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 sine of the	350
the center of the	298
to the sine of	271
the complement of the	265
the motion of the	250
the quadrant of altitude	221
the place of the	216
the cosine of the	198
the difference of the	166
the versed sine of	161
the time of the	160
the length of the	152
the weight of the	149
to the tangent of	138
the tangent of the	135
is the sine of	133
the poles of the	130
the top of the	128
the height of the	121
the distance of the	119
the pressure of the	118
so is the sine	118
versed sine of the	114
of the fixed stars	112
as the sine of	111
the line of sines	109
that is to say	105
the sum of the	102
the end of the	99
the distance between the	99
when the sun is	98
the number of degrees	97
the beginning of the	96
the thread to the	96
the sine of d	95
of the sines of	95
the hour of the	93
to the other foot	91
the sun is in	91
of the sun and	90
the sines of the	89
the right ascension of	88
to the cosine of	88
the degree of the	87
early english books online	85
the pole of the	85
as the cosine of	85
the day of the	84
the square of the	83
by reason of the	83
place of the sun	80
the measure of the	79
the secant of the	79
the sun and moon	77
hour of the day	76
the arch of the	76
in the midst of	74
is equal to the	73
the axis of the	73
the elevation of the	72
the rest of the	72
from the center of	71
day of the moneth	70
to the versed sine	70
the tangent of d	70
the body of the	69
in the beginning of	69
for the most part	68
of the quadrant of	68
the altitude of the	68
sine of the angle	68
elevation of the pole	68
the middle of the	67
be found to be	67
lay the thread to	66
the nearest distance to	66
by the help of	66
right ascension of the	66
at the same time	65
the versed sines of	65
pressure of the air	64
less then a quadrant	64
take the nearest distance	63
greater then a quadrant	63
sine of the hour	62
time of the day	62
in the time of	61
the point of the	60
of the primum mobile	60
difference of the versed	60
to be in the	59
distance from the earth	58
and you will find	58
in the center of	58
of the versed sines	58
center of the world	57
of the angle sought	57
the latitude of the	56
the declination of the	56
in respect of the	56
of the line of	56
of the hour from	55
the index of the	54
the use of the	54
the centre of the	54
degree of the ecliptick	54
place of the sunne	54
of the suns altitude	53
the description of the	53
when the sun hath	53
declination of the sun	53
poles of the world	53
sun is in the	52
motion of the earth	52
one and the same	52
cosine of the latitude	52
to the square of	51
in the line of	51
versed sines of the	51
complement of the latitude	50
index of the hour	50
will be found to	50
in the university of	50
of the sun or	50
the midst of the	49
the intersection of the	49
the rectangle of the	49
of the given angle	49
pressure of the water	48
the surface of the	48
motion of the sun	48
the point of entrance	48
the hour and azimuth	48
laying the thread to	48
of the side sought	48
right angled spherical triangle	48
to find the angle	47
edge of the quadrant	47
thread to the other	47
is the difference of	47
the quantity of the	46
the motions of the	45
the east or west	45
the inhabitants of the	45
to the secant of	45
the azimuth from the	44
the course of the	44
that part of the	44
notes for div a	44
as well as the	44
the diameter of the	44
of the suns declination	44
the sun in the	43
latitude of the place	43
height of the pole	43
take the distance between	43
you will find the	43
nearest distance to it	43
the semidiameter of the	43
motion of the moon	43
the suns greatest declination	42
axis of the world	42
the declination in the	42
versed sine of d	42
sine of the azimuth	41
in the right angled	41
the difference between the	41
on the other side	41
quadrant of altitude to	41
at the end of	41
from the beginning of	41
the sides of the	41
is the cosine of	40
the angle of the	40
hour of the night	40
the tropick of cancer	40
to the difference of	40
distance of the sun	40
of the motion of	40
that the earth is	40
the shade of the	40
of the difference of	40
the doctrine of the	40
by help of the	39
sine of the latitude	39
the wall or cieling	39
the nature of the	39
a table of the	39
of the given side	39
the degrees of the	39
the light of the	39
the cotangent of the	38
to find the hour	38
past in the morning	38
to find the suns	38
characters represented either as	38
so is the difference	38
represented either as utf	38
the number of the	38
complement of the suns	38
of the moon from	38
by the motion of	37
how to find the	37
the true time of	37
so is the cosine	37
is the tangent of	37
the hour from noon	37
the a clock line	37
the angle opposite to	36
the moon from the	36
number of degrees of	36
the parallel of the	36
center of the earth	36
the meridian of the	36
cosine of the declination	36
the area of the	36
the a clock hour	36
in the centre of	36
of the nature of	36
it is to be	36
be equal to the	36
sines of the suns	35
of the complement of	35
of the hour circle	35
of the same weight	35
on the quadrant of	35
the parts of the	35
the bottom of the	35
the distance from the	35
true time of the	35
the globe of the	35
in the middle of	35
the circle of position	35
a clock in the	35
being added to the	35
at the time of	35
from the authority of	34
which is all one	34
degrees of the equator	34
on the west with	34
by the name of	34
to the motion of	34
for the latitude of	34
from her cardinal point	34
which being added to	34
according to nearest distance	34
of mathematicks in the	34
to the complement of	34
sine of the declination	34
to the cotangent of	34
the theory of the	34
the same with the	34
difference of the sines	34
is said to have	34
professor of mathematicks in	34
be found in the	34
the feast of easter	34
into two equal parts	34
days from her cardinal	34
and the reason is	33
so the tangent of	33
as the tangent of	33
the head of the	33
parallel to the horizon	33
distance from the meridian	33
so is the radius	33
from east to west	33
a ruler laid from	33
square of the radius	33
