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 sine of the | 636 |
to the sine of | 401 |
the complement of the | 370 |
the cosine of the | 293 |
the tangent of the | 265 |
the versed sine of | 202 |
to the tangent of | 201 |
on the line of | 198 |
the center of the | 188 |
is the sine of | 184 |
the line of numbers | 181 |
so is the sine | 174 |
the length of the | 164 |
the difference of the | 160 |
the line of sines | 153 |
as the sine of | 145 |
versed sine of the | 141 |
the end of the | 139 |
by the line of | 128 |
the thread to the | 128 |
the same way from | 126 |
the sum of the | 126 |
sine of the suns | 125 |
the distance of the | 122 |
sine of the latitude | 120 |
the secant of the | 119 |
the inclination of meridians | 116 |
of the line of | 113 |
as the cosine of | 110 |
the distance between the | 108 |
in the line of | 105 |
of the suns declination | 104 |
complement of the latitude | 103 |
sine of the hour | 102 |
the thred to the | 99 |
of the sines of | 97 |
the meridian of the | 96 |
sine of the angle | 96 |
the sines of the | 96 |
the time of the | 95 |
of the hour from | 93 |
the sine of d | 92 |
the line of lines | 92 |
to the other foot | 91 |
the nearest distance from | 91 |
lay the thread to | 90 |
of the suns altitude | 89 |
lay the thred to | 89 |
the elevation of the | 89 |
take the nearest distance | 88 |
the square of the | 88 |
to the cosine of | 86 |
the height of the | 85 |
p m p m | 85 |
cosine of the latitude | 82 |
reach the same way | 81 |
the side of the | 81 |
to find the suns | 80 |
to the versed sine | 80 |
the use of the | 79 |
be found to be | 79 |
the nearest distance to | 79 |
shall reach the same | 78 |
is equal to the | 78 |
m p m p | 75 |
elevation of the pole | 74 |
is the tangent of | 74 |
sine of the azimuth | 71 |
the shadow of the | 70 |
tangent of the latitude | 70 |
the latitude of the | 70 |
greater then a quadrant | 69 |
the versed sines of | 68 |
will be found to | 67 |
the declination of the | 66 |
the beginning of the | 65 |
the tangent of d | 65 |
is to the sine | 65 |
the superficies of the | 65 |
s s s s | 63 |
from the sine of | 63 |
the altitude of the | 63 |
so is the tangent | 62 |
difference of the versed | 62 |
sine of the declination | 62 |
of the versed sines | 61 |
latitude of the place | 61 |
less then a quadrant | 61 |
so is the radius | 60 |
side of the square | 59 |
of the angle sought | 59 |
the hour of the | 58 |
the hour and azimuth | 57 |
the day of the | 57 |
declination of the sun | 56 |
the east or west | 56 |
early english books online | 56 |
the hour from noon | 55 |
the cotangent of the | 55 |
to the secant of | 55 |
the azimuth from the | 54 |
when the sun hath | 54 |
take the distance between | 53 |
laying the thread to | 53 |
suns distance from the | 52 |
the suns distance from | 52 |
versed sines of the | 52 |
of the complement of | 51 |
the radius of the | 51 |
to the difference of | 50 |
in the center of | 50 |
the place of the | 50 |
to the square of | 50 |
thread to the other | 50 |
superficies of the dyal | 50 |
cosine of the declination | 49 |
is the cosine of | 49 |
hour of the day | 49 |
to the complement of | 49 |
to find the content | 48 |
of the given angle | 48 |
laying the thred to | 48 |
time of the day | 48 |
of the side sought | 48 |
is the difference of | 48 |
the point of entrance | 48 |
meridian of the place | 48 |
secant of the latitude | 47 |
the rectangle of the | 47 |
the declination in the | 47 |
the extent from to | 47 |
at the end of | 47 |
the foot of the | 47 |
that is to say | 47 |
to finde the suns | 47 |
a rule laid from | 46 |
the distance from the | 45 |
the point of the | 45 |
to find the hour | 45 |
on the other side | 44 |
so is the difference | 44 |
one foot of the | 44 |
altitude of the sun | 44 |
the radius to the | 44 |
nearest distance to it | 43 |
part of the meridian | 43 |
and draw the line | 43 |
of the azimuth from | 42 |
as the tangent of | 42 |
of one of the | 42 |
the pole of the | 42 |
versed sine of d | 42 |
nearest distance from the | 41 |
of your compasses in | 41 |
sine of half the | 41 |
the suns altitude at | 41 |
tangent of the suns | 41 |
a table of the | 41 |
the poles of the | 40 |
and with the other | 40 |
the sine of half | 40 |
to the nearest distance | 40 |
cosine of the altitude | 40 |
the middle of the | 40 |
by help of the | 40 |
the wall or cieling | 39 |
of the given side | 39 |
the thred to nd | 39 |
of the stiles height | 39 |
past in the morning | 38 |
the difference of longitude | 38 |
extent of the compasses | 38 |
of the angle at | 38 |
to sine of the | 38 |
complement of the suns | 38 |
s a a s | 38 |
you shall find the | 37 |
sine of the altitude | 37 |
from the center to | 37 |
a line of chords | 37 |
so is the cosine | 37 |
edge of the quadrant | 37 |
with the other foot | 37 |
the substiles distance from | 37 |
the sun or stars | 36 |
sines of the suns | 36 |
hour of the night | 36 |
difference of the sines | 36 |
the line of hours | 36 |
the suns right ascention | 36 |
the extent of the | 36 |
the angle opposite to | 36 |
from the center of | 36 |
one point in the | 36 |
square of the radius | 36 |
and lay it from | 36 |
substiles distance from the | 35 |
and make it a | 35 |
line of versed sines | 35 |
be equal to the | 35 |
the eleuation of the | 35 |
complement of the angle | 35 |
one and the same | 35 |
in the scale of | 35 |
and the complement of | 35 |
set one foot of | 35 |
so the tangent of | 35 |
extend the compasses from | 35 |
for the latitude of | 34 |
of the sun or | 34 |
according to nearest distance | 34 |
the axis of the | 33 |
to finde the hour | 33 |
day of the month | 33 |
the length in feet | 33 |
from the plains perpendicular | 33 |
of the substile from | 33 |
center of the quadrant | 33 |
time of the suns | 33 |
same way from the | 33 |
as the radius is | 33 |
day of the moneth | 33 |
shall reach to the | 33 |
the radius is to | 32 |
a s s a | 32 |
after the same manner | 32 |
into two equal parts | 32 |
nearest distance to the | 32 |
point of the compasses | 32 |
the suns azimuth from | 32 |
is the radius to | 32 |
from thence to the | 32 |
the content in feet | 32 |
the scale of entrance | 32 |
be less then a | 32 |
the sun is in | 32 |
the quantity of the | 32 |
of the said ark | 31 |
to the same radius | 31 |
of the hours of | 31 |
the thread over the | 31 |
when the sun is | 31 |
azimuth from the south | 31 |
table of the suns | 31 |
set one point in | 31 |
half sum of the | 31 |
line of sines from | 31 |
the intersection of the | 31 |
in the latitude of | 31 |
the line of the | 31 |
the difference between the | 31 |
of the difference of | 31 |
radius is to the | 31 |
to find how much | 31 |
the ark of difference | 31 |
distance from the meridian | 30 |
in the equal limb | 30 |
to the point of | 30 |
of the meridian line | 30 |
sine of the stiles | 30 |
foot of the compasses | 30 |
the scale of altitudes | 30 |
and so is the | 30 |
the tangent of half | 30 |
the coast of declination | 30 |
the side sought as | 30 |
the half sum of | 29 |
find the content in | 29 |
the arch of a | 29 |
the sun hath d | 29 |
is to the cosine | 29 |
then take out the | 29 |
to the radius of | 29 |
then the complement of | 29 |
to find an angle | 29 |
the thread laid over | 29 |
a line of sines | 29 |
the difference of latitude | 29 |
the line of latitudes | 29 |
so the sine of | 29 |
the right sine of | 29 |
of the compasses from | 29 |
cotangent of the latitude | 29 |
azimuth of the sun | 29 |
of a line of | 29 |
poles of the world | 28 |
the suns greatest declination | 28 |
the side opposite to | 28 |
take the distance from | 28 |
is to the radius | 28 |
your compasses in the | 28 |
taken out of the | 28 |
of the pole above | 28 |
center of the dial | 28 |
the scale and the | 28 |
to the content in | 28 |
given to find the | 28 |
sine of the side | 28 |
angle opposite to the | 28 |
the suns meridian altitude | 28 |
is the complement of | 28 |
the line of tangents | 28 |
of the ark of | 28 |
in the lower figure | 27 |
sines from the center | 27 |
the other to the | 27 |
foot of your compasses | 27 |
ark of difference between | 27 |
to find the time | 27 |
of half the angle | 27 |
the degrees on the | 27 |
but if it be | 27 |
the latitude of london | 27 |
sine of the difference | 27 |
parallel to the horizon | 27 |
at the same time | 27 |
in the sine of | 27 |
