quadrant of altitude to41
of the poles elevation40
the arch of the39
axis of the world39
with the other foot39
the motion of the39
the altitude of the38
on the other side38
meridian of the place37
the tangent of the37
the line of contingence36
the number thought upon36
altitude of the sun35
degrees of the equator34
the top of the33
the sun is in33
on the quadrant of33
the edge of the32
in the middle of32
to the point of32
the degrees of the32
of the hour circle32
the pole of the31
the foot of the31
of the hours of31
of altitude to the31
is the number of31
the difference of longitude31
parallel to the horizon30
from the center a30
in one and the29
declination of the sun29
the points of the29
the number of the29
the plain of the29
at the end of29
pass through the meridian28
in respect of the28
the horizon of the27
houre of the day27
in the lower figure27
the diameter of the27
the same number of27
the latitude of the27
in the superficies of27
the rest of the27
the point of shadow26
of the higher figure26
the globe till the26
the axeltree of the26
foot of your compasses26
the circle of the26
of degrees of the25
one of the feet25
of one of the25
proper meridian of the25
to the sine of25
the a clock line25
from the center of25
meridian of the plane25
and with this space24
the centre of the24
about the globe till24
the proper meridian of24
the intersection of the24
the a clock hour24
one foot of your24
a clock hour line24
on the north side24
of the axeltree rod23
one of the hours23
of degrees and minutes23
which is in the23
the side of the23
the semidiameter of the23
one foot of the22
the parts of the22
screw the quadrant of22
draw a straight line22
to the point b22
the lower end of22
end of the quadrant22
hour of the night22
meridian of the plain22
axeltree of the dyal22
set one of the22
number of degrees and22
point of the horizon22
turn about the globe22
the feet of the21
the circle of position21
degree of the equator21
the east side the21
and the index of21
find the hour of21
in the circle of21
the north or south21
set one foot of21
of the lower figure21
for the latitude of21
foot of the compasse21
the cusp of the20
the east or west20
degrees above the horizon20
of the elevation of20
foot of the index20
the globe and quadrant20
poles of the world20
the heigth of the20
of the figure above20
the time of the20
the same with the20
one to the other20
into two equal parts19
and the number of19
of the second book19
to find the hour19
east side the horizon19
the north side the19
line parallel to the19
the distances of the19
to the degree of19
in a straight line19
of the equator pass19
that number of degrees19
in the same manner19
one of the points19
when the sun is18
which is all one18
between the pole and18
all sorts of people18
and quadrant of altitude18
the houre of the18
characters represented either as18
the west side the18
so much the more18
by the side of18
the lines of the18
the equator pass through18
meridian line on the18
of the feet of18
in the line of18
is equall to the18
drawn from the center18
represented either as utf18
so many degrees as18
complement of the poles18
equator pass through the18
the poles elevation above18
same number of degrees18
how to make a18
the north and south18
height of the sun18
globe and quadrant of17
point of the compass17
at the same time17
right angles with the17
it is to be17
as you see in17
lower end of the17
from the meridian of17
the sun in the17
to the east side17
plain of the horizon17
measure of the angle17
poles elevation above the17
the beginning of the17
by reason of the17
by help of a17
that is to say17
after the french way17
degrees of the equinoctial17
the east and west16
what degree of the16
and the brasen meridian16
of the meridian of16
parallel to the axis16
is the tangent of16
from the meridian line16
degrees and minutes of16
the globe of the16
the latitude of london16
the longitude and latitude16
the distance between the16
parallel to the index16
be the number of16
to the axis of16
first meridian and the16
the hour circle to16
the angle at the16
to find the rest16
every one of the16
to the latitude of16
to all sorts of16
the first meridian and16
centre of the earth16
by the help of16
come back to the15
is distant from the15
elevation above the plain15
a clock in the15
is in the zenith15
globe of the earth15
to the figure below15
from the point b15
between the first meridian15
to the meridian of15
sine of the poles15
heigth of the pole15
the points of shadow15
you see in the15
east point of the15
be the same with15
the position of the15
of the sun or15
the fiduciall edge of15
comprehended between the first15
point of the pin15
i turn the globe15
the use of the15
the line a b15
angles at the pole14
place one foot of14
of the sun in14
as you may see14
by the globes the14
a star of the14
of the fixt stars14
the globe to the14
shewing by the globes14
the pole is elevated14
the colure cut the14
the east point of14
of the pin ab14
latitude of the place14
be made to move14
on the west side14
many degrees as the14
north point of the14
the hour lines of14
and minutes of the14
the globes the solution14
the horizon and the14
the other side the14
at right angles with14
to the straight line14
the points b and14
globes the solution of14
and with the other14
the body of the14
and extend the other14
point of one of14
place of the dyal14
points of shadow cdf14
pole of the globe14
a line parallel to14
shall be the hour14
beams of the sun14
is parallel to the14
of the hour lines14
and the quadrant of14
the first point of14
the meridian line on14
what point of the14
so have you the14
on the top of14
till the index of14
measure of the side14
of the gnomonical semi13
of the compasse to13
straight ruler to the13
measure the distance of13
the placing of the13
is the same with13
on the east side13
the latitude of your13
i make a prick13
edge of the index13
it is in the13
the point in the13
the index points to13
by help of the13
number of degrees that13
but if it be13
on the south side13
compasse to the point13
the east side of13
the other foot to13
degree of the horizon13
fiduciall edge of the13
a b c d13
the making of a13
one from the other13
clock in the morning13
meridian comprehended between the13
to the complement of13
of the pin b13
the sun or star13
to the figure above13
colure to the meridian13
from the foot of13
so is the tangent13
lines from the center13
the north point of13
latitude of your place12
from the point of12
if your plane be12
of the pole above12
the sine of gr12
other foot of the12
you must turn the12
passes through the meridian12
