Last change
on this file since 4992 was 731, checked in by tbretz, 24 years ago |
*** empty log message ***
|
-
Property svn:executable
set to
*
|
File size:
1.2 KB
|
Line | |
---|
1 | #include "slalib.h"
|
---|
2 | #include "slamac.h"
|
---|
3 | double slaPav ( float v1 [ 3 ], float v2 [ 3 ] )
|
---|
4 | /*
|
---|
5 | ** - - - - - - -
|
---|
6 | ** s l a P a v
|
---|
7 | ** - - - - - - -
|
---|
8 | **
|
---|
9 | ** Position angle of one celestial direction with respect to another.
|
---|
10 | **
|
---|
11 | ** (single precision)
|
---|
12 | **
|
---|
13 | ** Given:
|
---|
14 | ** v1 float[3] direction cosines of one point
|
---|
15 | ** v2 float[3] direction cosines of the other point
|
---|
16 | **
|
---|
17 | ** (The coordinate frames correspond to RA,Dec, Long,Lat etc.)
|
---|
18 | **
|
---|
19 | ** The result is the bearing (position angle), in radians, of point
|
---|
20 | ** v2 with respect to point v1. It is in the range +/- pi. The
|
---|
21 | ** sense is such that if v2 is a small distance east of v1, the
|
---|
22 | ** bearing is about +pi/2. Zero is returned if the two points
|
---|
23 | ** are coincident.
|
---|
24 | **
|
---|
25 | ** The vectors v1 and v2 need not be unit vectors.
|
---|
26 | **
|
---|
27 | ** The routine slaBear performs an equivalent function except
|
---|
28 | ** that the points are specified in the form of spherical
|
---|
29 | ** coordinates.
|
---|
30 | **
|
---|
31 | ** Called: slaDpav
|
---|
32 | **
|
---|
33 | ** Last revision: 9 December 1996
|
---|
34 | **
|
---|
35 | ** Copyright P.T.Wallace. All rights reserved.
|
---|
36 | */
|
---|
37 | {
|
---|
38 | int i;
|
---|
39 | double d1 [ 3 ], d2 [ 3 ];
|
---|
40 |
|
---|
41 |
|
---|
42 | /* Call the double precision version. */
|
---|
43 | for ( i = 0; i < 3; i++ ) {
|
---|
44 | d1 [ i ] = (double) v1 [ i ];
|
---|
45 | d2 [ i ] = (double) v2 [ i ];
|
---|
46 | }
|
---|
47 | return (float) slaDpav ( d1, d2 );
|
---|
48 | }
|
---|
Note:
See
TracBrowser
for help on using the repository browser.