be less then a	33
of altitude to the	33
the right angled spherical	33
is bounded on the	33
so the sine of	33
day of the month	33
is said to be	33
half sum of the	33
the true motion of	33
be added to the	33
professor of mathematicks at	32
measure of the angle	32
from west to east	32
and so is the	32
the pondus of the	32
the foot of the	32
table of oblique ascensions	32
the scale of entrance	32
is to the radius	32
is not to be	32
after the same manner	32
the help of the	32
the radius of the	32
the potentia of the	31
inhabitants of the moon	31
part of the world	31
moon from the sun	31
the reason of the	31
of the sine of	31
tangent of the latitude	31
and setting of the	31
poles of the ecliptick	31
globe of the earth	31
length of the day	31
on the east with	31
which is in the	31
the sun to be	31
altitude of the sun	31
a table of oblique	31
in the equal limb	30
sine of the altitude	30
the half sum of	30
to find an angle	30
line of versed sines	30
oblique angled spherical triangle	30
of the azimuth from	30
on the line of	30
on the south with	30
the side sought as	30
of the ark of	30
the latitude of london	30
rising and setting of	30
cosine of the altitude	30
the face of the	30
parallel of the day	30
the sine of half	30
semidiameters of the earth	29
the thread over the	29
the sun hath d	29
the thread laid over	29
on the north with	29
have it to be	29
the true place of	29
angle opposite to the	29
of the pole above	29
is to the sine	29
weight of the air	29
center of the quadrant	29
it is in the	29
the same number of	29
bounded on the east	29
the order of the	29
to the latitude of	29
is one of the	28
the meridian at midnight	28
the opinion of the	28
of the sun to	28
of one of the	28
the shadow of the	28
the mouth of the	28
the globe till the	28
the distances of the	28
the scale and the	28
the side opposite to	28
is distant from the	28
right angled spherical triangles	28
pass through the meridian	28
a pillar of water	28
sub sub sub sub	28
in the scale of	28
side opposite to the	28
so is the tangent	28
taken out of the	28
to find the time	28
the thred to the	27
true place of the	27
mathematicks in the university	27
to the degree of	27
from the sine of	27
foot of the compasses	27
theory of the planets	27
the reason of this	27
the cusp of the	27
are said to be	27
point of the horizon	27
find the time of	27
the difference of longitude	27
the places of the	27
be the same with	27
find the hour of	27
the heat of the	27
to one of them	27
is that which is	27
of the sun in	27
secant of the latitude	27
the oblique ascension of	27
from the end of	27
between the scale and	27
sine of half the	27
a clock hour circle	26
in the space of	26
the tangent of half	26
nearest distance to the	26
scale and the thread	26
the earth and the	26
an arch of the	26
his distance from the	26
in the next place	26
so the cosine of	26
sum of the sines	26
the beginning of aries	26
is the number of	26
of the poles elevation	26
a line of sines	26
be greater then a	26
number of degrees and	26
the plane of the	26
given to find the	26
parts of the world	26
the side of the	26
the rising and setting	26
by reason of their	26
of degrees and minutes	26
in the same manner	26
are of the same	26
opposite to one of	26
will have it to	26
foot of your compasses	26
the sun or stars	26
be of the same	26
bring the place of	26
on the right edge	25
when he is in	25
it be required to	25
to the meridian of	25
what degree of the	25
the sunne and moone	25
it were required to	25
on the left edge	25
the upper part of	25
the ark of difference	25
the diameter of a	25
of the first magnitude	25
weight of the water	25
centre of the world	25
is to be observed	25
of the angle at	25
the product will be	25
an island in the	25
to be the same	25
rectangle of the sines	25
is nothing else but	24
is the complement of	24
opposite to the other	24
and the opposite side	24
to secant of the	24
one foot of the	24
the cosecant of the	24
if you would know	24
foot of the compassis	24
the cause of this	24
case of right angled	24
found to be d	24
suns distance from the	24
the vses of the	24
degrees and minutes of	24
of the angle opposite	24
the points of the	24
a star of the	24
in the versed sine	24
the meridian of london	24
the tropick of capricorn	24
about the globe till	24
that the pressure of	24
all the parts of	24
a table shewing the	24
that there is no	24
distance from the sun	24
that are in the	24
thread laid over the	24
region of the air	24
in reference to the	24
on the north side	24
in the first place	24
that there is a	24
to the opinion of	24
part of the earth	24
in the latitude of	24
sine of the suns	24
of half the angle	24
the air within the	24
of the sun from	23
to the common radius	23
lay the thread over	23
between the zenith and	23
find it to be	23
of a line of	23
other parts of the	23
and the index of	23
then lay the thread	23
which being deducted from	23
of the same kind	23
clock in the morning	23
a part of the	23
the first point of	23
if it be said	23
potentia of the surface	23
add add add add	23
ark of difference between	23
point of the compass	23
the earth to be	23
to the top of	23
time of the sun	23
the sine of a	23
side sought as the	23
at the hour of	23
the suns distance from	23
the parts of a	23
any part of the	23
come to the meridian	23
to the terms of	23
the force of the	23
oblique ascension of the	23
the suns true place	23
in regard of the	23
in the year of	23
from the east or	23
parts of the earth	23
the horizon of the	23
degrees above the horizon	23
i text is available	22
center of the glasse	22
degree of the equator	22
keyed and coded from	22
the edge of the	22
the line of latitudes	22
markup reviewed and edited	22
financial support to the	22
online text creation partnership	22
coded from proquest page	22
edition of the work	22
iv tiff page images	22
the early english books	22
complement of the poles	22
from proquest page images	22
heat of the sun	22
work described above is	22
text is available for	22
text can be copied	22
world in the moone	22
the superficies of the	22