the altitude in the | 27 |
but just touch the | 27 |
arch of a circle | 27 |
be greater then a | 27 |
the top of the | 27 |
find the suns altitude | 27 |
of the stile from | 27 |
the particular scale of | 27 |
the measure from the | 27 |
be the sine of | 27 |
between the scale and | 27 |
the angle at b | 26 |
from the east or | 26 |
side opposite to the | 26 |
scale and the thread | 26 |
of the higher figure | 26 |
beginning of the line | 26 |
of the sine of | 26 |
sum of the sines | 26 |
the semidiameter of the | 26 |
the axeltree of the | 26 |
one foot of your | 26 |
to the cotangent of | 26 |
in the superficies of | 26 |
the distance on the | 26 |
the true time of | 26 |
from east or west | 26 |
line of equal parts | 26 |
of the angle opposite | 26 |
the point of shadow | 26 |
make it a in | 26 |
the azimuth of the | 26 |
the description of the | 26 |
find the time of | 26 |
suns azimuth from the | 26 |
true time of the | 26 |
line on the plain | 26 |
of sines from the | 26 |
to secant of the | 25 |
of the inclination of | 25 |
rectangle of the sines | 25 |
the logarithm of the | 25 |
to the distance between | 25 |
on the right edge | 25 |
the pole above the | 25 |
one of the feet | 25 |
half the difference of | 25 |
tangent of the angle | 25 |
which is all one | 25 |
make it a parallel | 25 |
complement of the poles | 25 |
then lay the thread | 25 |
the stile from the | 25 |
of the latitude to | 25 |
the cosecant of the | 25 |
on the left edge | 25 |
from the end of | 25 |
to draw the hour | 25 |
to the line of | 25 |
the angle of the | 25 |
if it be a | 25 |
and that shall be | 25 |
of the plains declination | 25 |
the diameter of the | 25 |
one foot in the | 25 |
pole of the plain | 24 |
thread laid over the | 24 |
the suns present altitude | 24 |
to the coast of | 24 |
in feet and parts | 24 |
length of the day | 24 |
one point of the | 24 |
in the versed sine | 24 |
the measure of the | 24 |
the points of the | 24 |
sum of the two | 24 |
the parallel sine of | 24 |
that shall be the | 24 |
foot of the compassis | 24 |
a ruler laid from | 24 |
and the opposite side | 24 |
is to the tangent | 24 |
find it to be | 24 |
so is the co | 24 |
and from the point | 24 |
of the latitude and | 24 |
tangent of half the | 24 |
at the sine of | 24 |
setting one point in | 24 |
complement of the altitude | 24 |
use of the line | 24 |
past in the afternoon | 24 |
meridian of the plane | 24 |
and with this space | 24 |
as in the figure | 24 |
the natural sine of | 24 |
of the axeltree rod | 23 |
distance to the thread | 23 |
of difference between the | 23 |
same way from to | 23 |
distance from the plains | 23 |
one of the hours | 23 |
of the compasses in | 23 |
opposite to the other | 23 |
be found in the | 23 |
other foot of the | 23 |
take out the sine | 23 |
azimuth from the north | 23 |
found to be d | 23 |
side sought as the | 23 |
height of the stile | 23 |
s s a a | 23 |
the plain of the | 23 |
the compasses from the | 23 |
the north pole is | 23 |
tangent of the declination | 23 |
lay the thread over | 23 |
line of natural sines | 23 |
thred to the nearest | 22 |
distance from the pole | 22 |
and setting one point | 22 |
complement of the declination | 22 |
of the suns greatest | 22 |
a a s s | 22 |
the right edge of | 22 |
and lay the thred | 22 |
represented either as utf | 22 |
the rule of three | 22 |
set one of the | 22 |
to the number of | 22 |
the bead to the | 22 |
the sine of deg | 22 |
a foot of timber | 22 |
end of the line | 22 |
find the suns azimuth | 22 |
side of the quadrant | 22 |
center of the glasse | 22 |
the edge of the | 22 |
is a line of | 22 |
the east and west | 22 |
from the right edge | 22 |
of the half sum | 22 |
characters represented either as | 22 |
the circle of the | 22 |
right edge of the | 22 |
axeltree of the dyal | 22 |
the parallels of the | 22 |
and of the ark | 21 |
set one foot in | 21 |
of the lower figure | 21 |
the lines of the | 21 |
thred to the other | 21 |
as in the table | 21 |
the latitude and declination | 21 |
you must place one | 21 |
particular scale of altitudes | 21 |
equal to the sine | 21 |
it a parallel in | 21 |
out the sine of | 21 |
upon the line of | 21 |
pole of the world | 21 |
and on the degrees | 21 |
the remainder is the | 21 |
sine of the course | 21 |
laid to the other | 21 |
the compasses from to | 21 |
of the suns azimuth | 21 |
from the elevated pole | 21 |
the angle at c | 21 |
and take the nearest | 21 |
the center to the | 21 |
must place one foot | 21 |
the lines on the | 21 |
the uses of the | 21 |
north part of the | 21 |
the extent from the | 21 |
is no other then | 21 |
the two including sides | 21 |
north pole is elevated | 21 |
distance of the stile | 21 |
to the point b | 21 |
and lay the thread | 21 |
line of sines on | 20 |
so when the sun | 20 |
so is the length | 20 |
from the point b | 20 |
place one foot of | 20 |
in a foot long | 20 |
that part of the | 20 |
is the same with | 20 |
right sine of the | 20 |
end of the horizontal | 20 |
distance of the substile | 20 |
of the figure above | 20 |
from the point of | 20 |
the sum and difference | 20 |
by help of a | 20 |
meridian of the plain | 20 |
axis of the world | 20 |
part of the horizon | 20 |
to the thread laid | 20 |
of the third side | 20 |
foot of the compasse | 20 |
find the hour of | 20 |
the line of contingence | 20 |
the tropick of cancer | 20 |
is the time of | 20 |
the hour from the | 20 |
from the beginning of | 20 |
sine of the said | 20 |
the other side of | 20 |
of the sum of | 20 |
to the length of | 20 |
the suns right ascension | 20 |
issuing from the center | 20 |
point of your compasses | 20 |
then draw the line | 20 |
from the line of | 20 |
is found to be | 20 |
distance from the elevated | 19 |
the same with the | 19 |
shall be the sine | 19 |
right angles with the | 19 |
the latitude to the | 19 |
from the point d | 19 |
by a line of | 19 |
distance from the sine | 19 |
the diameter of a | 19 |
cosine of the given | 19 |
of the suns distance | 19 |
is the secant of | 19 |
to find the angle | 19 |
equal to the complement | 19 |
the thread in the | 19 |
and laying the thread | 19 |
hour from the meridian | 19 |
and the line of | 19 |
be the tangent of | 19 |
a line of versed | 19 |
complement of the other | 19 |
time of the night | 19 |
if the hipotenusal be | 19 |
is the line of | 19 |
at the beginning of | 19 |
thread laid to the | 19 |
to make a foot | 19 |
to its opposite side | 19 |
end of the rule | 19 |
one of the sides | 19 |
shall be the true | 19 |
the houre of the | 19 |
cosine of the angle | 19 |
to be sold at | 19 |
the thread laid to | 19 |
of the feet of | 19 |
and the sine of | 19 |
sine of the ark | 19 |
as the secant of | 19 |
distance from the center | 19 |
it from the center | 19 |
the angle between the | 19 |
from the meridian line | 19 |
sun is in the | 19 |
the substile from the | 19 |
laying the thread over | 19 |
on the wall or | 18 |
come to the meridian | 18 |
of the three sides | 18 |
of half the difference | 18 |
the line of natural | 18 |
the angle at a | 18 |
from the particular scale | 18 |
the sector at that | 18 |
set one point of | 18 |
to find the azimuth | 18 |
keeping the sector at | 18 |
sines of the third | 18 |
from the center downwards | 18 |
so the cosine of | 18 |
rule laid from q | 18 |
line of the suns | 18 |
as the rectangle of | 18 |
the thread and the | 18 |
it shall reach to | 18 |
the feet of the | 18 |
to the common radius | 18 |
sum of the three | 18 |
if the sun be | 18 |
houre of the day | 18 |
the suns declination is | 18 |
length of the shadow | 18 |
and the remainder is | 18 |
in the use of | 18 |
the hour from six | 18 |
opposite to one of | 18 |
is less then the | 18 |
finding the hour and | 18 |
the hours of and | 18 |
the true hour of | 18 |
if the given angle | 18 |
the suns altitude in | 18 |
in the same manner | 18 |
the north part of | 18 |
the sine of an | 18 |
it were required to | 18 |
one point of your | 18 |
of the said thread | 17 |
true hour of the | 17 |
and you shall find | 17 |
in the versed sines | 17 |
to one of them | 17 |
of the scale of | 17 |
and the other to | 17 |
a line of tangents | 17 |
are to be sold | 17 |
just touch the thred | 17 |
would be found to | 17 |
and setting one foot | 17 |
measure from the center | 17 |
radius to the sine | 17 |
of the latitude is | 17 |