line on the ceeling12
the radius of the12
and set it from12
pole of the world12
of the sun to12
in the center of12
horizon of the place12
go to the figure12
is elevated above the12
in the meridian line12
point in the horizon12
and screw the quadrant12
use of the globes12
be the hour lines12
foot of the compass12
the gnomonical semi circle12
to the elevation of12
on the right hand12
at right angles to12
i elevate the pole12
the line of the12
and there make a12
count the number of12
the sun and moon12
in the figure below12
the difference of the12
of the first meridian12
superficies of the dyall12
of the latitude of12
side of the quadrant12
which shall be the12
by how much the12
your line of chords12
for the making of12
of the half circle12
the point of one12
to finde out the12
the point b of12
lines drawn from the12
the compasse to the12
poles of the ecliptick12
is the distance of12
the houres of the12
east side of the12
elevated above the horizon12
globe till the index12
are the distances of12
a line of sines12
and the degree of12
images scanned from microfilm11
edge of the quadrant11
zenith line of the11
line of the plain11
to the line of11
find the colure cut11
the center of your11
keyboarded and encoded edition11
even for commercial purposes11
till the index points11
placing of the axeltree11
sine of the latitude11
of degrees that the11
that it may be11
draw a line parallel11
support to the early11
this keyboarded and encoded11
encoded edition of the11
upon the horizontall plain11
to the end of11
from proquest page images11
the work described above11
the beams of the11
degrees of the quadrant11
in a right line11
the pole above the11
the motions of the11
of the suns declination11
the early english books11
english books online text11
sun is in the11
markup reviewed and edited11
this phase i text11
therefore i elevate the11
the equinoctial and the11
be parallel to the11
the cursor of the11
point i of the11
text is available for11
of the equinoctiall circle11
on the terrestrial globe11
is available for reuse11
into the equinoctiall circle11
in the middle rule11
terms of creative commons11
the pole and the11
set off that distance11
keyed and coded from11
upon the hour of11
is the measure of11
all without asking permission11
height of the style11
it is easie to11
phase i text is11
according to the terms11
complement of the elevation11
the text can be11
and setting of the11
the institutions providing financial11
the right ascension of11
side of the plane11
of the work described11
institutions providing financial support11
to one of the11
of the number of11
tcp assigned for keying11
by the institutions providing11
financial support to the11
then i turn the11
houre points of the11
comprehended between the pole11
in the place of11
with this space come11
to the early english11
it ought to be11
these are the distances11
longitude and latitude of11
the terms of creative11
which in this example11
parallel to the line11
of the ecliptick is11
what place of the11
a table of the11
point b of the11
of the equator at11
degrees of the horizon11
encoded text transcribed from11
providing financial support to11
is a great circle11
of the parts of11
coded from proquest page11
the secant of the11
if it be a11
to the terms of11
assigned for keying and11
described above is co11
i text is available11
of the compasse upon11
ruler to the center11
text can be copied11
for keying and markup11
books online text creation11
line at right angles11
and coded from proquest11
work described above is11
from the point d11
from the proper meridian11
space come back to11
owned by the institutions11
the meridian line of11
proper to the plain11
and the same point11
text and markup reviewed11
as in the figure11
length of the day11
points to a clock11
to the height of11
online text creation partnership11
the tangent of gr11
in the point of11
the longitude of the11
a straight ruler to11
and markup reviewed and11
place of the earth11
edition of the work11
meridian and the brasen11
the meridian altitude of11
erect direct south dyal11
for example in the11
and encoded edition of11
perpendicular to the plain11
be the measure of11
and set off that11
by the coelestial globe10
the surface of the10
distances of the hour10
in the air i10
the equator at the10
bring the place of10
you have drawn about10
by the shadow of10
at the top of10
a dyal upon a10
to make an erect10
a pair of compasses10
and from the point10
the side a c10
points of the equinoctiall10
be made about the10
and use of the10
degrees contained between the10
that you have drawn10
rectifie the globe to10
line on the floor10
and from the center10
by so much the10
is the sine of10
in the latitude of10
is the elevation of10
of the superficies of10
made on the globe10
draw lines from the10
is to be noted10
comes to the meridian10
a line of chords10
on both sides the10
of altitude comprehended between10
day of the month10
altitude comprehended between the10
the beames of the10
part of the meridian10
upon the plain of10
the double of the10
perpendicular to the straight10
quadrant of altitude in10
arch of the quadrant10
one of the ends10
motion of the sun10
of the sun for10
find the heigth of10
how to make an10
index or zenith line10
to the place of10
turn the globe till10
to find by the10
distance of the meridian10
equall to the angle10
the bottome of the10
as you were taught10
to the west side10
is to the radius10
the point where the10
a paire of compasses10
the reclination of the10
to the center of10
to the right hand10
according to the quantity10
how to make the10
of the points of10
how is it that10
of the sun and10
of the plains latitude10
side of the horizon10
go back again to10
may be made to10
make an erect direct10
west side the horizon10
of the difference of10
quadrant of altitude comprehended10
in such sort that10
to the day of10
to find the heigth10
reclination of the index10
one of the sides10
upon the terrestrial globe10
point in the air10
i would know the10
draw the line a10
it may be done10
height of the pole10
line shall be the10
three points of shadow10
with a paire of10
the sun to the10
draw with the other10
have drawn about the10
back to the figure10
example in the point10
drawn about the point10
back again to the10
this space come back10
an arch of the10
between the equinoctial and10
the point of concourse10
to the horizon of10
based on the new9
and these are the9
the zenith and the9
must meet with it9
upon the superficies of9
aware of the process9
of the side a9
index points to a9
filling in of gaps9
encoded texts based on9
or tei g elements9