assigned for keying and	22
or which is all	22
of the second book	22
keyboarded and encoded edition	22
end of the quadrant	22
images scanned from microfilm	22
the institutions providing financial	22
by the institutions providing	22
that the sun is	22
described above is co	22
degrees of the equinoctial	22
text and markup reviewed	22
encoded text transcribed from	22
at the sine of	22
and encoded edition of	22
all without asking permission	22
of the work described	22
and coded from proquest	22
one foot of your	22
institutions providing financial support	22
phase i text is	22
tcp assigned for keying	22
this keyboarded and encoded	22
the right edge of	22
encoded edition of the	22
the text can be	22
in the head of	22
to the early english	22
screw the quadrant of	22
the nearest distance from	22
the plain of the	22
the azimuth of the	22
terms of creative commons	22
even for commercial purposes	22
by which it is	22
doctrine of the sphere	22
owned by the institutions	22
circles of the sphere	22
to be added to	22
of the said ark	22
let there be given	22
this phase i text	22
right edge of the	22
books online text creation	22
according to the terms	22
is the same with	22
and markup reviewed and	22
it to be the	22
from the right edge	22
the altitude in the	22
and minutes of the	22
the terms of creative	22
english books online text	22
the work described above	22
providing financial support to	22
support to the early	22
for keying and markup	22
of degrees of the	22
the radius to the	22
turn about the globe	22
is clear from the	22
the side m h	22
is available for reuse	22
the third part of	22
of the third side	22
pole of the world	22
sines from the center	21
complement of the altitude	21
as you may see	21
nearest distance from the	21
and on the south	21
tangent of half the	21
of the christian aera	21
so much is the	21
you must place one	21
third part of the	21
beginning of the christian	21
is to be added	21
the two including sides	21
is an arch of	21
the other side of	21
is the measure of	21
the circle of the	21
to the axis of	21
must place one foot	21
be found by the	21
of the celestial motions	21
was placed in heaven	21
of the three sides	21
the angle of inclination	21
line of sines from	21
the zenith and the	21
distance to the thread	21
hourly motion of the	21
the north and south	21
to find the side	21
place of the moone	21
laid to the other	21
thred to the other	21
past in the afternoon	21
the sun and the	21
place one foot of	21
in the oblique angled	21
of a great circle	21
true motion of latitude	21
seasons of the year	21
of the dragons head	21
may be found by	21
about the end of	21
of sines from the	20
azimuth from the south	20
some part of the	20
the thread in the	20
the same with that	20
all the world over	20
so when the sun	20
the point where the	20
point of the ecliptick	20
true nature of the	20
he is in the	20
middle region of the	20
the lower end of	20
from the poles of	20
the help of a	20
azimuth of the sun	20
the heigth of the	20
the bead to the	20
sine of the said	20
and for this reason	20
pole of the circle	20
the sine of m	20
is evident from the	20
of the half sum	20
is not able to	20
of the sun is	20
of the suns rising	20
the pillar of water	20
to the thread laid	20
of the sunne and	20
light of the sun	20
half the difference of	20
latitude of the moon	20
upon the top of	20
and so of the	20
that can be made	20
the moons mean motions	20
the inches of mercury	20
let it be required	20
the true nature of	20
by the pressure of	20
cosine of the angle	20
there is not any	20
declination under the earth	20
the globe and quadrant	20
time of the night	20
the east side the	20
as it is in	20
and of the ark	20
from the top of	20
so of the rest	20
in the end of	20
a clock hour line	20
be the tangent of	19
such instances will never	19
assumptions that can be	19
the suns azimuth from	19
will be marked as	19
the text encoding initiative	19
that due credit and	19
to external keying companies	19
their works are eligible	19
errors will remain and	19
of the center of	19
texts for their own	19
bibliography of english literature	19
were corrected where possible	19
cosine of the given	19
intended to range over	19
up to a limit	19
are available at the	19
title published between and	19
as opposed to critical	19
edition of a work	19
of michigan and oxford	19
therefore of any assumptions	19
all likelihood such instances	19
is given to their	19
a work was chosen	19
partnership between the universities	19
works in english were	19
corrected where possible up	19
be aware of the	19
was chosen if there	19
to the keyers to	19
companies for transcription and	19
are a number of	19
and therefore of any	19
overall quality of tcp	19
and use these texts	19
is a partnership between	19
was enhanced and or	19
then carried out by	19
texts created during phase	19
aimed to produce large	19
and those which did	19
some readable characters will	19
and or corrected and	19
qa standards were returned	19
is the distance of	19
from the center a	19
at the text creation	19
is the cause of	19
is to be found	19
sets published by proquest	19
the end of it	19
square of the sine	19
mnemonic sdata character entities	19
were encoded and linked	19
users should bear in	19
tcp is a partnership	19
converting tcp files to	19
general aim of eebo	19
divided into two phases	19
a second or later	19
of every monographic english	19
chose to create diplomatic	19
the project have been	19
standards were returned to	19
tcp is to encode	19
top of the tub	19
credit and attribution is	19
chosen if there was	19
for an anonymous work	19
or for an anonymous	19
project have been released	19
language title published between	19
part of the horizon	19
project restraints of time	19
nothing else but the	19
page images in accordance	19
and some readable characters	19
the suns right ascension	19
if it were required	19
should bear in mind	19
by university of nebraska	19
take and use these	19
be marked as illegible	19
proquest via their early	19
in mind that in	19
were returned to the	19
texts were encoded and	19