turned twice the same | 17 |
the points b and | 17 |
be greater then the | 17 |
will but just touch | 17 |
and there keep it | 17 |
to the side sought | 17 |
and it shall reach | 17 |
the right ascension of | 17 |
and the thread laid | 17 |
to work proportions in | 17 |
eleuation of the meridian | 17 |
to find the side | 17 |
the first of march | 17 |
all sorts of people | 17 |
to tangent of the | 17 |
twice the same way | 17 |
sine of the given | 17 |
that end of the | 17 |
half the angle sought | 17 |
it is to be | 17 |
drawn into the center | 17 |
of the suns right | 17 |
and in the line | 17 |
complement of the reclination | 17 |
the declination of a | 17 |
secant of the declination | 17 |
to find the distance | 17 |
after the french way | 17 |
a point in the | 17 |
so is sine of | 17 |
the other end of | 17 |
then from the point | 17 |
sector at that gage | 17 |
as you see in | 17 |
is greater than the | 17 |
to the end of | 16 |
over the secant of | 16 |
square of the sine | 16 |
other side of the | 16 |
tangent of the reclination | 16 |
the left edge of | 16 |
at the hour of | 16 |
of the meridian of | 16 |
end of the said | 16 |
one of the middle | 16 |
tangent of the complement | 16 |
sine of the sum | 16 |
azimuth from the meridian | 16 |
the center on the | 16 |
the suns going off | 16 |
height of the sun | 16 |
on the degrees it | 16 |
pole above the plaine | 16 |
as the cotangent of | 16 |
time of the year | 16 |
on the th of | 16 |
the tangent of an | 16 |
of the containing sides | 16 |
other end of the | 16 |
the length and breadth | 16 |
and are to be | 16 |
of sines on the | 16 |
from the meridian of | 16 |
is greater then the | 16 |
out of the line | 16 |
as thus for example | 16 |
where it intersects the | 16 |
product shall be the | 16 |
of the length of | 16 |
left edge of the | 16 |
of the fixed piece | 16 |
to the height of | 16 |
of the trianguler quadrant | 16 |
every one of the | 16 |
to the winter ecliptick | 16 |
take the sine of | 16 |
the given angle be | 16 |
to find the latitude | 16 |
the converse of the | 16 |
sun hath d of | 16 |
it a in the | 16 |
the line of versed | 16 |
the pole to the | 16 |
the other foot of | 16 |
the product shall be | 16 |
with the meridian line | 16 |
in a straight line | 16 |
open the other to | 16 |
the azimuth from south | 16 |
take out the parallel | 16 |
enter one foot of | 16 |
the rest of the | 16 |
one of the points | 16 |
of the th ark | 16 |
end of the meridian | 16 |
is the versed sine | 16 |
you see in the | 16 |
to all sorts of | 16 |
it shall shew the | 16 |
according to the terms | 15 |
by the institutions providing | 15 |
to cosine of the | 15 |
and the nearest distance | 15 |
the angle at the | 15 |
lay it from the | 15 |
of the center of | 15 |
laid from q to | 15 |
the thred on the | 15 |
all without asking permission | 15 |
to the latitude of | 15 |
line of the plain | 15 |
english books online text | 15 |
secant of the given | 15 |
the work described above | 15 |
it be required to | 15 |
keyboarded and encoded edition | 15 |
images scanned from microfilm | 15 |
enter the former extent | 15 |
the compasses on the | 15 |
the early english books | 15 |
providing financial support to | 15 |
as before is shewed | 15 |
come back to the | 15 |
and take out the | 15 |
and encoded edition of | 15 |
and markup reviewed and | 15 |
coded from proquest page | 15 |
sum and difference of | 15 |
for finding the hour | 15 |
the institutions providing financial | 15 |
is to the distance | 15 |
this phase i text | 15 |
assigned for keying and | 15 |
one foot of this | 15 |
encoded edition of the | 15 |
for keying and markup | 15 |
to the terms of | 15 |
as the difference of | 15 |
work described above is | 15 |
eleuation of the stile | 15 |
as the radius to | 15 |
your line of chords | 15 |
of the night by | 15 |
the placing of the | 15 |
on the fixed piece | 15 |
to the early english | 15 |
the content of the | 15 |
phase i text is | 15 |
is to the secant | 15 |
terms of creative commons | 15 |
the sum is the | 15 |
the difference in longitude | 15 |
the sine of any | 15 |
support to the early | 15 |
encoded text transcribed from | 15 |
then the nearest distance | 15 |
and coded from proquest | 15 |
markup reviewed and edited | 15 |
is parallel to the | 15 |
foot on the right | 15 |
the lines of sines | 15 |
books online text creation | 15 |
be less then the | 15 |
the compasses in the | 15 |
this keyboarded and encoded | 15 |
of the suns going | 15 |
from proquest page images | 15 |
is to the square | 15 |
tangent of the given | 15 |
is available for reuse | 15 |
and the given angle | 15 |
text can be copied | 15 |
in the middle of | 15 |
the complements of the | 15 |
just touch the thread | 15 |
to a fourth sine | 15 |
i text is available | 15 |
text and markup reviewed | 15 |
use of the trianguler | 15 |
to the figure below | 15 |
edition of the work | 15 |
the first to the | 15 |
in feet and inches | 15 |
of the elevation of | 15 |
from the pole to | 15 |
owned by the institutions | 15 |
how much is in | 15 |
and open the other | 15 |
from the substilar line | 15 |
sum of the sides | 15 |
measured from the center | 15 |
point of the pin | 15 |
foot of this extent | 15 |
the text can be | 15 |
the line of equal | 15 |
of the cosine of | 15 |
iv tiff page images | 15 |
of the suns place | 15 |
the points of shadow | 15 |
keyed and coded from | 15 |
described above is co | 15 |
or which is all | 15 |
the terms of creative | 15 |
day of the week | 15 |
financial support to the | 15 |
even for commercial purposes | 15 |
foot of that extent | 15 |
tcp assigned for keying | 15 |
one foot of that | 15 |
half the sum of | 15 |
is represented by the | 15 |
of the work described | 15 |
institutions providing financial support | 15 |
the sides of the | 15 |
secant of the altitude | 15 |
online text creation partnership | 15 |
the side of a | 15 |
is in a foot | 15 |
text is available for | 15 |
to be divided into | 15 |
from the foot of | 15 |
the sum or difference | 15 |
the dial a upon | 14 |
a s a a | 14 |
the sine of a | 14 |
it shall be the | 14 |
cuts the limb at | 14 |
the scale of hours | 14 |
some uses of the | 14 |
the parallels of declination | 14 |
of the horizontal line | 14 |
the use of this | 14 |
the tropick of capricorn | 14 |
you shall have the | 14 |
set the bead to | 14 |
the first day of | 14 |
thred to the nd | 14 |
minutes past in the | 14 |
a a s a | 14 |
height of the style | 14 |
is the distance of | 14 |
if it were required | 14 |
altitudes on all hours | 14 |
in the lesser sines | 14 |
you must lay the | 14 |
will be less then | 14 |
the tangent of a | 14 |
be taken out of | 14 |
points of shadow cdf | 14 |
when the declination is | 14 |
at the point of | 14 |
to the day of | 14 |
in the equal limbe | 14 |
description and use of | 14 |
a parallel in the | 14 |
of a great circle | 14 |
tangent of the hour | 14 |
of the declination in | 14 |
to cosecant of the | 14 |
the breadth in inches | 14 |
it will intersect the | 14 |
the latitude in the | 14 |
the south pole is | 14 |
to find the altitude | 14 |
to the distance run | 14 |
to find out the | 14 |
in the meridian line | 14 |
of the pin ab | 14 |
the sun being in | 14 |
the superficial content of | 14 |
the sun will be | 14 |
shall reach from the | 14 |
of the lines of | 14 |
when the altitude is | 14 |
third part of the | 14 |
to the straight line | 14 |
sum or difference of | 14 |
a clock in the | 14 |
the night by the | 14 |
of this extent at | 14 |
the north and south | 14 |
right ascension of the | 14 |
the other foot according | 14 |
and at the same | 14 |
other foot according to | 14 |
is to be found | 14 |
setting one point of | 14 |
is greater then a | 14 |
foot of the stile | 14 |
between the thread and | 14 |
to the meridian of | 14 |
place of the sun | 14 |
stile from the substilar | 14 |
sine of the th | 14 |
and the tangent of | 14 |
hour and azimuth in | 14 |
the answer to the | 14 |
place of the dyal | 14 |
secant of the angle | 14 |
length of the shaddow | 14 |
finde the suns azimuth | 14 |
the breadth of the | 14 |
half an hour past | 14 |
for finding the azimuth | 14 |
of the middle tearms | 14 |
of the latitude of | 14 |
and you have the | 14 |
south part of the | 14 |
may be found by | 14 |
much is in a | 14 |
shadow of the thred | 14 |
the declination from the | 14 |
which shall be the | 14 |