feet of the compasse9
created by converting tcp9
was divided into two9
in english were prioritized9
perpendicular to the horizon9
from the east point9
in oxford and michigan9
text with mnemonic sdata9
the tei in libraries9
creation partnership web site9
it to be the9
likelihood such instances will9
or corrected and characters9
of the suns course9
with mnemonic sdata character9
notably latin and welsh9
teams in oxford and9
to the east point9
a clock at night9
the text encoding initiative9
restraints of time and9
corrected and characters marked9
changes to facilitate morpho9
assumptions that can be9
on the new cambridge9
and there i make9
a works in english9
should bear in mind9
sine of your latitude9
work was chosen if9
texts based on the9
is to encode one9
was intended to range9
out by editorial teams9
based on the text9
released into the public9
selection was based on9
ecliptick the sun is9
while the overall quality9
with level of the9
at the text creation9
extent have been transformed9
all likelihood such instances9
point of the needle9
respectfully request that due9
project have been released9
in the straight line9
been looked at by9
transcription and basic encoding9
of any assumptions that9
as opposed to critical9
bear in mind that9
to range over a9
of your compasses in9
copies of the texts9
have been transformed into9
elements of known extent9
now take and use9
of tcp data is9
as illegible were corrected9
so much as the9
meet qa standards were9
limit of instances per9
and some readable characters9
transformed into placeholder characters9
given to their original9
the universities of michigan9
of the project have9
sent to external keying9
or which is all9
during phase of the9
general aim of eebo9
the overall quality of9
a compelling reason to9
and characters marked as9
the notches of the9
to produce large quantities9
but the number of9
of the ecliptick the9
with changes to facilitate9
for an anonymous work9
the text creation partnership9
sets were sent to9
publisher proquest to create9
of known extent have9
tcp is to encode9
the process of creating9
public domain as of9
and are to be9
a clock it is9
whichever is the greater9
is represented by the9
therefore chose to create9
companies for transcription and9
of the texts have9
is the length of9
for their own purposes9
into placeholder characters or9
can now take and9
but we respectfully request9
those which did not9
have been looked at9
on the image sets9
proquest to create accurately9
to the length of9
known extent have been9
text strings within braces9
of creating the tcp9
project restraints of time9
for transcription and basic9
external keying companies for9
be marked as illegible9
and encoded texts based9
circle of the horizon9
sets published by proquest9
lines shall be the9
text selection was based9
tcp data is very9
to their original source9
at the hour of9
were corrected where possible9
works are eligible for9
to the keyers to9
texts have been issued9
the project have been9
characters will be marked9
compelling reason to do9
was chosen if there9
to simplify the filling9
edition of a work9
in the first place9
nature of the print9
keying companies for transcription9
never have been looked9
on the left hand9
errors will remain and9
creating the tcp texts9
some errors will remain9
that point of the9
elements to simplify the9
their early english books9
accurately transcribed and encoded9
tei in libraries guidelines9
the usual project restraints9
the suns declination is9
line of the place9
up into the equinoctiall9
editorial teams in oxford9
published by proquest via9
of degrees from the9
therefore of any assumptions9
editions of a works9
not meet qa standards9
been released into the9
to page images in9
bring the lower end9
was proofread for accuracy9
the suns declination and9
will remain and some9
number of degrees contained9
tcp is a partnership9
credit and attribution is9
are eligible for inclusion9
divided into two phases9
was placed in heaven9
linked to page images9
a limit of instances9
should make clear that9
the print record of9
right ascensions and declinations9
page images in accordance9
the keyers to be9
north and south line9
vnto every pound of9
the halfe of it9
second or later edition9
range over a wide9
mind that in all9
elevation of the index9
accordance with level of9
of the print record9
the index or zenith9
and the arch of9
structural encoding based on9
a wide variety of9
phase of the project9
was then carried out9
produce large quantities of9
unicode or text strings9
the texts have been9
and use these texts9
encoded as gap s9
any remaining illegibles were9
or text strings within9
should be aware of9
of a works in9
of degrees contained between9
language title published between9
illegibles were encoded as9
tcp aimed to produce9
length of the night9
was based on the9
the hour of sun9
of michigan and oxford9
as it ought to9
the encoding was enhanced9
in this example is9
it must meet with9
to external keying companies9
to make a dyal9
the publisher proquest to9
up to a limit9
remain and some readable9
the texts were encoded9
the plains proper meridian9
mnemonic sdata character entities9
works in other languages9
diameter of the earth9
chose to create diplomatic9
be aware of the9
based on the image9
wide variety of subject9
cambridge bibliography of english9
west side of the9
you may see by9
then measure the distance9
index be made to9
and or corrected and9
draw with the rule9
corrected where possible up9
and therefore chose to9
s s p m9
process of creating the9
between and available in9
over a wide variety9
or for an anonymous9
returned to the keyers9
that can be made9
print record of the9
then carried out by9
for it must meet9
in the time of9
title published between and9
proquest via their early9
published between and available9
keyers to be redone9
been transformed into placeholder9
any assumptions that can9
texts created during phase9
domain as of january9
to the points of9
of every monographic english9
text was proofread for9
will be marked as9
bring the quadrant of9
the south side the9
have been issued variously9
distance from the meridian9
all the hour lines9
texts for their own9
qa standards were returned9
gap elements of known9
a work was chosen9
assurance was then carried9
transcribed and encoded texts9
new cambridge bibliography of9
first editions of a9
to a limit of9
were encoded and linked9
image sets were sent9
users should bear in9
as the sine of9
quality assurance was then9
characters marked as illegible9
are a number of9
mainly structural encoding based9
instances will never have9
