1 | /*
|
---|
2 | *+
|
---|
3 | * Name:
|
---|
4 | * palMap
|
---|
5 |
|
---|
6 | * Purpose:
|
---|
7 | * Convert star RA,Dec from mean place to geocentric apparent
|
---|
8 |
|
---|
9 | * Language:
|
---|
10 | * Starlink ANSI C
|
---|
11 |
|
---|
12 | * Type of Module:
|
---|
13 | * Library routine
|
---|
14 |
|
---|
15 | * Invocation:
|
---|
16 | * void palMap( double rm, double dm, double pr, double pd,
|
---|
17 | * double px, double rv, double eq, double date,
|
---|
18 | * double *ra, double *da );
|
---|
19 |
|
---|
20 | * Arguments:
|
---|
21 | * rm = double (Given)
|
---|
22 | * Mean RA (radians)
|
---|
23 | * dm = double (Given)
|
---|
24 | * Mean declination (radians)
|
---|
25 | * pr = double (Given)
|
---|
26 | * RA proper motion, changes per Julian year (radians)
|
---|
27 | * pd = double (Given)
|
---|
28 | * Dec proper motion, changes per Julian year (radians)
|
---|
29 | * px = double (Given)
|
---|
30 | * Parallax (arcsec)
|
---|
31 | * rv = double (Given)
|
---|
32 | * Radial velocity (km/s, +ve if receding)
|
---|
33 | * eq = double (Given)
|
---|
34 | * Epoch and equinox of star data (Julian)
|
---|
35 | * date = double (Given)
|
---|
36 | * TDB for apparent place (JD-2400000.5)
|
---|
37 | * ra = double * (Returned)
|
---|
38 | * Apparent RA (radians)
|
---|
39 | * dec = double * (Returned)
|
---|
40 | * Apparent dec (radians)
|
---|
41 |
|
---|
42 | * Description:
|
---|
43 | * Convert star RA,Dec from mean place to geocentric apparent.
|
---|
44 |
|
---|
45 | * Authors:
|
---|
46 | * PTW: Patrick T. Wallace
|
---|
47 | * TIMJ: Tim Jenness (JAC, Hawaii)
|
---|
48 | * {enter_new_authors_here}
|
---|
49 |
|
---|
50 | * Notes:
|
---|
51 | * - Calls palMappa and palMapqk
|
---|
52 |
|
---|
53 | * - The reference systems and timescales used are IAU 2006.
|
---|
54 |
|
---|
55 | * - EQ is the Julian epoch specifying both the reference frame and
|
---|
56 | * the epoch of the position - usually 2000. For positions where
|
---|
57 | * the epoch and equinox are different, use the routine palPm to
|
---|
58 | * apply proper motion corrections before using this routine.
|
---|
59 | *
|
---|
60 | * - The distinction between the required TDB and TT is always
|
---|
61 | * negligible. Moreover, for all but the most critical
|
---|
62 | * applications UTC is adequate.
|
---|
63 | *
|
---|
64 | * - The proper motions in RA are dRA/dt rather than cos(Dec)*dRA/dt.
|
---|
65 | *
|
---|
66 | * - This routine may be wasteful for some applications because it
|
---|
67 | * recomputes the Earth position/velocity and the precession-
|
---|
68 | * nutation matrix each time, and because it allows for parallax
|
---|
69 | * and proper motion. Where multiple transformations are to be
|
---|
70 | * carried out for one epoch, a faster method is to call the
|
---|
71 | * palMappa routine once and then either the palMapqk routine
|
---|
72 | * (which includes parallax and proper motion) or palMapqkz (which
|
---|
73 | * assumes zero parallax and proper motion).
|
---|
74 | *
|
---|
75 | * - The accuracy is sub-milliarcsecond, limited by the
|
---|
76 | * precession-nutation model (see palPrenut for details).
|
---|
77 | *
|
---|
78 | * - The accuracy is further limited by the routine palEvp, called
|
---|
79 | * by palMappa, which computes the Earth position and velocity.
|
---|
80 | * See eraEpv00 for details on that calculation.
|
---|
81 |
|
---|
82 | * History:
|
---|
83 | * 2012-03-01 (TIMJ):
|
---|
84 | * Initial version
|
---|
85 | * Adapted with permission from the Fortran SLALIB library.
|
---|
86 | * {enter_further_changes_here}
|
---|
87 |
|
---|
88 | * Copyright:
|
---|
89 | * Copyright (C) 2001 Rutherford Appleton Laboratory
|
---|
90 | * Copyright (C) 2012 Science and Technology Facilities Council.
|
---|
91 | * All Rights Reserved.
|
---|
92 |
|
---|
93 | * Licence:
|
---|
94 | * This program is free software; you can redistribute it and/or
|
---|
95 | * modify it under the terms of the GNU General Public License as
|
---|
96 | * published by the Free Software Foundation; either version 3 of
|
---|
97 | * the License, or (at your option) any later version.
|
---|
98 | *
|
---|
99 | * This program is distributed in the hope that it will be
|
---|
100 | * useful, but WITHOUT ANY WARRANTY; without even the implied
|
---|
101 | * warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
|
---|
102 | * PURPOSE. See the GNU General Public License for more details.
|
---|
103 | *
|
---|
104 | * You should have received a copy of the GNU General Public License
|
---|
105 | * along with this program; if not, write to the Free Software
|
---|
106 | * Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
|
---|
107 | * USA.
|
---|
108 |
|
---|
109 | * Bugs:
|
---|
110 | * {note_any_bugs_here}
|
---|
111 | *-
|
---|
112 | */
|
---|
113 |
|
---|
114 | #include "pal.h"
|
---|
115 |
|
---|
116 | void palMap( double rm, double dm, double pr, double pd,
|
---|
117 | double px, double rv, double eq, double date,
|
---|
118 | double *ra, double *da ) {
|
---|
119 |
|
---|
120 | double amprms[21];
|
---|
121 |
|
---|
122 | /* Star independent parameters */
|
---|
123 | palMappa( eq, date, amprms );
|
---|
124 |
|
---|
125 | /* Mean to apparent */
|
---|
126 | palMapqk( rm, dm, pr, pd, px, rv, amprms, ra, da );
|
---|
127 |
|
---|
128 | }
|
---|