for the inclination of | 13 |
the sine of one | 13 |
measure it on the | 13 |
all the uses of | 13 |
finde the hour of | 13 |
the angle of position | 13 |
of the pin b | 13 |
of the side opposite | 13 |
and to the other | 13 |
the latitude is to | 13 |
being turned twice the | 13 |
required to find the | 13 |
the index and square | 13 |
the content of a | 13 |
to find the third | 13 |
former extent between the | 13 |
the suns altitude on | 13 |
suns altitude in the | 13 |
the description and use | 13 |
down the line of | 13 |
the ark of the | 13 |
declination of the plain | 13 |
between the eye and | 13 |
the half of the | 13 |
sine of one of | 13 |
foot of the compass | 13 |
to the breadth in | 13 |
azimuth from the vertical | 13 |
out of the greater | 13 |
equal to the angle | 13 |
without the help of | 13 |
contrary to the coast | 13 |
compasse to the point | 13 |
by the trianguler quadrant | 13 |
altitude or depression at | 13 |
between it and the | 13 |
or pole of the | 13 |
of the suns meridian | 13 |
of the meridian altitude | 13 |
that extent at the | 13 |
the finding of the | 13 |
sides with the angle | 13 |
two sides with the | 13 |
distance between the two | 13 |
distance from thence to | 13 |
of that arks complement | 13 |
it shall give the | 13 |
one third part of | 13 |
lay a ruler from | 13 |
from the half sum | 13 |
take out the tangent | 13 |
if you would have | 13 |
after the manner of | 13 |
upon the center a | 13 |
an east or west | 13 |
of the compasse to | 13 |
of the new latitude | 13 |
and it shall be | 13 |
time of sun rising | 13 |
the first leg to | 13 |
the horizontal line of | 13 |
pole to the plain | 13 |
dial a upon the | 13 |
and of the difference | 13 |
south pole is elevated | 13 |
axis of the horizon | 13 |
the quadrant to the | 13 |
and one of the | 13 |
distance of the meridian | 13 |
the place where the | 13 |
term is to the | 13 |
be found by the | 13 |
out the tangent of | 13 |
to the figure above | 13 |
they shall be the | 13 |
find how much is | 13 |
the line a b | 13 |
the making of a | 13 |
secant of the complement | 13 |
with the angle comprehended | 13 |
the angle at d | 13 |
the length in inches | 13 |
finde the suns altitude | 13 |
on the sine of | 13 |
applied the same way | 13 |
of the hipotenusal as | 13 |
the hour will be | 13 |
and the meridian of | 13 |
draw a line to | 13 |
out of the center | 13 |
arks on the plain | 13 |
and the foot of | 13 |
extent between the scale | 13 |
in one and the | 13 |
laid over the secant | 13 |
find the length of | 13 |
sine of an ark | 13 |
you shall find it | 13 |
the angle of and | 13 |
lay the dial a | 13 |
from the point i | 13 |
be added to the | 13 |
natural sine of the | 13 |
the difference in latitude | 13 |
so tangent of the | 13 |
that th to the | 13 |
the two first tearms | 13 |
parallel sine of the | 13 |
from the next equinoctial | 13 |
line of a clock | 13 |
scale of equal parts | 13 |
the sine of degrees | 13 |
the time of sun | 13 |
the former extent between | 13 |
the south part of | 12 |
found to be deg | 12 |
equal to the latitude | 12 |
of the tangent of | 12 |
be to find the | 12 |
of the sun from | 12 |
of the substiles distance | 12 |
then take the nearest | 12 |
and the distance of | 12 |
draw a straight line | 12 |
till you see the | 12 |
let it be required | 12 |
the sector stands at | 12 |
compasses in the point | 12 |
to the sum of | 12 |
cosecant of the side | 12 |
to prick off the | 12 |
and keeping the sector | 12 |
side of the loose | 12 |
and measure it on | 12 |
in the figure below | 12 |
by the lines of | 12 |
of the half circle | 12 |
superficies of the dyall | 12 |
the suns height at | 12 |
so sine of the | 12 |
from toward the end | 12 |
at the cosine of | 12 |
in like manner may | 12 |
the second term is | 12 |
a pair of compasses | 12 |
the cuspis of the | 12 |
on the opposite side | 12 |
from the scale of | 12 |
the figure of the | 12 |
the sine of that | 12 |
shall be the tangent | 12 |
if the sun have | 12 |
sine of an arch | 12 |
it on the line | 12 |
so cosine of the | 12 |
the point b of | 12 |
first to the second | 12 |
on the other leg | 12 |
for example in the | 12 |
declination of a plain | 12 |
equal to the radius | 12 |
first leg to the | 12 |
laid from p to | 12 |
and you will find | 12 |
will be to find | 12 |
the tangents of the | 12 |
the meridian between the | 12 |
rule laid from p | 12 |
cosine of the suns | 12 |
is the length in | 12 |
and take the distance | 12 |
as in the former | 12 |
thread in the limb | 12 |
fourth part of the | 12 |
right angled sphoerical triangles | 12 |
foot on the left | 12 |
in a right line | 12 |
artificial sines and tangents | 12 |
go to the figure | 12 |
side of the meridian | 12 |
to the distance of | 12 |
and difference of the | 12 |
end of the head | 12 |
the help of the | 12 |
suns altitude on all | 12 |
and where it intersects | 12 |
the declination to the | 12 |
the reclination of the | 12 |
cosecant of the given | 12 |
take with your compasses | 12 |
or in the afternoon | 12 |
side greater then a | 12 |
to draw the dial | 12 |
the differences of the | 12 |
of the sun being | 12 |
is the measure of | 12 |
by reason of the | 12 |
to be in the | 12 |
an hour past in | 12 |
of the sun in | 12 |
foot according to nearest | 12 |
the compasse to the | 12 |
as much as the | 12 |
be the cosine of | 12 |
shall shew the true | 12 |
the logarithms of the | 12 |
times the same way | 12 |
a quarter of a | 12 |
the azimuth in the | 12 |
from the point a | 12 |
cosine of the side | 12 |
the number of feet | 12 |
superficial content of the | 12 |
hour past in the | 12 |
where the end of | 12 |
the affection of the | 12 |
the degrees of the | 12 |
make a foot of | 12 |
the ark or angle | 12 |
to the length in | 12 |
of the suns present | 12 |
to the given side | 12 |
being one of the | 12 |
to finde the azimuth | 12 |
the solid content of | 12 |
is the sum of | 12 |
difference between the two | 12 |
point of one of | 12 |
of the poles elevation | 12 |
the secant of d | 12 |
and azimuth in the | 12 |
one degree of longitude | 12 |
a second or later | 11 |
the texts were encoded | 11 |
reason to do so | 11 |
equal to the distance | 11 |
and characters marked as | 11 |
remain and some readable | 11 |
assurance was then carried | 11 |
a limit of instances | 11 |
bibliography of english literature | 11 |
by university of nebraska | 11 |
all likelihood such instances | 11 |
with this space come | 11 |
so much is the | 11 |
the opposite side greater | 11 |
divided into two phases | 11 |
standards were returned to | 11 |
the divisions of the | 11 |
that in all likelihood | 11 |
take and use these | 11 |
a line of equal | 11 |
are given to find | 11 |
or for an anonymous | 11 |
was then carried out | 11 |
will be marked as | 11 |
were corrected where possible | 11 |
such proportion to the | 11 |
to produce large quantities | 11 |
known extent have been | 11 |
the suns azimuth at | 11 |
or tei g elements | 11 |
issued variously as sgml | 11 |
texts based on the | 11 |
as illegible were corrected | 11 |
possible up to a | 11 |
of the tei in | 11 |
of any assumptions that | 11 |
been issued variously as | 11 |
were encoded and linked | 11 |
a work was chosen | 11 |
sets published by proquest | 11 |
elements of known extent | 11 |
the filling in of | 11 |
these texts for their | 11 |
been released into the | 11 |
intended to range over | 11 |
to the cosecant of | 11 |
the eye and the | 11 |
their works are eligible | 11 |
being set to the | 11 |
between and available in | 11 |
keyers to be redone | 11 |
editions of a works | 11 |
the two middle tearms | 11 |
placeholder characters or elements | 11 |
on the new cambridge | 11 |
texts have been issued | 11 |
the print record of | 11 |
encoded texts based on | 11 |
structural encoding based on | 11 |
that can be made | 11 |
due credit and attribution | 11 |
to tei p using | 11 |
and sometimes a second | 11 |
aware of the process | 11 |
selection was intended to | 11 |
till it stay in | 11 |
is to encode one | 11 |
and set one foot | 11 |
a number of works | 11 |
was divided into two | 11 |
to find the length | 11 |
to one of the | 11 |
of right angled sphoerical | 11 |
work was chosen if | 11 |
was based on the | 11 |
large quantities of textual | 11 |
was proofread for accuracy | 11 |
we respectfully request that | 11 |