the art of painting9
files to tei p9
is the complement of9
data is very good9
was a compelling reason9
intended to range over9
we respectfully request that9
image sets published by9
possible up to a9
the new cambridge bibliography9
to finde how much9
point of shadow f9
and in the other9
a second or later9
will never have been9
tei p using tcp9
these texts for their9
opposed to critical editions9
encoding based on the9
quality of tcp data9
a number of works9
attribution is given to9
reason to do so9
what a clock it9
that due credit and9
data within the usual9
were sent to external9
and the publisher proquest9
tcp files to tei9
the ecliptick the sun9
simplify the filling in9
sometimes a second or9
the fourth part of9
in the art of9
is a partnership between9
in the same time9
level of the tei9
their works are eligible9
usual project restraints of9
remaining illegibles were encoded9
were returned to the9
did not meet qa9
or elements to simplify9
of textual data within9
these processes should make9
iv tiff page images9
and available in eebo9
take and use these9
by proquest via their9
for accuracy and those9
been issued variously as9
elevate the north pole9
understanding these processes should9
to the radius of9
available at the text9
in mind that in9
of a work was9
by converting tcp files9
in accordance with level9
project was divided into9
where possible up to9
some readable characters will9
point through which the9
into the public domain9
can be made about9
request that due credit9
included and sometimes a9
via their early english9
true nature of the9
parallel to the equinoctial9
there was a compelling9
the face of the9
of the tei in9
within the usual project9
such instances will never9
the filling in of9
reflect the true nature9
issued variously as sgml9
keying and markup guidelines9
partnership between the universities9
or later edition of9
and markup guidelines are9
guidelines are available at9
an erect direct south9
nearest to the point9
encoding was enhanced and9
and so of the9
by university of nebraska9
of day and night9
create accurately transcribed and9
markup guidelines are available9
texts were encoded and9
anyone can now take9
number of works in9
line bd of the9
is given to their9
to the lower figure9
upon the cusp of9
carried out by editorial9
in what place of9
made about the data9
and oxford and the9
gaps by user contributors9
placeholder characters or elements9
to reflect the true9
at by a tcp9
a partnership between the9
the image sets published9
were encoded as gap9
large quantities of textual9
record of the period9
processed by university of9
to encode one copy9
are available at the9
standards were returned to9
of the process of9
later edition of a9
due credit and attribution9
illegible were corrected where9
created during phase of9
of works in other9
characters or elements to9
the general aim of9
and linked to page9
enhanced and or corrected9
parallel to the meridian9
users should be aware9
the true nature of9
marked as illegible were9
the west side of9
on the text encoding9
chosen if there was9
come to the meridian9
processes should make clear9
between the two places9
universities of michigan and9
works in english were9
have you the number9
of gaps by user9
the reason of the9
text creation partnership web9
converting tcp files to9
of each text was9
and transfer that distance9
have been released into9
encoded and linked to9
by a tcp editor9
readable characters will be9
and so you have9
and sometimes a second9
point of the compasse9
oxford and the publisher9
tcp project was divided9
in all likelihood such9
accuracy and those which9
and therefore of any9
the side a b9
between the universities of9
of time and funding9
between the zenith and9
plain of the equinoctiall9
textual data within the9
each text was proofread9
p using tcp tei9
bibliography of english literature9
was enhanced and or9
place in the ecliptick9
variety of subject areas9
s s s p9
to finde which of9
usually the first edition9
quadrant of altitude shall9
sine of the elevation9
the public domain as9
if there was a9
proofread for accuracy and9
aimed to produce large9
quantities of textual data9
michigan and oxford and9
to create diplomatic transcriptions9
looked at by a9
overall quality of tcp9
unicode or tei g9
although there are a9
by editorial teams in9
s p m p9
of instances per text9
the other foot draw9
to tei p using9
lines of the hours9
in of gaps by9
images in accordance with9
there are a number9
and attribution is given9
ascii text with mnemonic9
then their works are9
use these texts for9
to create accurately transcribed9
that in all likelihood9
which did not meet9
selection was intended to9
and those which did9
have it to be8
with the meridian line8
point at the hour8
the quantity of the8
to the meridian with8
through the notches of8
light of the sun8
the line bd of8
if you desire to8
from the noon line8
ocm this keyboarded and8
the mouth of the8
the sun above the8
will have it to8
of the longest day8
when the shadow of8
of the ecliptick on8
from the brasen meridian8
plane of the horizon8
hours after the french8
by little and little8
the hours after the8
for which account onely8
degrees on the quadrant8
onely but the number8
the meridian in the8
the meridian line ns8
account onely but the8
of the sun is8
reproduction of original in8
from west to east8
the upper end of8
you will have the8
one side or other8
altitude to the degree8
the point i of8
center of the equinoctial8
shadow of the index8
the sun comes to8
with this space go8
of the world is8
description and use of8
by joseph moxon hydrographer8
in the first meridian8
at one and the8
upon what point of8
parallel to the equator8
and draw the line8
shall be the number8
it will not be8
to the index or8
from the center o8
the parallel of the8
in the zenith line8
that the earth is8
the remainder is the8
of the equator that8
the space from the8
then turn about the8
estc r ocm this8
number of the hundreds8
found by the globe8
so is the sine8
set down in the8
which is proper to8
circle of the point8
your compasses in the8
place to the meridian8
the nearest to the8
one of the two8
center of the quadrant8
to the hour of8
point of shadow d8
sun above the horizon8
shadow upon the hour8
in the second figure8
and the first meridian8
be equal to the8
make marks in the8
you the number thought8
this space go to8
upon the equinoctiall plain8
the degree and minute8
how to finde the8
counted from the zenith8
r ocm this keyboarded8
angle at the pole8
the same distance from8
to the proper meridian8
the three points of8
and turn the globe8
right ascension of the8