should be aware of	19
later edition of a	19
by converting tcp files	19
the east and west	19
the keyers to be	19
keying and markup guidelines	19
cambridge bibliography of english	19
text with mnemonic sdata	19
within the usual project	19
into the public domain	19
never have been looked	19
characters or elements to	19
in english were prioritized	19
a limit of instances	19
been transformed into placeholder	19
compelling reason to do	19
there are a number	19
over a wide variety	19
published by proquest via	19
accordance with level of	19
tcp data is very	19
publisher proquest to create	19
of any assumptions that	19
opposed to critical editions	19
or later edition of	19
aware of the process	19
now take and use	19
second or later edition	19
tcp aimed to produce	19
nature of the print	19
and available in eebo	19
the overall quality of	19
for their own purposes	19
the obliquity of the	19
returned to the keyers	19
assurance was then carried	19
elements of known extent	19
gap elements of known	19
these processes should make	19
created during phase of	19
suns azimuth from the	19
of each text was	19
based on the text	19
request that due credit	19
data is very good	19
the first day of	19
unicode or tei g	19
of works in other	19
large quantities of textual	19
project was divided into	19
range over a wide	19
quantities of textual data	19
a compelling reason to	19
and attribution is given	19
included and sometimes a	19
the public domain as	19
p using tcp tei	19
users should be aware	19
published between and available	19
by proquest via their	19
external keying companies for	19
limit of instances per	19
on the image sets	19
have been transformed into	19
and encoded texts based	19
or tei g elements	19
and markup guidelines are	19
unicode or text strings	19
the print record of	19
mind that in all	19
created by converting tcp	19
their early english books	19
tei in libraries guidelines	19
the encoding was enhanced	19
tei p using tcp	19
use these texts for	19
of known extent have	19
changes to facilitate morpho	19
the image sets published	19
or text strings within	19
to simplify the filling	19
characters marked as illegible	19
the publisher proquest to	19
texts have been issued	19
selection was based on	19
and oxford and the	19
in of gaps by	19
gaps by user contributors	19
the process of creating	19
files to tei p	19
work was chosen if	19
keyers to be redone	19
the th of april	19
there was a compelling	19
whichever is the greater	19
selection was intended to	19
known extent have been	19
were sent to external	19
processed by university of	19
been looked at by	19
and draw the line	19
the fourteenth day of	19
of the project have	19
respectfully request that due	19
notably latin and welsh	19
motion of the heavens	19
the tei in libraries	19
have been issued variously	19
was based on the	19
based on the new	19
the fourth part of	19
the universities of michigan	19
tcp files to tei	19
level of the tei	19
cut the primitive circle	19
for transcription and basic	19
accurately transcribed and encoded	19
have been released into	19
new cambridge bibliography of	19
which is to be	19
and linked to page	19
or elements to simplify	19
filling in of gaps	19
was proofread for accuracy	19
illegibles were encoded as	19
each text was proofread	19
was intended to range	19
between the pole and	19
at by a tcp	19
domain as of january	19
the general aim of	19
the texts were encoded	19
mainly structural encoding based	19
linked to page images	19
of the texts have	19
readable characters will be	19
during phase of the	19
by editorial teams in	19
out by editorial teams	19
anyone can now take	19
sets were sent to	19
were encoded as gap	19
if there was a	19
and the publisher proquest	19
to reflect the true	19
corrected and characters marked	19
did not meet qa	19
if the hipotenusal be	19
proquest to create accurately	19
to encode one copy	19
the usual project restraints	19
in all likelihood such	19
universities of michigan and	19
the pillar of air	19
elements to simplify the	19
restraints of time and	19
to create diplomatic transcriptions	19
creation partnership web site	19
usual project restraints of	19
oxford and the publisher	19
available at the text	19
the line of the	19
to tei p using	19
released into the public	19
text was proofread for	19
extent have been transformed	19
of difference between the	19
bear in mind that	19
that it may be	19
of the print record	19
encoding based on the	19
produce large quantities of	19
encoded as gap s	19
into placeholder characters or	19
was a compelling reason	19
text selection was based	19
with level of the	19
likelihood such instances will	19
of a works in	19
reflect the true nature	19
that in all likelihood	19
sent to external keying	19
but we respectfully request	19
text creation partnership web	19
works are eligible for	19
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to the east side	19
the new cambridge bibliography	19
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image sets published by	19
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instances will never have	19
encoding was enhanced and	19
of time and funding	19
placeholder characters or elements	19
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was then carried out	19
the texts have been	19
transformed into placeholder characters	19
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day of the moon	19
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as illegible were corrected	19
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of gaps by user	19
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editorial teams in oxford	19
by a tcp editor	19
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variety of subject areas	19
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between the universities of	19
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illegible were corrected where	19
text strings within braces	19
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diameter of the earth	19