laid the same way | 11 |
in the upper quadrant | 11 |
be marked as illegible | 11 |
there was a compelling | 11 |
between the two including | 11 |
the radius of your | 11 |
the usual project restraints | 11 |
opposed to critical editions | 11 |
accordance with level of | 11 |
the stile is to | 11 |
unicode or tei g | 11 |
creation partnership web site | 11 |
keying companies for transcription | 11 |
proofread for accuracy and | 11 |
looked at by a | 11 |
copies of the texts | 11 |
illegible were corrected where | 11 |
text selection was based | 11 |
available at the text | 11 |
to external keying companies | 11 |
text strings within braces | 11 |
not meet qa standards | 11 |
the point of one | 11 |
given to their original | 11 |
were sent to external | 11 |
no other then a | 11 |
tangent of the said | 11 |
is to the length | 11 |
find how much in | 11 |
draw a line from | 11 |
and or corrected and | 11 |
domain as of january | 11 |
chosen if there was | 11 |
based on the image | 11 |
a in the co | 11 |
a south plain declining | 11 |
tei p using tcp | 11 |
simplify the filling in | 11 |
true nature of the | 11 |
or elements to simplify | 11 |
complement of the elevation | 11 |
proquest via their early | 11 |
each text was proofread | 11 |
and the angle at | 11 |
image sets published by | 11 |
then the extent from | 11 |
must lay the dial | 11 |
corrected and characters marked | 11 |
be aware of the | 11 |
characters will be marked | 11 |
whichever is the greater | 11 |
and linked to page | 11 |
transcribed and encoded texts | 11 |
texts created during phase | 11 |
the sun from the | 11 |
characters marked as illegible | 11 |
as opposed to critical | 11 |
external keying companies for | 11 |
texts were encoded and | 11 |
instances will never have | 11 |
which did not meet | 11 |
placing of the axeltree | 11 |
illegibles were encoded as | 11 |
to create diplomatic transcriptions | 11 |
characters or elements to | 11 |
teams in oxford and | 11 |
in all likelihood such | 11 |
the center of a | 11 |
and at the end | 11 |
page images in accordance | 11 |
gaps by user contributors | 11 |
transformed into placeholder characters | 11 |
errors will remain and | 11 |
included and sometimes a | 11 |
to reflect the true | 11 |
users should bear in | 11 |
tcp is a partnership | 11 |
transcription and basic encoding | 11 |
rumb from the meridian | 11 |
text with mnemonic sdata | 11 |
text was proofread for | 11 |
usually the first edition | 11 |
of michigan and oxford | 11 |
into the public domain | 11 |
angles with the horizon | 11 |
will reach to the | 11 |
have been transformed into | 11 |
never have been looked | 11 |
the sector so set | 11 |
then their works are | 11 |
till the other foot | 11 |
for transcription and basic | 11 |
find the third side | 11 |
created during phase of | 11 |
any remaining illegibles were | 11 |
works in other languages | 11 |
on the day of | 11 |
is the length of | 11 |
sometimes a second or | 11 |
the parallel of declination | 11 |
first day of march | 11 |
will remain and some | 11 |
can be made about | 11 |
are a number of | 11 |
the suns altitudes on | 11 |
of the project have | 11 |
texts for their own | 11 |
creating the tcp texts | 11 |
a works in english | 11 |
any ark or angle | 11 |
linked to page images | 11 |
difference of the base | 11 |
of a work was | 11 |
to find how many | 11 |
latitude is to the | 11 |
the suns declination in | 11 |
are eligible for inclusion | 11 |
for an anonymous work | 11 |
released into the public | 11 |
point b of the | 11 |
request that due credit | 11 |
made about the data | 11 |
for their own purposes | 11 |
opposite to the coast | 11 |
tangent of any ark | 11 |
based on the text | 11 |
was intended to range | 11 |
and some readable characters | 11 |
data within the usual | 11 |
of the suns rising | 11 |
in accordance with level | 11 |
the angle sought as | 11 |
and the product shall | 11 |
the first tearm in | 11 |
restraints of time and | 11 |
by converting tcp files | 11 |
the length of a | 11 |
new cambridge bibliography of | 11 |
changes to facilitate morpho | 11 |
suns altitudes on all | 11 |
of the print record | 11 |
credit and attribution is | 11 |
keying and markup guidelines | 11 |
notes for div a | 11 |
have the line of | 11 |
but we respectfully request | 11 |
ascii text with mnemonic | 11 |
can now take and | 11 |
the tei in libraries | 11 |
guidelines are available at | 11 |
works are eligible for | 11 |
project have been released | 11 |
have been issued variously | 11 |
the image sets published | 11 |
some readable characters will | 11 |
the hour line of | 11 |
th part of the | 11 |
understanding these processes should | 11 |
created by converting tcp | 11 |
lesse then the complement | 11 |
represented by the line | 11 |
tcp files to tei | 11 |
general aim of eebo | 11 |
aimed to produce large | 11 |
the text encoding initiative | 11 |
then carried out by | 11 |
with mnemonic sdata character | 11 |
of the suns coming | 11 |
or later edition of | 11 |
range over a wide | 11 |
the project have been | 11 |
out by editorial teams | 11 |
project was divided into | 11 |
therefore chose to create | 11 |
the meridian from the | 11 |
based on the new | 11 |
root of a number | 11 |
second or later edition | 11 |
marked as illegible were | 11 |
text creation partnership web | 11 |
of textual data within | 11 |
quality assurance was then | 11 |
of the loose piece | 11 |
their early english books | 11 |
title published between and | 11 |
for the most part | 11 |
will never have been | 11 |
any assumptions that can | 11 |
encoding based on the | 11 |
of each text was | 11 |
the hipotenusal be greater | 11 |
in respect of the | 11 |
every hour and quarter | 11 |
from the left edge | 11 |
to range over a | 11 |
by editorial teams in | 11 |
opposite side greater then | 11 |
to find the square | 11 |
cambridge bibliography of english | 11 |
were encoded as gap | 11 |
notably latin and welsh | 11 |
overall quality of tcp | 11 |
as in the first | 11 |
the product of the | 11 |
to find a side | 11 |
although there are a | 11 |
level of the tei | 11 |
carried out by editorial | 11 |
the circle on the | 11 |
to a limit of | 11 |
remaining illegibles were encoded | 11 |
images in accordance with | 11 |
while the overall quality | 11 |
length of the line | 11 |
into placeholder characters or | 11 |
partnership between the universities | 11 |
later edition of a | 11 |
and available in eebo | 11 |
processed by university of | 11 |
converting tcp files to | 11 |
data is very good | 11 |
to the keyers to | 11 |
on the versed sines | 11 |
out the secant of | 11 |
were returned to the | 11 |
to page images in | 11 |
in the middle rule | 11 |
chose to create diplomatic | 11 |
so is the parallel | 11 |
proquest to create accurately | 11 |
limit of instances per | 11 |
the square to the | 11 |
unicode or text strings | 11 |
of tcp data is | 11 |
publisher proquest to create | 11 |
accuracy and those which | 11 |
during phase of the | 11 |
compelling reason to do | 11 |
a line of natural | 11 |
elements to simplify the | 11 |
and markup guidelines are | 11 |
was enhanced and or | 11 |
plain of the horizon | 11 |
then take the distance | 11 |
from on the moveable | 11 |
the arch of the | 11 |
at the text creation | 11 |
users should be aware | 11 |
some errors will remain | 11 |
of time and funding | 11 |
by proquest via their | 11 |
there are a number | 11 |
encoding was enhanced and | 11 |
number of works in | 11 |
phase of the project | 11 |
of creating the tcp | 11 |
space come back to | 11 |
distance on the meridian | 11 |
files to tei p | 11 |
first tearm in the | 11 |
of the process of | 11 |
accurately transcribed and encoded | 11 |
therefore of any assumptions | 11 |
and use these texts | 11 |
quality of tcp data | 11 |
the nd from the | 11 |
image sets were sent | 11 |
now take and use | 11 |
the line of degrees | 11 |
usual project restraints of | 11 |
companies for transcription and | 11 |
was a compelling reason | 11 |
encoded as gap s | 11 |
where possible up to | 11 |
published between and available | 11 |
the general aim of | 11 |
public domain as of | 11 |
gap elements of known | 11 |
and therefore of any | 11 |
at by a tcp | 11 |
and encoded texts based | 11 |
the quadrant of latitudes | 11 |
in of gaps by | 11 |
and oxford and the | 11 |
p using tcp tei | 11 |
on the image sets | 11 |