if you would know8
and let it be8
as may be seen8
if you have been8
the meridian with the8
or tangent of gr8
i find the colure8
to the point o8
the zenith line of8
as was said before8
let fall a perpendicular8
center of the dyal8
of the compass upon8
the parallels of the8
of the sun above8
that it may not8
in which the sun8
foot of the compasses8
the manner of the8
one foot in the8
till you come to8
of the first figure8
divided into equal parts8
points of shadow c8
at the intersection of8
to every one of8
as long as you8
the ecliptick on the8
meridian altitude of the8
of the hundreds viz8
make a dyal upon8
on the line of8
is the declination of8
so that it may8
see in the figure8
from the point o8
out of the glasse8
which account onely but8
line from the point8
a quarter of an8
a line from the8
point of shadow c8
rising and setting of8
the north pole is8
quadrant of altitude and8
the places of the8
notches of the horizon8
middle of the gnomonical8
of the brasen meridian8
the index be made8
elevate the pole of8
the houre points of8
m p m horizo8
the side b c8
or other of the8
to the quantity of8
by this means you8
shewing the making of8
is to be made8
between the horizon and8
zodiac is to be7
right angles to the7
your compasses at the7
feet of the compasses7
to move upon the7
beames of the sunne7
of the equator passes7
of the angle c7
is the point of7
the suns place in7
declination of the index7
number on the quadrant7
first meridian comprehended between7
the place where you7
to the axeltree rod7
you may find the7
of the second magnitude7
in its true position7
setting of the stars7
degree and minute of7
into twelve equal parts7
an east and west7
same distance from the7
and the meridian of7
find the height of7
upon the poles of7
is perpendicular to the7
if the sun be7
to the top of7
quadrant of altitude rectified7
and the axeltree of7
on that side the7
the suns place given7
to find the right7
is to the tangent7
the other foot a7
setting of the sun7
the other side of7
the unformed stars belonging7
the horizon in the7
to draw a dyal7
the number of cards7
pole and the horizon7
meridian through the notches7
even with the space7
the afternoon hour lines7
if the index be7
of the horizon the7
to the end that7
opposite to the degree7
to finde the houre7
of the angle b7
the index a b7
or degree of the7
of the length of7
the plain it selfe7
with a pair of7
the number of leagues7
and the rest of7
then turn the globe7
the sun moon or7
which suppose to be7
ecliptick on the cusp7
quadrant of altitude the7
to those which are7
you have been exact7
to finde a number7
long as you can7
and latitude of the7
upon the quadrant of7
the point the sun7
a shadow upon the7
to the number of7
counting them by and7
azimuth of the sun7
the difference of right7
the north part of7
to be the same7
of the dyal is7
arch of a circle7
hour lines must be7
of the point b7
the zodiac must be7
a part of the7
meridian line of the7
as i have said7
placed in the heaven7
superficies of the earth7
for that is the7
that part of the7
the diameter of a7
the longest day is7
when you would find7
in forme of a7
the help of the7
of the sun given7
on the first meridian7
a straight line from7
to the secant of7
the line of declination7
right ascension and declination7
the equator passes through7
you may see the7
have the sun in7
upon one of the7
of the dyal plane7
equator passes through the7
through which the ellipsis7
degree of the meridian7
shall be the measure7
that are in the7
of the day given7
notes for div a7
the latitudes of the7
this other foot of7
upon the foot of7
star or degree of7
of the moneth given7
the variation of the7
the circles of the7
the bottom of the7
bring it to the7
and so of others7
all the rest of7
is it that a7
upon the point of7
it will be a7
minutes of the equinoctial7
your plane be a7
with the help of7
the contents of the7
back to the lower7
the quadrant on the7
the center of this7
so of the rest7
of the meridian line7
the sun being in7
may go and meet7
at the beginning of7
the nature of the7
of the sun at7
the vernal colure to7
is the nearest to7
of the earth the7
the figure of the7
so is the co7
bring that degree to7
the verticall of the7
when the sun shines7
of the poles of7
arch of the first7
towards the right hand7
of the globe to7
on the cusp of7
as a tangent of7
the points of hour7
double of the number7
to find in what7
point of the globe7
is the difference of7
invented and written by7
that the shadow of7
part of a circle7
to the meridian line7
and put it into7
to the left hand7
it to the meridian7
plains difference of longitude7
by the third probleme7
draw a line from7
and to find the7
at the foot of7
arch of the meridian7
of the day and7
and its opposite degree7
of the proper meridian7
to the edge of7
and bring it to7
b of the pin7
the plains difference of7
chuse a point in7
be made on the7
number of degrees between7
bring the first point7
is to the sine7
north part of the7
space go to the7
extend the other foot7
the north side of7
the sun or any7
to the point d7
of the nature of7
suns place to the7
it come to the7
verticall of the plane7
the tropick of cancer7
that degree to the7
a figure of heaven7
it is evident that7
and according to the7
to find out the7
sun or any star7
circle of the equinoctial7
seasons of the year7
therefore i say the7
of the suns altitude7
so shall the triangle7
degrees counted from the7
and one of the7
of your line of7
by the motion of7
therefore it containeth it7
which is the complement7
for the most part7
by substracting the lesser7
the other in the7
number of degrees from7
the suns place to7
will be the same7
there i make a7
cast a shadow upon7
with the rule by7
feet of the compass7
i screw the quadrant7
in the line qop7
laying a straight ruler7
parallel to the perpendicular7
declining from the south7
is the degree of7
from the north point7
and through the point7
hang in the aire7
the dyal in the7
that may go and7
the description and use7
and draw a line7
the angle of the7
through the center of7
when you have thus7
bd of the lower7
the first meridian comprehended7
are to be sold7
from the center through7
number of degrees the7
comming from the center7
in his book of6
to the suns place6
minutes of the equator6
the meridian through the6
a straight line parallel6
a number thought upon6
you are to draw6
the hour lines must6
by the rule of6
to the horizontal line6
as in the first6
the number of hours6
the azimuth of the6
may meet with the6
is the same in6
time of the year6
if you have done6
globe westwards till the6
which in the east6
the star or degree6
space from d to6
