Last change
on this file since 14782 was 731, checked in by tbretz, 24 years ago |
*** empty log message ***
|
-
Property svn:executable
set to
*
|
File size:
1.4 KB
|
Line | |
---|
1 | #include "slalib.h"
|
---|
2 | #include "slamac.h"
|
---|
3 | float slaRverot ( float phi, float ra, float da, float st )
|
---|
4 | /*
|
---|
5 | ** - - - - - - - - - -
|
---|
6 | ** s l a R v e r o t
|
---|
7 | ** - - - - - - - - - -
|
---|
8 | **
|
---|
9 | ** Velocity component in a given direction due to Earth rotation.
|
---|
10 | **
|
---|
11 | ** (single precision)
|
---|
12 | **
|
---|
13 | ** Given:
|
---|
14 | ** phi float latitude of observing station (geodetic)
|
---|
15 | ** ra,da float apparent RA,Dec
|
---|
16 | ** st float local apparent sidereal time
|
---|
17 | **
|
---|
18 | ** phi, ra, dec and st are all in radians.
|
---|
19 | **
|
---|
20 | ** Result:
|
---|
21 | ** Component of Earth rotation in direction ra,da (km/s)
|
---|
22 | **
|
---|
23 | ** Sign convention:
|
---|
24 | ** The result is +ve when the observer is receding from the
|
---|
25 | ** given point on the sky.
|
---|
26 | **
|
---|
27 | ** Accuracy:
|
---|
28 | ** The simple algorithm used assumes a spherical Earth, of
|
---|
29 | ** a radius chosen to give results accurate to about 0.0005 km/s
|
---|
30 | ** for observing stations at typical latitudes and heights. For
|
---|
31 | ** applications requiring greater precision, use the routine
|
---|
32 | ** slaPvobs.
|
---|
33 | **
|
---|
34 | ** Last revision: 9 April 1998
|
---|
35 | **
|
---|
36 | ** Copyright P.T.Wallace. All rights reserved.
|
---|
37 | */
|
---|
38 |
|
---|
39 | #define ESPEED 0.4655 /* Nominal mean sidereal speed of Earth equator
|
---|
40 | in km/s (the actual value is about 0.4651) */
|
---|
41 |
|
---|
42 | {
|
---|
43 | return (float) ( ESPEED * cos ( (double) phi ) *
|
---|
44 | sin ( (double) ( st - ra ) ) *
|
---|
45 | cos ( (double) da ) );
|
---|
46 | }
|
---|
Note:
See
TracBrowser
for help on using the repository browser.