point i of the | 11 |
the keyers to be | 11 |
and attribution is given | 11 |
been transformed into placeholder | 11 |
tei in libraries guidelines | 11 |
published by proquest via | 11 |
of gaps by user | 11 |
universities of michigan and | 11 |
on the right hand | 11 |
should bear in mind | 11 |
selection was based on | 11 |
when the latitude and | 11 |
the universities of michigan | 11 |
of every monographic english | 11 |
the halfs and quarters | 11 |
a compelling reason to | 11 |
have been looked at | 11 |
meridian or pole of | 11 |
michigan and oxford and | 11 |
ascension of the sun | 11 |
by a tcp editor | 11 |
edition of a work | 11 |
solid content of the | 11 |
language title published between | 11 |
mind that in all | 11 |
is in the equinoctial | 11 |
to simplify the filling | 11 |
how much in length | 11 |
cosine of the ark | 11 |
of the versed sine | 11 |
the end of that | 11 |
to the angle sought | 11 |
textual data within the | 11 |
of the texts have | 11 |
and the same point | 11 |
mainly structural encoding based | 11 |
nature of the print | 11 |
likelihood such instances will | 11 |
print record of the | 11 |
given to find an | 11 |
markup guidelines are available | 11 |
meet qa standards were | 11 |
in english were prioritized | 11 |
on the text encoding | 11 |
to their original source | 11 |
the encoding was enhanced | 11 |
sun being in the | 11 |
and it shall shew | 11 |
tcp is to encode | 11 |
record of the period | 11 |
anyone can now take | 11 |
or corrected and characters | 11 |
the tangent of any | 11 |
process of creating the | 11 |
being turned two times | 11 |
reflect the true nature | 11 |
to encode one copy | 11 |
via their early english | 11 |
sent to external keying | 11 |
attribution is given to | 11 |
the meridian or pole | 11 |
the proportion will be | 11 |
is given to their | 11 |
the overall quality of | 11 |
till the shadow of | 11 |
first editions of a | 11 |
against it in the | 11 |
to the other side | 11 |
the true nature of | 11 |
due east or west | 11 |
assumptions that can be | 11 |
respectfully request that due | 11 |
these processes should make | 11 |
editorial teams in oxford | 11 |
the publisher proquest to | 11 |
have been released into | 11 |
the text creation partnership | 11 |
if there was a | 11 |
for the suns azimuth | 11 |
or text strings within | 11 |
tcp project was divided | 11 |
stile from the meridian | 11 |
with the other draw | 11 |
oxford and the publisher | 11 |
be made about the | 11 |
tangent of the side | 11 |
variety of subject areas | 11 |
extent have been transformed | 11 |
bear in mind that | 11 |
the texts have been | 11 |
of the th chapter | 11 |
wide variety of subject | 11 |
such instances will never | 11 |
of known extent have | 11 |
sines of the containing | 11 |
tcp aimed to produce | 11 |
of works in other | 11 |
quantities of textual data | 11 |
filling in of gaps | 11 |
and the publisher proquest | 11 |
between the zenith and | 11 |
project restraints of time | 11 |
this extent at the | 11 |
enhanced and or corrected | 11 |
that due credit and | 11 |
of a works in | 11 |
create accurately transcribed and | 11 |
over a wide variety | 11 |
sets were sent to | 11 |
returned to the keyers | 11 |
use these texts for | 11 |
to create accurately transcribed | 11 |
is a partnership between | 11 |
was chosen if there | 11 |
of the latitude in | 11 |
and those which did | 11 |
sine of the distance | 11 |
length of the gnomon | 11 |
within the usual project | 11 |
the third to the | 11 |
processes should make clear | 11 |
from the center a | 11 |
of the declination to | 11 |
of any ark or | 11 |
shall be the content | 11 |
the hour from midnight | 11 |
with level of the | 11 |
a partnership between the | 11 |
did not meet qa | 11 |
of instances per text | 11 |
been looked at by | 11 |
should make clear that | 11 |
qa standards were returned | 11 |
in oxford and michigan | 11 |
with changes to facilitate | 11 |
a wide variety of | 11 |
tcp data is very | 11 |
be d from the | 11 |
and set it from | 11 |
encoded and linked to | 11 |
produce large quantities of | 11 |
mnemonic sdata character entities | 11 |
between the universities of | 11 |
readable characters will be | 11 |
and therefore chose to | 11 |
in mind that in | 11 |
for accuracy and those | 11 |
are available at the | 11 |
those which did not | 11 |
the ends of the | 11 |
that side of the | 11 |
up to a limit | 11 |
the sun hath deg | 11 |
the new cambridge bibliography | 11 |
works in english were | 11 |
should be aware of | 11 |
corrected where possible up | 11 |
the public domain as | 11 |
the process of creating | 11 |
center of the sun | 10 |
the outward ledge of | 10 |
one of the including | 10 |
find the hour and | 10 |
to the meridian between | 10 |
lay the thred on | 10 |
length of a foot | 10 |
perpendiculer height of the | 10 |
shall be the hour | 10 |
distance from the zenith | 10 |
and in the morning | 10 |
fiducial edge of the | 10 |
the vses of the | 10 |
and extend the other | 10 |
parts of a foot | 10 |
from the tangent of | 10 |
and you shall have | 10 |
to a new latitude | 10 |
extent from the center | 10 |
then set one foot | 10 |
in all other cases | 10 |
the sum or remainder | 10 |
in such sort that | 10 |
meridian of the world | 10 |
and you shall finde | 10 |
it ought to be | 10 |
the other side the | 10 |
is to the difference | 10 |
extent applied the same | 10 |
arch of a great | 10 |
sine of the amplitude | 10 |
degree of longitude in | 10 |
on the degrees from | 10 |
declination in the scale | 10 |
at right angles to | 10 |
to the time of | 10 |
to the suns altitude | 10 |
length in feet and | 10 |
three sides are given | 10 |
may be found in | 10 |
drawn from the center | 10 |
the true altitude required | 10 |
and tangents on the | 10 |
the other turned about | 10 |
may but just touch | 10 |
the zenith and the | 10 |
and the thread in | 10 |
to the difference in | 10 |
of the points of | 10 |
the leggs from the | 10 |
meridian between the zenith | 10 |
so is the secant | 10 |
as far as the | 10 |
versed sines in the | 10 |
is the inclination of | 10 |
diameter of a circle | 10 |
then the latitude of | 10 |
the general scale of | 10 |
vertical altitude or depression | 10 |
find the distance of | 10 |
of the quadrant to | 10 |
half difference of the | 10 |
opposite side less then | 10 |
of the altitude sought | 10 |
if you take the | 10 |
the suns true place | 10 |
of the day to | 10 |
is contrary to the | 10 |
found out on the | 10 |
quadrant of a circle | 10 |
point in the air | 10 |
the sine to the | 10 |
outward ledge of the | 10 |
distance from the point | 10 |
the contrary way from | 10 |
perpendicular to the straight | 10 |
horizontal line of the | 10 |
from the midnight meridian | 10 |
the number of men | 10 |
meridians distance from the | 10 |
in the first place | 10 |
the two first terms | 10 |
three points of shadow | 10 |
sines of the sum | 10 |
distance from a to | 10 |
the price of one | 10 |
of the east or | 10 |
back again to the | 10 |
to finde the declination | 10 |
greater than the first | 10 |
the sun being given | 10 |
to project the triangle | 10 |
what day of the | 10 |
side of a square | 10 |
sine of any ark | 10 |
side less then a | 10 |
to a line of | 10 |
in the air i | 10 |
shall be equal to | 10 |
diameter of the circle | 10 |
as the sector stands | 10 |
the time when the | 10 |
the latteral sine of | 10 |
sines of the half | 10 |
is the number of | 10 |
suns rising and setting | 10 |
page the use of | 10 |
end of the scale | 10 |
to perform the same | 10 |
of the compasse upon | 10 |
lay a ruler to | 10 |
in the said reflected | 10 |
of the two including | 10 |
the second and third | 10 |
be due east or | 10 |
the line of shadows | 10 |
of the dial a | 10 |
sine of the plains | 10 |
the parralels of altitude | 10 |
along the line of | 10 |
the scale of equal | 10 |
of the two middle | 10 |
have drawn about the | 10 |
case of right angled | 10 |
the azimuth will be | 10 |
setting one foot in | 10 |
of the substilar line | 10 |
the time of rising | 10 |
the plains horizontal line | 10 |
this space come back | 10 |
the head of the | 10 |
from the point f | 10 |
from the noon meridian | 10 |
from the complement of | 10 |
the meridian line in | 10 |
and it shews the | 10 |
of the said arch | 10 |
of the differences of | 10 |
at the same instant | 10 |