time of sun rising6
the horizon opposite to6
and the point of6
there shall be a6
the latitude of a6
to the succession of6
the true place of6
shew the true houre6
the center a through6
degrees below the horizon6
which is perpendicular to6
points of the hours6
be supposed to be6
the meridian and the6
the obliquity of the6
in regard of the6
to the knowledge of6
distance between the two6
the zenith of the6
distances of all the6
according to the succession6
to the center a6
turn the quadrant of6
the points d and6
at the signe of6
the situation of the6
untill it be full6
in the figure above6
be a line of6
pole is elevated above6
the west must be6
of longitude and latitude6
about the point d6
of any star given6
draw a meridian line6
marks in the line6
as if it were6
the side of it6
in the poles of6
the top of it6
for the length of6
the sides of it6
till it come to6
of degrees between the6
find a meridian line6
equator at the meridian6
the art of navigation6
global keyed and coded6
compasse upon the points6
be equall to the6
by the last probleme6
are said to be6
be ground very fine6
to the subindicall line6
of shadow c and6
for the a clock6
that distance in the6
the center of it6
rectifie the globe and6
the graduated edge of6
as you see the6
lay a straight ruler6
which the sun is6
of the suns rising6
in respect of your6
bright star in the6
to the globe of6
from the point m6
the equator on the6
double line of sines6
the length of a6
superficies and the axeltree6
turn the globe eastwards6
that there is no6
on the contrary side6
number of hour lines6
a point in the6
the center of a6
vernal colure to the6
and set one foot6
in the substilar line6
be found by the6
from the centre of6
so shall the degree6
of the horizon opposite6
east and west line6
find by the coelestial6
the hole of the6
at right angles in6
as far as the6
towards the east or6
by how much it6
upon the point d6
of leagues you have6
east and west diall6
points b and d6
of the shadow of6
parts of the world6
then place one foot6
of the ecliptick that6
of the third magnitude6
side of the meridian6
the ends of the6
upon the edge of6
to take altitudes by6
from the middle of6
screwed to the zenith6
ascension of the sun6
is to the globe6
upon the center a6
that which is in6
north side of the6
almicantar of the sun6
a bright star in6
there make a prick6
from east to west6
the houre lines of6
foot of the style6
be a point through6
of the place of6
after the same manner6
the help of a6
line shall be drawn6
compass to the point6
of the compass to6
so shall the index6
xii a clock line6
it comes to the6
of the quadrant to6
of your compasses at6
this is to be6
magnitude is to the6
let there be a6
the space from d6
and so much the6
of the other hours6
and in the same6
for the placing of6
diameter of the circle6
and on the other6
parallel of the suns6
spi global keyed and6
made for the latitude6
b of the axeltree6
and at the same6
and if there be6
of altitude in the6
every pound of powder6
straight line parallel to6
horizon of the world6
the number of years6
cut the quadrant of6
the globe westwards till6
be numbred from the6
length of the zodiac6
take altitudes by the6
other foot to the6
sharp at both ends6
degree of the equinoctial6
of the index above6
bring the vernal colure6
you come to the6
i rectifie the globe6
number of leagues you6
with your compasses the6
the declination of a6
of the side b6
the superficies and the6
to the zenith line6
time of the day6
the rhumb you have6
to the horizontall line6
upon the top of6
the dayes and nights6
south points of the6
n s in the6
a double line of6
passeth to the point6
that may meet in6
altitude to the zenith6
the sides of the6
altitude above the horizon6
and laying a straight6
and turning this foot6
finde the secant of6
to find the height6
a point through which6
stars that are in6
of the fixed stars6
cursor of the axis6
intersection of the meridian6
side of the clinatory6
index above the plain6
difference of right ascension6
the angle d a6
degree of the suns6
be the sine of6
i count from the6
into the superficies of6
to finde the declination6
must be numbred from6
you may learn to6
on the hour circle6
which passeth to the6
altitude of any star6
pound of powder dust6
and declination of the6
you were directed to6
and the angle at6
the name of the6
the shadow of a6
again to the figure6
find the difference of6
parallels of the sun6
of the houre lines6
circles parallel to the6
and you will find6
that which passeth to6
of the last book6
the light of the6
your compasse upon the6
and to that radius6
do the like for6
which are in the6
the two points of6
the degrees and minutes6
that end of the6
it is called the6
so that the space6
and lines drawn from6
the foot of a6
a clock hour lines6
take the halfe of6
shall the index of6
may be even with6
to make use of6
each of them to6
by the terrestrial globe6
that the sun is6
the pole and zenith6
of the horizon till6
upper end of the6
of one side or6
upwards on the quadrant6
the zodiac is to6
is contained between the6
from the a clock6
is to be described6
setting one foot in6
from the meridian or6
is an arch of6
be perpendicular to the6
is seen in the6
in the west must6
the earth the sun6
as you were directed6
that which in the6
of all the other6
to the brasen meridian6
end of the pipe6
semidiameter of the equator6
the parallels of declination6
true place of the6
the shortest distance between6
is to be set6
must turn the triangle6
the shadow of that6
space from the point6
pole above the plane6
erect a figure of6
right angled spherical triangle6
shall be a point6
and bring that degree6
as for example in6
stand parallel to the6
superficies of the horizon6
zenith and the first6
the compass to the6
on both sides of6
side or other of6
shall the degree of6
the hour circle points6
the day and night6
the form of a6
an east or west6
and when the sun6
shall the triangle be6
of the table of6
suns place in the6
straight line from the6
the plain whereon the6
of the first magnitude6
for if it be6
if it be not6
when the sun comes6
the coelestial globe the6
towards the left hand6
it is supposed that6
cut the degree of6
i turn about the6
the whole art of6
upon the celestial globe6
two points of shadow6
as in this example6
sine of the plains6
the east dyal is6
degree of the quadrant6
put it into the6
in the east dyal6
how to draw a6
as you shall see6
globe to the latitude6
star on the globe6
the index above the6
fore noon hour lines5
turn the globe westwards5
between the two pricks5
equally distant from the5
of the axeltree of5
of the equinoctial comprehended5