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works in other languages	19
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in oxford and michigan	19
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encoded texts based on	19
editions of a works	19
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data within the usual	19
transcription and basic encoding	19
a works in english	19
then their works are	19
ascii text with mnemonic	19
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the west with the	18
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upon the surface of	18
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the suns altitude at	17
your string from the	17
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out of the earth	17
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table of right ascensions	17
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the north side the	17
you desire to know	17
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pole of the ecliptick	17
degree of the horizon	17
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the uses of the	17
of the said thread	17
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fourteenth day of the	17
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the other end of	17
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the just weight of	17
the most part of	17
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of the other planets	17
the same manner as	17
the summe of the	17
half an hour past	17
to that of the	17
under the title of	17
the given angle be	17
of the sum of	17
the sine of b	17
and from the point	17
scale of equal parts	17
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to the testimony of	17
the east side of	17
said to be in	17
the longitude and latitude	17
the content of the	17
arch of the aequator	17
bright star in the	17
is greater then the	17
the line of chords	17
and difference of the	17
part of the heavens	17
right angles in the	17
as much as the	17
is to the square	17
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sun hath d of	16
of the use of	16
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the part of the	16
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a surface of water	16
a treatise of the	16
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may thus be found	16
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part of the meridian	16
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place of the moon	16
you come to the	16
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to the winter ecliptick	16
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a b c d	16
and the brasen meridian	16
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the moon to be	16
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of the fixed starres	16
by the weight of	16
the west side the	16
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place in the ecliptick	16
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the matter of the	16
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the sphere of the	16
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one of the most	16
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that number of degrees	16
is represented by the	16
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of the royal society	15
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angle m e h	14
a s a a	14
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altitudes on all hours	14
meridian at midnight about	14
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the houre of the	14
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place of the aphelion	14
the zenith and nadir	14
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other end of the	14
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meridian of the place	14
fourth part of the	14
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the observation of the	14
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the line of tangents	14
the phenomena of the	14
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the year of the	14
body of the moone	14
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of aries and libra	14
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line of sines on	13
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meridian comprehended between the	13
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i make a prick	13
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by which if you	13
one of the greatest	13
is found to be	13
the east with the	13
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scale of a ballance	13
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then to find the	13
c d e f	13
the sine of one	13
of the gnomonical semi	13
of the earth as	13
d e f g	13
the bowels of the	13
meridian altitude of the	13
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bensil of the air	13
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the year of our	13
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the moon and the	13
true place in the	13
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colure to the meridian	13
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the time when the	13
side of the quadrant	13
secant of the declination	13
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the angle of and	13
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one from the other	13
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arch of the meridian	13
the former extent between	13
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the first part of	13
motion of the fixed	13
a circle being given	13
meridian of the world	13
the first and second	13
dial a upon the	13
that it is the	13
according to the common	13
to the center of	13
the two first tearms	13
motion of the planets	13
it comes to pass	13
arch of the horizon	13
the degrees and parts	13
at right angles with	13
under the same degree	13
the time of his	13