the thread and plummet | 10 |
to draw the reflected | 10 |
and let it be | 10 |
of versed sines to | 10 |
of that extent at | 10 |
of the other sides | 10 |
reach to the sine | 10 |
made equal to the | 10 |
take the declination from | 10 |
the cosine of half | 10 |
the first term is | 10 |
of the reclination inclination | 10 |
of east and west | 10 |
distance from the next | 10 |
the other point to | 10 |
to the beginning of | 10 |
on the moveable piece | 10 |
the suns coming on | 10 |
the hour in the | 10 |
where it cuts cancer | 10 |
and declination of the | 10 |
the declination on the | 10 |
of your line of | 10 |
parts of an inch | 10 |
to find the declination | 10 |
the other middle tearm | 10 |
you have drawn about | 10 |
counted from the right | 10 |
drawn about the point | 10 |
angle sought as the | 10 |
of the first term | 10 |
of the small quadrant | 10 |
draw with the other | 10 |
back to the figure | 10 |
then laying the thread | 10 |
it will not be | 10 |
the other draw the | 10 |
given to finde the | 10 |
example in the point | 10 |
is the cotangent of | 10 |
the opposite side less | 10 |
the base of the | 10 |
height of the tower | 10 |
six in the morning | 10 |
two times the same | 10 |
must be taken out | 10 |
thread and the scale | 10 |
and enter the former | 10 |
go back again to | 10 |
the hipotenusal be less | 10 |
it stay in like | 10 |
that you have drawn | 10 |
is to be added | 9 |
the sun to be | 9 |
between the hours of | 9 |
if you lay the | 9 |
distance between the versed | 9 |
altitudes of the sun | 9 |
of the day will | 9 |
into three equal parts | 9 |
the angles at the | 9 |
take out the tangents | 9 |
in the straight line | 9 |
the nature of the | 9 |
to finde the inclination | 9 |
on the under face | 9 |
ark in the limb | 9 |
let the altitude be | 9 |
a polar plains reclination | 9 |
on the middle of | 9 |
the plaine of the | 9 |
the thread on the | 9 |
between the two meridians | 9 |
s s s p | 9 |
the touch of an | 9 |
of half the sum | 9 |
by the former directions | 9 |
draw the line c | 9 |
with the help of | 9 |
of a circle given | 9 |
and in the versed | 9 |
in the place of | 9 |
will be the same | 9 |
the line of a | 9 |
the same way as | 9 |
to foot on the | 9 |
for the stiles height | 9 |
on the general scale | 9 |
shewes the time of | 9 |
our latitude of london | 9 |
of the houre lines | 9 |
an angle opposite to | 9 |
as the first term | 9 |
the fiducial edge of | 9 |
other foot lay the | 9 |
in the morning or | 9 |
equal to the square | 9 |
so is the distance | 9 |
will be equal to | 9 |
sine complement of the | 9 |
to be equal to | 9 |
complement of the new | 9 |
end is fastened in | 9 |
the line of right | 9 |
the parallels of altitude | 9 |
the parallel of the | 9 |
sine of d is | 9 |
the dayes and nights | 9 |
tangent of the inclination | 9 |
by introducing the radius | 9 |
nearest to the point | 9 |
to the summer ecliptick | 9 |
the second to the | 9 |
comes to the meridian | 9 |
you will find the | 9 |
so is the breadth | 9 |
is the same that | 9 |
the th part of | 9 |
sine of the complement | 9 |
of the altitude in | 9 |
finde the declination of | 9 |
the true content of | 9 |
height of the pole | 9 |
it must meet with | 9 |
the horizon of the | 9 |
if the sum of | 9 |
so is the cotangent | 9 |
and the difference of | 9 |
of the sum or | 9 |
point of shadow f | 9 |
the upper face of | 9 |
of d to the | 9 |
you shall finde the | 9 |
the price of a | 9 |
but if the sun | 9 |
no other then the | 9 |
in the particular scheam | 9 |
is fastened in the | 9 |
in the annexed tangent | 9 |
the suns rising and | 9 |
and it shall give | 9 |
the distance from to | 9 |
whose end is fastened | 9 |
divided into equal parts | 9 |
the thred and plummet | 9 |
of the sun is | 9 |
fastened in the center | 9 |
the sine of his | 9 |
it will be necessary | 9 |
tearm of the proportion | 9 |
the latteral tangent of | 9 |
the stars right ascention | 9 |
extend the threed from | 9 |
the point of intersection | 9 |
be sold at his | 9 |
and the time of | 9 |
the same manner as | 9 |
it may be observed | 9 |
sine to the sine | 9 |
line bd of the | 9 |
compasses in the center | 9 |
distance from b to | 9 |
segment of a circle | 9 |
the hour from towards | 9 |
the other angle be | 9 |
to the suns declination | 9 |
the perpendiculer height of | 9 |
by the answer to | 9 |
then lay the thred | 9 |
one from the other | 9 |
the figure of your | 9 |
dial in the minories | 9 |
the position of the | 9 |
azimuth from the east | 9 |
end of a thread | 9 |
above the upper horizon | 9 |
if the declination be | 9 |
will be greater then | 9 |
to the elevation of | 9 |
in the meridian of | 9 |
in sines and tangents | 9 |
found will be less | 9 |
if one of the | 9 |
with the other make | 9 |
on the scale of | 9 |
the sun shall have | 9 |
by this means you | 9 |
the distance from thence | 9 |
foot and a half | 9 |
the other foot draw | 9 |
some part of the | 9 |
apply the side of | 9 |
radius of the sines | 9 |
thread to the sine | 9 |
foot lay the thread | 9 |
for it must meet | 9 |
from the center o | 9 |
of the sides of | 9 |
then from the center | 9 |
a line from the | 9 |
the north or south | 9 |
general scale of altitudes | 9 |
cosecant of the angle | 9 |
the same time the | 9 |
bears such proportion to | 9 |
the line of azimuths | 9 |
in this case the | 9 |
and in the equal | 9 |
direct east or west | 9 |
whole content of the | 9 |
the third term is | 9 |
of the stiles elevation | 9 |
on the degrees on | 9 |
stiles height above the | 9 |
d in the limb | 9 |
s s p m | 9 |
draw with the rule | 9 |
stile is to be | 9 |
at the declination in | 9 |
and the suns distance | 9 |
and first for the | 9 |
the turning sight to | 9 |
so is the sum | 9 |
lines of the hours | 9 |
by laying the thread | 9 |
so is the square | 9 |
sides are given to | 9 |
example for finding the | 9 |
the declination of any | 9 |
setting one foot of | 9 |
the whole content of | 9 |
method of calculation for | 9 |
the complement of it | 9 |
out the tangents of | 9 |
the line of decimal | 9 |
of one of those | 9 |
the day will be | 9 |
thred to the declination | 9 |
is the same as | 9 |
take out the secant | 9 |
the lines of lines | 9 |
angle at the pole | 9 |
d of north declination | 9 |
and prick them from | 9 |
the line of segments | 9 |
the other part of | 9 |
a line parallel to | 9 |
from the center on | 9 |
hipotenusal be less then | 9 |
or difference of sines | 9 |
sine of the arch | 9 |
the sun in the | 9 |
when the two places | 9 |
when three sides are | 9 |
the meridians distance from | 9 |
about the th of | 9 |
of the complements of | 9 |
for the distance of | 9 |
opposite to the angle | 9 |
the substilar line is | 9 |
is more then the | 9 |
till the other point | 9 |
distance between the hours | 9 |
and the elevated pole | 9 |
of d in the | 9 |
amplitude of the sun | 9 |
the other lay the | 9 |
tangent of an ark | 9 |
the two points of | 9 |
of the day and | 9 |
s p m p | 9 |
converse of the former | 9 |
line perpendicular to the | 9 |
so is to foot | 9 |
for the placing of | 9 |
line parallel to the | 9 |
over the day of | 9 |
may be taken off | 9 |
take the nd from | 9 |
if the other angle | 9 |
time when the sun | 9 |
which is in the | 9 |
the third and fourth | 9 |
substile from the meridian | 9 |
difference of the sides | 9 |
found to be degrees | 9 |
to divide a line | 9 |
were required to find | 9 |
must meet with it | 9 |
so much as the | 9 |
and of the sum | 9 |
the point where the | 9 |
in the substilar line | 9 |
from on the loose | 9 |
but by the line | 9 |
sine of the other | 9 |
take the suns altitude | 9 |
you see that the | 9 |
the end of a | 9 |
and that th to | 9 |
to draw a direct | 9 |
to the lower figure | 9 |
it may be found | 9 |
is the sine to | 9 |
feet of the compasse | 9 |
be the substilar line | 9 |
and the length of | 9 |
being the complement of | 9 |
center of the said | 9 |
shall be the substilar | 9 |
then the sine of | 9 |
leg to the sine | 9 |
angle opposite to one | 9 |
the line of chords | 9 |
compasses on the line | 9 |
make a right angle | 9 |
the other foot lay | 9 |
the cube of the | 9 |
sines and tangents on | 8 |
the head toward the | 8 |
when the given angle | 8 |
turned about may but | 8 |
lines are to be | 8 |
from toward the center | 8 |
the sun or any | 8 |
north end of the | 8 |
to the point o | 8 |