find the day of5
as the lower figure5
shew the length of5
draw from the point5
of the index is5
semidiameter of the horizon5
practical use of the5
the index point at5
stand perpendicular to the5
how many degrees of5
it were in the5
a fixed star of5
other side the meridian5
it is a thing5
the point of inflammation5
degrees shall be the5
the equinoctial line on5
of the properties of5
find the longitude and5
with the horizon on5
after noon hour lines5
and by consequence the5
trace with the other5
any part of the5
any point of the5
according to the proportion5
is the axeltree of5
in the former figure5
upon the point c5
of the plane and5
center of the world5
if it be upon5
and at the end5
the meridian and horizon5
the upper side of5
the fore noon hour5
the ellipsis it selfe5
middle of the plane5
the other end of5
will be in the5
when you have found5
be noted that the5
by which you may5
the middle of a5
other end of the5
pin b to the5
the equator from the5
these lines shall be5
what number of degrees5
of your own horizon5
in the horizontal intersection5
through that point draw5
of powder dust adde5
or that which is5
to the line a5
line that you have5
the limitation of the5
heigth of the sun5
you have found out5
b to the point5
go and meet the5
go and mark with5
altitude to the east5
the equinoctial comprehended between5
the ecliptick shall be5
in the centre of5
finde the declination of5
of the line of5
for this other foot5
the after noon hour5
there make a mark5
according to the proper5
the opposite degree of5
other side of the5
point of a needle5
of many sorts of5
of the third figure5
sides of the clinatory5
either north or south5
north side the equator5
subindicall line r s5
meridian with the horizon5
by the quadrant of5
of hours and minutes5
to one of them5
point of the equinoctiall5
the ellipsis is to5
on one side the5
equinoctial line on the5
and the shadow of5
according to the former5
other foot draw from5
parallel to the subindicall5
center of the earth5
from the horizon upwards5
unformed stars belonging unto5
as by the second5
from the south westwards5
that side the pole5
for that number of5
an erect direct west5
those that are skilled5
of fire for the5
shall you have the5
i would know what5
that are skilled in5
in the plain of5
shall be the meridian5
against the line of5
in the other ballance5
upon the points b5
a circle divided into5
the description of the5
to be sold at5
tangent of your latitude5
the sun from the5
you may by the5
of the place be5
an erect direct east5
is no other then5
is the double of5
edge of the horizon5
the complement of your5
about the point g5
close to the stay5
one of the poles5
the hour lines from5
one point in the5
of the ecliptick which5
if you will have5
is an hour longer5
circle of the suns5
mark with the other5
the meridian between the5
shall the arch of5
if you turn the5
to hang in the5
the other parts of5
shall shew the length5
space bi of the5
and set one of5
degrees on the meridian5
quarter of the ecliptick5
such a position that5
of degrees on the5
to the quadrant of5
the horizon from the5
perpendicular to the line5
point in the middle5
are said to have5
of the circle a5
unto the diameter of5
ascension and declination of5
all parallel to the5
workmen of many sorts5
of the third book5
be answerable to the5
in the quadrant on5
open your compasses to5
as much as the5
side of the ruler5
and hour index rectified5
foot draw from the5
to the radius r5
together in one and5
above the meridian line5
north pole is elevated5
i count in the5
points of the compass5
the best way to5
go back to the5
which are called the5
and minute of the5
cut by the horizon5
circle that may meet5
radius or decimall scale5
tangent of the declination5
draw an obscure line5
be a meridian line5
pole above the plain5
of degrees of altitude5
points of the horizon5
points in the superficies5
point on the globe5
to find the longitude5
in the zenith of5
the center a of5
rhumb you have sailed5
complement of your latitude5
are parallel to the5
i elevate the north5
ellipsis is to be5
then go to the5
arch of the horizon5
or an oyled paper5
to the angle of5
the horizon is the5
it is in your5
hour lines of the5
degrees comprehended between the5
or parallel of the5
poetical stories of the5
of the second triangle5
of the pole in5
find the measure of5
other foot go and5
to the same point5
by the points b5
you intend to make5
which is upon the5
of the planes declination5
to prick down the5
be even with the5
from the latitude of5
motion of the index5
the feet to the5
may be seen in5
same number of hour5
the horizon till the5
horizon on that side5
arch of the sun5
from the top of5
at the same instant5
and south points of5
to finde the centre5
and through that point5
in the same longitude5
the horizon on that5
is equal to the5
to shew the houre5
you may do it5
therefore it containeth the5
ounces of cole dust5
which is the difference5
after the name of5
the ancient and modern5
of the place and5
it is certaine that5
was placed in the5
table of angles at5
lesser from the greater5
of a planetary hour5
of angles at the5
the time of sun5
the head of the5
a pound of water5
latitude of the index5
by means of the5
turning the globe westwards5
is said to be5
the other of the5
in the first triangle5
it is said to5
of the motion of5
your compasses upon the5
a solid body consisting5
but if it have5
from the first point5
and divided one from5
length of the shadow5
an arch of a5
to the superficies of5
draw a right line5
find the place of5
the extremity of the5
and the stilar line5
that comes to the5
make the sine of5
by the two points5
and these lines shall5
this is done by5
from the point e5
are distant from the5
have been exact in5
from the point i5
the second and third5
with the same space5
point up into the5
the definition of the5
to the point g5
of the wooden horizon5
is proper to the5
triangle be made on5
the quadrant to the5
complement of the latitude5
a right angled spherical5
two points b and5
day of the week5
is a solid body5
italian or babylonian way5
represented by the line5
other of the point5
so is the triangle5
erect direct north dyal5
in the mean time5
furthest from the point5
the first of the5
in the hour circle5
have the same distance5
those lines shall be5
the sun upon the5
number of degrees is5
in the first of5
of the three points5
that it is the5
end of the meridian5
center of the circle5
after the italian or5
may be found by5
and with the same5
it is also called5
star of the second5
north and south points5
and the remains is5
upon the middle rule5
and the points of5
the meridian with it5