is by the arabs	13
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height of the tower	13
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line of equal parts	13
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whole weight of the	13
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the surface of air	13
star from the meridian	13
the mean motions of	13
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the centers of the	13
that extent at the	13
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sine of one of	13
cotangent of the latitude	13
the distance of a	13
thread in the limb	13
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your scale of equal	13
a table of right	13
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the index points to	13
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if they had been	13
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you will find it	12
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place of the earth	12
the circumference of the	12
part of the globe	12
the thread laid to	12
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the pressure upon the	12
in the publick library	12
if you would have	12
is greater then a	12
of the julian period	12
thread laid to the	12
this is evident from	12
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the element of air	12
a line of chords	12
in like manner may	12
right ascensions and declinations	12
the pole is elevated	12
other foot of the	12
let us suppose the	12
point in the horizon	12
to this i answer	12
of the other sides	12
than any of the	12
thorow the poles of	12
will be to find	12
rising of a star	12
compounded table of the	12
the swiftnesse of the	12
more of him in	12
position of the sphere	12
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beams of the sun	12
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in a straight line	12
of the earths shadow	12
the sunne being in	12
nearer to the earth	12
head of the comet	12
it is parted from	12
e f g a	12
every degree of the	12
published in the year	12
time of sun rising	12
center of the epicycle	12
motions of the planets	12
is to the cosine	12
right angled sphoerical triangles	12
the pole above the	12
what constellations rise with	12
are to be sold	12
as was said before	12
f g a b	12
through the center of	12
a compounded table of	12
of the first meridian	12
plain of the horizon	12
is set on fire	12
as well of the	12
every one of these	12
the other part of	12
i elevate the pole	12
for finding out the	12
that side of the	12
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diameters of the earth	12
from which it is	12
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the gnomonical semi circle	12
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an hour past in	12
hour past in the	12
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hour and azimuth in	12
to find the declination	12
desire to know the	12
the same weight with	12
use of the globes	12
on the east side	12
sine of m b	12
cosecant of the side	12
magnitude is to the	12
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to the same point	12
from this experiment we	12
the affection of the	12
so cosine of the	12
to be the center	12
the shape of a	12
meridian line on the	12
foot according to nearest	12
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both sides of the	12
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in this case the	12
the season of the	12
the setting of a	12
the rising of a	12
to find a side	12
is to be noted	12
apogaeum of the eccentrick	12
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cosine of the side	12
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eclipse of the moon	12
of a right angled	12
if it be not	12
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center of the dial	12
cosecant of the given	12
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side greater then a	12
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signs of the zodiack	12
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the angle b a	12
the sun or star	12
to find the content	12
in a right sphere	12
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the heavens to be	12
g a b c	12
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the table of the	12
the hourly motion of	12
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azimuth from the vertical	12
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the one half of	12
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that of the earth	12
the beginning of this	12
at the cosine of	12
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of the earth from	12
number of degrees that	12
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by some of the	12
tangent of halfe the	12
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on the west side	12
of the planets in	12
when the sunne is	12
the edges of the	12
lines from the center	12
which if you multiply	12
of the earth in	12
in this example is	12
so tangent of the	12
there is no such	12
what a clock it	12
we may find the	12
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some of the most	12
about the same time	12
as may appear by	12
which being subtracted from	12
where the end of	12
side of the meridian	12
and screw the quadrant	12
the azimuth in the	12
greatest declination of the	12
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upon the terrestrial globe	12
angle m b h	12
about the time of	12
ascension of the mid	12
the vse of the	12
the north with the	12
of the side opposite	12
side opposite to one	12
cycle of the moon	12
difference between the two	12
the pole and the	12
count the number of	12
of the sun at	12
the elevation of london	12
in the middle region	12
the first book of	12
globe till the index	12
a pillar of mercury	12
is in the zenith	12
and what remaineth is	12
by the force of	12
and the point of	12
being of the same	12
a catalogue of the	11
the sun to the	11
the motion of a	11
from the left edge	11
