«CODECLINATION»に関連する英語の本
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1
Elements of Trigonometry, Plane and Spherical: Adapted to ...
Then ZP will be the colatitude, PS the codeclination, z s the coaltitude, and the
angle ZPS the hour angle, or time of day, (apparent astronomical time). Given the
latitude of a place of observation 30° 43' 37" the sun's declination 19° 55' 42", his
...
Charles William Hackley,
1838
2
A treatise on trigonometry, plane and spherical, with its ...
... the altitude of any celestial object whose declination is known; for the
coaltitude, codeclination, and colatitude, will be three sides of a spherical triangle
. given to find the hour angle, comprised between the codeclination and the
colatitude.
3
A TREATISE ON TRIGONOMETRY, PLANE AND SPHERICAL
When the latitude of the place is known (and it may be found by the methods
already explained), the time may be computed from the altitude of any celestial
object whose declination is known ; for the coaltitude, codeclination, and
colatitude, ...
REV. CHARLES W. HACKLEY,
1853
4
The Mathematical Diary: Containing New Researches and ...
Now o=the angle forméd by the sun's coaltitude and codeclination, for they have
the angle formed by the circle of declination and the vertical through the lower
extremity of t, for their common complement. Let then o'=the angle formed by said
...
5
A Philosophical and Mathematical Dictionary: Containing an ...
In the foregoing figure, rs is the mean polar' distance, or mean codeclination of
the star 5, when the ll'JlP place of the pole is 0; and so the aparent codeclination;
also, the angle SP3 is the mean right ascension, and 5015 the app'arent one, ...
6
The Leeds Correspondent: A Literary, Mathematical and ...
55', the codeclination on April third, PS = 67° 45' the codeclination on the third of
June, and the included ^ SP.r = 15°; whence by case III oblique ^i'd spherics we
find ^ S*P = 38° 48'; and in the right ^'d A YZs, as rad : co-dec. *P :: sin.
7
Elements of plane and spherical trigonometry
When the latitude of the place is known, (and it may be found by the methods
already explained,) the time may be computed from the altitude of any celestial
object whose declination is known; for the co- altitude, codeclination, and
colatitude, ...
8
The Mathematical Diary: Containing Collections of Original ...
Let then q>'=the angle formed by said vertical and the meridian of New-York ;
also let l denote its colatitude, and D=the sun's
codeclination, then by a known
theorem in Spheric Trigonometry, I have sin. o : sin. l sin. <p' : sin. <p=^^'Xsin. ip'
but l ...
9
The Leeds Correspondent: A Literary, Mathematical, and ...
55', the codeclination on April third, PS = &T 45' the codeclination on the third of
June, and the included SP* = 15°; whence by case III oblique .<^'d spherics we
find Si-P = 38J 48'; and in the right ^i'd A PZ*, as rad : co-dec. si' :: sin. ^ ZsP : sin
...
John Ryley, John Gawthorp, John Whitley,
1818
10
Collection of English Almanacs for the Years 1702-1835
First , in an oblique — angled spherical triangle , there arc given two side* and an
included angle, viz. the codeclination — 820 19"' , the eolatitude ~ 370 54', and
the time from nosn — 6 trs 40 ^tnin □— ioo° 6'; to find the coaltitudeof the fun's ...