so cosecant of the | 8 |
so is the versed | 8 |
then right against the | 8 |
what altitude the sun | 8 |
of a piece of | 8 |
towards the depressed pole | 8 |
shall stay at the | 8 |
as in this example | 8 |
to the other given | 8 |
you may plainly see | 8 |
to the middle of | 8 |
upon the complement of | 8 |
season of the year | 8 |
cotangent of half the | 8 |
the whole length of | 8 |
difference of any two | 8 |
plain and easie directions | 8 |
a sine in the | 8 |
in the right angled | 8 |
shewing the making of | 8 |
in the particular sine | 8 |
line from the point | 8 |
to the season of | 8 |
out of the scale | 8 |
lines on the quadrant | 8 |
from the point o | 8 |
the number of dayes | 8 |
work proportions in sines | 8 |
which if you add | 8 |
any one of the | 8 |
sine is to the | 8 |
of the quadrant of | 8 |
the tangent of degrees | 8 |
whole length of the | 8 |
be set to the | 8 |
the meridian line be | 8 |
content of the base | 8 |
as i have said | 8 |
to the scale of | 8 |
the line of altitudes | 8 |
with the radius of | 8 |
the inside of the | 8 |
plaine of the meridian | 8 |
of the said glasse | 8 |
a ruler laid to | 8 |
you have the time | 8 |
found to be the | 8 |
thred to the day | 8 |
of these two arks | 8 |
tangent of a fourth | 8 |
if you count from | 8 |
greater then the complement | 8 |
from the first to | 8 |
it is in the | 8 |
of the stile is | 8 |
you shall finde it | 8 |
on the right side | 8 |
with the plaine of | 8 |
of the leggs from | 8 |
to the second term | 8 |
at foot in length | 8 |
is the declination from | 8 |
before in the morning | 8 |
and there will be | 8 |
of the fitted scale | 8 |
the line of houres | 8 |
is to be graduated | 8 |
half the tangent of | 8 |
a piece of timber | 8 |
to the line ab | 8 |
the point i of | 8 |
from the center is | 8 |
the answer in the | 8 |
as in the second | 8 |
find the content of | 8 |
and note the place | 8 |
passing through the center | 8 |
the space from the | 8 |
points of the horizon | 8 |
to the use of | 8 |
with this space go | 8 |
as the cosecant of | 8 |
it in the line | 8 |
to which if you | 8 |
east and west incliners | 8 |
this space go to | 8 |
quantity of the angle | 8 |
is to be drawn | 8 |
of the dyal is | 8 |
be less than the | 8 |
in the tangent of | 8 |
the number of inches | 8 |
depression under the horizon | 8 |
the given angle is | 8 |
it will cut the | 8 |
of the angle adjacent | 8 |
to finde the angle | 8 |
tangent of the lesser | 8 |
cosine of half the | 8 |
or other of the | 8 |
sine of the substile | 8 |
the distance between and | 8 |
of the other to | 8 |
point of shadow c | 8 |
greater or less then | 8 |
the season of the | 8 |
so that if you | 8 |
equal to the sum | 8 |
the stiles height above | 8 |
we may find the | 8 |
product of the two | 8 |
differences of the leggs | 8 |
is distant from the | 8 |
it shews the azimuth | 8 |
draw the hour lines | 8 |
and they shall be | 8 |
the legs of the | 8 |
of the horizontal dial | 8 |
the suns altitude or | 8 |
the body of the | 8 |
sine of the rumb | 8 |
will be found in | 8 |
the diameter in inches | 8 |
the summer half year | 8 |
from the first term | 8 |
declining from the south | 8 |
reproduction of original in | 8 |
of the suns ascension | 8 |
and turn the other | 8 |
above that end of | 8 |
the beams of the | 8 |
may be called the | 8 |
on the left is | 8 |
the place where you | 8 |
the sines and tangents | 8 |
the three points of | 8 |
the other given side | 8 |
east reclining d lat | 8 |
the thread being laid | 8 |
the th term required | 8 |
azimuth in the equal | 8 |
is made equal to | 8 |
one side of the | 8 |
of a fourth ark | 8 |
same extent applied the | 8 |
hour from towards noon | 8 |
much in length makes | 8 |
to find his declination | 8 |
from the point e | 8 |
distance from d to | 8 |
d from the south | 8 |
side opposite to one | 8 |
in the table of | 8 |
you have in the | 8 |
and tenth parts of | 8 |
the sine is to | 8 |
the suns altitude is | 8 |
thread fixed in the | 8 |
find the suns declination | 8 |
the residue is the | 8 |
to be added to | 8 |
touch the wall or | 8 |
and just against it | 8 |
angle found will be | 8 |
on each side the | 8 |
of the sun above | 8 |
then carry the compasses | 8 |
draw the circle bcde | 8 |
rectangle or product of | 8 |
the sun or star | 8 |
the motion of the | 8 |
side of the instrument | 8 |
the right angled triangle | 8 |
the given angle acute | 8 |
poles of the zodiack | 8 |
difference of versed sines | 8 |
either in the morning | 8 |
see in the figure | 8 |
then you must lay | 8 |
its complement to d | 8 |
the thread lying over | 8 |
about may but just | 8 |
one leg to the | 8 |
the side a b | 8 |
and the length in | 8 |
which is to be | 8 |
point of shadow d | 8 |
points of the compasse | 8 |
in the general scheam | 8 |
in summer is the | 8 |
the angle found will | 8 |
center of the dyal | 8 |
remain is the declination | 8 |
with your compasses the | 8 |
term is greater than | 8 |
the compassis in the | 8 |
out the parallel sine | 8 |
of the reclination of | 8 |
azimuth will be found | 8 |
the rectangle or product | 8 |
so is the third | 8 |
if you have a | 8 |
which is called the | 8 |
azimuth from east or | 8 |
help of the limb | 8 |
which is equal to | 8 |
enter it at the | 8 |
and the sum of | 8 |
the parts of the | 8 |
the first and second | 8 |
ledge of the fixed | 8 |
or the complement of | 8 |
and azimuth of the | 8 |
arks at the pole | 8 |
greatest declination of the | 8 |
is the logarithm of | 8 |
it from c to | 8 |
on the meridian from | 8 |
to find the true | 8 |
required to be found | 8 |
the latitude and altitude | 8 |
the true time sought | 8 |
of the bulls eye | 8 |
finde it to be | 8 |
cotangent of the given | 8 |
clock in the morning | 8 |
thread to the complement | 8 |
draw lines into the | 8 |
of the same radius | 8 |
the suns declination being | 8 |
in the end of | 8 |
and use of the | 8 |
the moons true place | 8 |
leggs from the half | 8 |
and enter one foot | 8 |
so is to a | 8 |
of the superficies of | 8 |
a side opposite to | 8 |
and the azimuth of | 8 |
on the same line | 8 |
you must turn the | 8 |
to find the hipotenusal | 8 |
of the carpenters rule | 8 |
the degrees it shall | 8 |
content in feet and | 8 |
m p m horizo | 8 |
zenith and the elevated | 8 |
declination out of the | 8 |
circle of the point | 8 |
a thread and plummet | 8 |
from the point g | 8 |
to prick down the | 8 |
with the line of | 8 |
perpendicular to the meridian | 8 |
is the declination of | 8 |
shall shew on the | 8 |
c as a center | 8 |
is the square of | 8 |
the sine complement of | 8 |
the reclination of a | 8 |
is equall to the | 8 |
point of the compasse | 8 |
altitude of the segment | 8 |
the bead amongst the | 8 |
the suns altitude for | 8 |
parts cut by the | 8 |
sine of the greatest | 8 |
d east reclining d | 8 |
and lay off the | 8 |
to the points of | 8 |
on the limb from | 8 |
in the second figure | 8 |
or feet and inches | 8 |
down from the center | 8 |
to every one of | 8 |
of the compassis in | 8 |
latteral tangent of the | 8 |
given angle be obtuse | 8 |
then the nd from | 8 |
of the tangent required | 8 |
at the other end | 8 |
the cosine of an | 8 |
of the first figure | 8 |
height above the substile | 8 |
the north end of | 8 |
the point in the | 8 |
of the first ship | 8 |
thread to the tangent | 8 |
and the bead amongst | 8 |
in the vertical circle | 8 |
upon the lines of | 8 |
to find the quantity | 8 |
may be found the | 8 |
in the center a | 8 |
secant of the hipotenusal | 8 |
a line drawn into | 8 |
so in summer is | 8 |
by the index and | 8 |
with the center of | 8 |
to the horizontal line | 8 |
the hours after the | 8 |
and the declination in | 8 |
less then a semicircle | 8 |
page to find the | 8 |
angle between the two | 8 |
east and west recliners | 8 |
if you have been | 8 |
line drawn into the | 8 |
the line bd of | 8 |
lines into the center | 8 |
as the sine is | 8 |
the answer will be | 8 |
to find the point | 8 |
on the loose piece | 8 |
south plaine declin d | 8 |
the table of the | 8 |
of the tower above | 8 |
draw a right line | 8 |
content of the whole | 8 |
interpose between the eye | 8 |
finde the inclination of | 8 |
the artificial sines and | 8 |
the nearest to the | 8 |
the complement thereof to | 8 |
a south plaine declin | 8 |
and the sum is | 8 |
brick and a half | 8 |
on the left hand | 8 |