and bring it to	11
you must lay the	11
sines of the containing	11
of the table of	11
is not so much	11
this extent at the	11
region of the aire	11
the sun and moone	11
open your compasses at	11
at the same distance	11
distances of the hour	11
may be called the	11
the sunne in the	11
which are in the	11
from the original text	11
setting one foot of	11
to which is added	11
opposite side greater then	11
of right angled sphoerical	11
one degree of longitude	11
circumference of a circle	11
praecession of the aequinox	11
put forth a treatise	11
and that they are	11
through the poles of	11
the angle at a	11
is the sum of	11
to find the true	11
the side of a	11
is the point of	11
so called from the	11
of the air lm	11
motion on its axis	11
be subtracted from the	11
is the degree of	11
given to find an	11
our latitude of london	11
which he dedicated to	11
the horizon and the	11
of the sun given	11
is the place of	11
to the cosecant of	11
the point in the	11
yet it is not	11
the tangent of halfe	11
the university of oxford	11
surface of the stagnant	11
it to the meridian	11
the sun it self	11
to be in a	11
being multiplyed by the	11
in any of the	11
must lay the dial	11
in the place of	11
first tearm in the	11
middle place of the	11
of the first and	11
the ascensional difference of	11
in reference to this	11
as the sun is	11
the angle of position	11
for the confirmation of	11
the knowledge of the	11
out of the scale	11
according to the former	11
from the elevated pole	11
the equinoctial and the	11
the ark of the	11
to find the area	11
as much pressure in	11
sum or difference of	11
the earth to the	11
the stars in heaven	11
to work proportions in	11
centre of the universe	11
the eccentrick place of	11
the suns altitudes on	11
tangent of the said	11
the angles of the	11
of them being given	11
diameter of a circle	11
of the moone from	11
they are in the	11
the sine of any	11
the words of scripture	11
the middle motion of	11
an account of the	11
meridian and the brasen	11
intersection of the meridian	11
which is called the	11
the hipotenusal be greater	11
find the place of	11
the line of lines	11
therefore i elevate the	11
the eye and the	11
the sun shall have	11
of the versed sine	11
towards the south pole	11
altitude or depression at	11
the sun hath deg	11
the remainder is the	11
to the extent of	11
these are the distances	11
the first tearm in	11
latitude of your place	11
in the parallel of	11
to find in what	11
for finding the azimuth	11
of the pressure of	11
as if you would	11
the influence of the	11
a right angled spherical	11
is the angle m	11
the orbe of the	11
according to the theorem	11
find the colure cut	11
the original text notes	11
weight of the pillar	11
suns altitudes on all	11
quadrant of altitude in	11
in which the sun	11
of the meridian with	11
he treats of the	11
a line at pleasure	11
of day and night	11
open your compasses to	11
difference of the sides	11
earth is in the	11
so much as the	11
that which is called	11
be in the center	11
hour from the meridian	11
the complement of latitude	11
line of a clock	11
if the sun have	11
in the table of	11
and the place of	11
the latitude of your	11
it will cut the	11
of the air is	11
about the body of	11
difference of the base	11
through the sights you	11
turn the globe till	11
and the meridian of	11
at of the clock	11
the same to the	11
as is the weight	11
be less then the	11
and by reason of	11
the image of the	11
from the right ascension	11
in the description of	11
the foundations of the	11
of the measuring of	11
the fixed stars are	11
points to a clock	11
the contents of the	11
between the two including	11
the tables of the	11
the secant of d	11
to the side m	11
and the distance between	11
are given to find	11
the two middle tearms	11
sine of the ark	11
how many degrees of	11
center of the said	11
shall be the hour	11
and there make a	11
a great deal of	11
be d from the	11
the middle place of	11
in sines and tangents	11
m e h and	11
sine of an arch	11
the opposite side greater	11
that of the sun	11
equal to the distance	11
sphere of the fixed	11
between the equinoctial and	11
text notes for div	11
have nothing to do	11
against it in the	11
the day will be	11
till the index points	11
the cuspis of the	11
of the differences of	11
and the potentia of	11
the angle sought as	11
that it is in	11
so that the longest	11
secant of the angle	11
tangent of the side	11
and it will cut	11
quarter of an hour	11
to the angle sought	11
the suns meridian altitude	11
of the sunnes apogaeum	11
the bounds of the	11
it is said to	11
in the quadrant of	11
if the declination be	11
from the death of	11
therefore it containeth it	11
the scale of a	11
original text notes for	11
on the th of	11
of the clock in	11
by the side of	11
the sides of a	11
before the death of	11
from the east point	11
of the day and	11
the sun being in	11
side less then a	11
soul of the world	11
to tangent of the	11
in the yeare of	11
upon the quadrant of	11
on the terrestrial globe	11
the longitude of the	11
in an oblique sphaere	11
it must needs be	11
sides with the angle	11
of the doctrine of	11
substiles distance from the	11
the quadrant of latitudes	11
seen in the morning	11
it is called by	11
then i turn the	11
pressure of the vvater	11
so have you the	11
motion of the moone	11
the bright star in	11
a clock it is	11
till it come to	11
comprehended between the pole	11
degrees and an halfe	11
the substiles distance from	11
be the sine of	11
not to be understood	11
the sine of that	11
circles parallel to the	11
draw a line at	10
to the meridian at	10
same distance from the	10
and the angle at	10
part of a surface	10
that point of the	10
is the right ascension	10
which may be done	10
of the meridian altitude	10
the base of the	10
of the surface of	10
a quarter of an	10
angle sought as the	10
the university of paris	10
of that arks complement	10
opposite side less then	10
is the secant of	10
to be divided into	10
meridian or a clock	10
of the ecliptick the	10
weight of the vvater	10
the other middle tearm	10