latitude you departed from5
for when the sun5
the stile must stand5
the pole to the5
the compasse upon the5
by reason of its5
is mention made of5
north side the equinoctial5
in the equinoctial line5
adde the number of5
as shall be shewed5
leagues you have sailed5
and placing one foot5
to the line ab5
the horizontall plain of5
from the intersection of5
number of degrees on5
meridian under the horizon5
in or parallel to5
the triangle be made5
and if it be5
the latitude of any5
be the tangent of5
from the point c5
hour circle points to5
and if you have5
quadrant of altitude upwards5
to find the difference5
which is to be5
by the name of5
it from m to5
the distance from the5
fixed star of the5
how to find the5
to the parts of5
in the number of5
the houres after the5
is the latitude of5
to make an horizontall5
in the last probleme5
to a fourth quantity5
that they may be5
hour lines of an5
finde which of them5
the point of a5
every degree of the5
of the most eminent5
all one with the5
they are to be5
stars belonging unto this5
so shall you have5
the course of the5
the same may be5
as in the second5
of the sun from5
of the horizon i5
take the altitude of5
the index from the5
with the quadrant of5
from the first meridian5
through the meridian in5
the plane of the5
houre from the meridian5
of a fixed star5
of that which is5
and by means of5
the degree in the5
in the point b5
which is called the5
the practical use of5
to the line bd5
the lesser from the5
rockets of or ounces5
as it must be5
cut by the meridian5
of the principal places5
erect direct east dyal5
the latitude you departed5
with the compasse the5
meridian of the index5
over the substilar line5
be the point of5
finde a number thought5
lines parallel to the5
the greatnesse of the5
course of the sun5
be found in the5
in the triangle of5
a hole in the5
are contained between the5
the equinoctial between the5
of the center of5
foot of a mountaine5
to his own respectively5
every houre of the5
of the increase of5
make an horizontall diall5
the drawing of the5
the stars in heaven5
the heighth of the5
in an oblique sphear5
westwards till the index5
will give you leave5
so as it may5
as in the former5
from the line of5
of degrees is the5
complement of the plains5
and bring the lower5
opposite degree of the5
plain and easie directions5
the place from the5
of the place from5
this kinde of diall5
off that distance in5
the signe of the5
straight lines drawn from5
ascensions and declinations of5
solid body consisting of5
degree of the planes5
you must have a5
the scituation of the5
the horizon it is5
line drawn from the5
be seen in a5
to erect a figure5
the signes in the5
of the horizon of5
the space betwixt the5
upon the points d5
point of in the5
i of the axeltree5
the rule by the5
the lower figure shews5
must be in the5
divided one from the5
of the meridian and5
the italian or babylonian5
and easie directions for5
twilight in the morning5
you shall finde the5
how much it is5
degrees that the sun5
shadow of the style5
the north point in5
make right angles with5
meet in the point5
i make another prick5
of the compasses in5
the day an hour5
poles of the globe5
of the moneth in5
one side of the5
to the workmen of5
to be in the5
the triangle of prob5
so shall the arch5
day is an hour5
is to be drawn5
such sort that the5
which is the nearest5
the use of it5
places of the fixt5
be done by the5
the latitude you are5
in degrees and minutes5
the xii a clock5
foot in the center5
equinoctial comprehended between the5
to be described upon5
in a direct line5
in the following figure5
of it to the5
as was shewed in5
say that it is5
length of the longest5
then turning the globe5
side the pole is5
difference of right ascensions5
with the diameter of5
the end of it5
set it from m5
the vi a clock5
you shall find the5
all the afternoon hour5
complement of the angle5
the sight of the5
if the eye be5
many sorts of arts5
and mark with the5
the other foot go5
the rising of the5
from the beginning of5
the axeltree rod of5
the sun for that5
between the equator and5
of the point d5
you may see that5
radius or tangent of5
the work will be5
the true places of5
upon the proper horizon5
body of the moon5
observe the altitude of5
is to be understood5
horizon opposite to the5
any one of the5
the subindicall line r5
altitude of the pole5
is made by the5
circle parallel to the5
center of the plane5
place of the world5
of a vessell which5
from the axeltree rod5
to the distance of5
of them to his5
take with the compasse5
to the centre of5
equal to the three5
pots of fire for5
and set it upon5
the pin b to5
decline from the south5
lie parallel to the5
of the sun by5
and keeping the globe5
them to his own5
to the meridian and5
of the plane de5
of the other of5
slope edges of the5
of altitude and the5
the principal places in5
at the sign of5
pole of the ecliptick5
the workmen of many5
the first meridian be5
of the declination of5
there is mention made5
the th part of5
at the other end5
reclination of the plane5
find the length of5
every one to his5
to be found in5
through the middle of5
equal with the space5
from one of the5
from e to f5
place on the globe5
are skilled in geometry5
the dayes of the5
is the height of5
it is said that5
it that a man4
segment of a circle4
will shew the houre4
of the primary ellipsis4
zenith line a b4
of the pole be4
many of them as4
equall to the tangent4
discourse of the antiquity4
styles height above the4
minute in the ecliptick4
of degrees counted from4
distance in the equinoctial4
any place of the4
for rockets of or4
motion of the shaddow4
places given in the4
of the points b4
of the clock it4
sun being in the4
point the sun rises4
you see that the4
that the plumbet may4
hour lines from the4
the generall horologicall ring4
no other then a4
is best to be4
of the upright index4
of the houre distance4
the ende of the4
be the center of4
sine of the angle4
to the meridian altitude4
of altitude shall be4
or a clock line4
on the meridian the4
it must be noted4
in what number of4
of the night and4
one of the three4
above the horizon at4
shall be the several4
that may meet with4
of the aequinoctiall distance4
of the body of4
the knowledge of the4
is on the north4
or any star is4
according to the time4
you were taught in4
the distance which is4
which you are to4
from the middle rule4
latitude of the plain4
elevate the pole to4
for the help of4
equinoctial and the quadrant4
how the zodiac is4
from the north or4
each side of the4
the arches of the4
you have been very4
the variation is eastwards4
the ecliptick is elevated4
forms are pictured on4