source: branches/FACT++_part_filenames/pal/palPreces.c@ 19758

Last change on this file since 19758 was 18347, checked in by tbretz, 9 years ago
File size: 3.4 KB
Line 
1/*
2*+
3* Name:
4* palPreces
5
6* Purpose:
7* Precession - either FK4 or FK5 as required.
8
9* Language:
10* Starlink ANSI C
11
12* Type of Module:
13* Library routine
14
15* Invocation:
16* void palPreces ( const char sys[3], double ep0, double ep1,
17* double *ra, double *dc );
18
19* Arguments:
20* sys = const char [3] (Given)
21* Precession to be applied: FK4 or FK5. Case insensitive.
22* ep0 = double (Given)
23* Starting epoch.
24* ep1 = double (Given)
25* Ending epoch
26* ra = double * (Given & Returned)
27* On input the RA mean equator & equinox at epoch ep0. On exit
28* the RA mean equator & equinox of epoch ep1.
29* dec = double * (Given & Returned)
30* On input the dec mean equator & equinox at epoch ep0. On exit
31* the dec mean equator & equinox of epoch ep1.
32
33* Description:
34* Precess coordinates using the appropriate system and epochs.
35
36* Authors:
37* PTW: Patrick T. Wallace
38* TIMJ: Tim Jenness (JAC, Hawaii)
39* {enter_new_authors_here}
40
41* Notes:
42* - Uses palPrec for FK5 data and palPrebn for FK4 data.
43* - The epochs are Besselian if SYSTEM='FK4' and Julian if 'FK5'.
44* For example, to precess coordinates in the old system from
45* equinox 1900.0 to 1950.0 the call would be:
46* palPreces( "FK4", 1900.0, 1950.0, &ra, &dc );
47* - This routine will NOT correctly convert between the old and
48* the new systems - for example conversion from B1950 to J2000.
49* For these purposes see palFk425, palFk524, palFk45z and
50* palFk54z.
51* - If an invalid SYSTEM is supplied, values of -99D0,-99D0 will
52* be returned for both RA and DC.
53
54* History:
55* 2012-03-02 (TIMJ):
56* Initial version
57* Adapted with permission from the Fortran SLALIB library.
58* {enter_further_changes_here}
59
60* Copyright:
61* Copyright (C) 1995 Rutherford Appleton Laboratory
62* Copyright (C) 2012 Science and Technology Facilities Council.
63* All Rights Reserved.
64
65* Licence:
66* This program is free software; you can redistribute it and/or
67* modify it under the terms of the GNU General Public License as
68* published by the Free Software Foundation; either version 3 of
69* the License, or (at your option) any later version.
70*
71* This program is distributed in the hope that it will be
72* useful, but WITHOUT ANY WARRANTY; without even the implied
73* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
74* PURPOSE. See the GNU General Public License for more details.
75*
76* You should have received a copy of the GNU General Public License
77* along with this program; if not, write to the Free Software
78* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston,
79* MA 02110-1301, USA.
80
81* Bugs:
82* {note_any_bugs_here}
83*-
84*/
85
86#include "pal.h"
87#include "pal1sofa.h"
88
89#include <string.h>
90
91void palPreces ( const char sys[3], double ep0, double ep1,
92 double *ra, double *dc ) {
93
94 double pm[3][3];
95 double v1[3];
96 double v2[3];
97
98 /* Generate appropriate precession matrix */
99 if ( strncasecmp( "FK4", sys, 3 ) == 0 ) {
100 palPrebn( ep0, ep1, pm );
101 } else if (strncasecmp( "FK5", sys, 3 ) == 0 ) {
102 palPrec( ep0, ep1, pm );
103 } else {
104 *ra = -99.0;
105 *dc = -99.0;
106 return;
107 }
108
109 /* Convert RA,Dec to x,y,z */
110 eraS2c( *ra, *dc, v1 );
111
112 /* Precess */
113 eraRxp( pm, v1, v2 );
114
115 /* Back to RA,Dec */
116 eraC2s( v2, ra, dc );
117 *ra = eraAnp( *ra );
118}
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