pondus and the potentia	10
half difference of the	10
find the azimuth of	10
the ebbing and flowing	10
in any part of	10
one part of the	10
the difference of right	10
the west side of	10
the leggs from the	10
of the circles of	10
to the right ascension	10
lowest region of the	10
of that extent at	10
therefore it must be	10
of versed sines to	10
counted from the right	10
eclipses of the sun	10
as high as the	10
of the other to	10
like may be done	10
as it were in	10
from the time of	10
body of the earth	10
or in the afternoon	10
the distance thereof from	10
the eclipse of the	10
of a fluid is	10
they come to the	10
as the radius is	10
are the same with	10
of the euxine sea	10
oblique angled spherical triangles	10
the complement of it	10
in the triangle a	10
of the point sought	10
such proportion to the	10
meridian between the zenith	10
of the pole of	10
the new star in	10
the opposite side less	10
will be equal to	10
length of the shaddow	10
to one degree of	10
to the hour of	10
the author of this	10
in his own language	10
time when the sun	10
the hipotenusal be less	10
the seasons of the	10
in the constellation of	10
from the complement of	10
the stars in the	10
the end of that	10
of the angle b	10
the continuance of the	10
distant from the equator	10
face of the earth	10
the publick library at	10
be the cause of	10
the half whereof is	10
rectifie the globe to	10
thread and the scale	10
the suns place to	10
the pressure of a	10
of the stagnant mercury	10
the beginning of cancer	10
of the two middle	10
and the time of	10
of the suns distance	10
to a fourth sine	10
the latter end of	10
for the time of	10
as it were a	10
rising of the sun	10
page against degree for	10
eccentrick place of the	10
the side m e	10
under the name of	10
tangent of the complement	10
those things that are	10
and there i make	10
the greatest part of	10
parts of an hour	10
take a view of	10
the bredth of the	10
vpon the houre circle	10
unformed stars belonging unto	10
north declination under the	10
is taken from the	10
the building of rome	10
in so much that	10
for put the case	10
to the nature of	10
you have nothing to	10
that part of heaven	10
by the coelestial globe	10
course of the sun	10
the same distance from	10
from the noon meridian	10
that it was not	10
surface of the water	10
in the said reflected	10
the equator at the	10
of the latitude of	10
which being multiplyed by	10
is in the equinoctial	10
the plaine of the	10
it will be found	10
the west part of	10
according to the rules	10
he published likewise a	10
west side the horizon	10
to the meridian between	10
sunne being in the	10
and enter the former	10
one of the including	10
the variation of the	10
by which means the	10
then in the right	10
it must needs follow	10
not being able to	10
sine of the difference	10
the mercury in the	10
that when the sun	10
in the catalogue of	10
not be able to	10
what point of the	10
of the suns meridian	10
to be understood of	10
the pondus and the	10
to the same radius	10
body of the sunne	10
the perigaeum of the	10
the north pole of	10
towards the left hand	10
at any time of	10
anomaly of the orbe	10
from east or west	10
from the zenith to	10
you would know the	10
is the just weight	10
the bright star of	10
the longest day is	10
semidiameter of the earth	10
is a part of	10
find the heigth of	10
made on the globe	10
of the tangent of	10
towards the depressed pole	10
the study of astronomy	10
the halfe sum of	10
the clock in the	10
of the given sides	10
of the altitude sought	10
tangent of the angle	10
of the meridian and	10
of the weight of	10
to a whole circle	10
to make use of	10
or point of the	10
being given to find	10
sunne is in the	10
but it may be	10
meridian with the horizon	10
there is no need	10
a line of tangents	10
and that of the	10
if one of the	10
minutes past in the	10
natural sine of the	10
south declination under the	10
the lower part of	10
north side of the	10
greatest distance from the	10
in greek and latine	10
by the revolution of	10
part of an inch	10
complement of the stars	10
right ascension of a	10
of the side a	10
distant from the pole	10
towards the elevated pole	10
of the small quadrant	10
stars belonging unto this	10
you would have the	10
the art of navigation	10
found to be deg	10
top of the tower	10
was placed in the	10
being sought in the	10
and is called the	10
to find the heigth	10
as also of the	10
that space of time	10
it consists according to	10
of degrees that the	10
semidiameter of the sun	10
sines of the sum	10
to the inhabitants of	10
two sides with the	10
because the pressure of	10
to the east point	10
to draw the reflected	10
the scituation of the	10
from the body of	10
as they are in	10
then the latitude of	10
the horizon with the	10
how to finde the	10
just touch the thread	10
hours of the day	10
is found in the	10
the parralels of altitude	10
of altitude comprehended between	10
by the line of	10
the notches of the	10
the horizon in the	10
of the order of	10
to make the day	10
and therefore it is	10
bright one in the	10
the hour from midnight	10
of the equinoctiall circle	10
the center of that	10
three sides are given	10
proportions in sines and	10
or angle of the	10
put forth a small	10
middle motion of the	10
the cube of the	10
the moone from the	10
altitude comprehended between the	10
the hour lines of	10
center of the circle	10
of the night by	10
the northern temperate zone	10
with the angle comprehended	10
it is also called	10
halfe sum of the	10
the radius is to	10
houre of the day	10
the appearance of the	10
declination in the scale	10
find the angle of	10
part of the said	10
to be of a	10
to one of the	10
theory of the earth	10
perigaeum of the eccentrick	10
secant of the complement	10
the scruples of incidence	10
the proportion of the	10
of sines on the	10
west part of the	10
foundations of the earth	10
of the latitude in	10
the weight of a	10
any time of the	10
the power of the	10
the dimensions of the	10
the ecliptick in the	10
to pass through the	10
so long as the	10
of degrees from the	10