source: branches/FACT++_lidctrl_usb/erfa/src/pmpx.c@ 19875

Last change on this file since 19875 was 18711, checked in by tbretz, 10 years ago
Updated to ERFA 1.3.0 (no relevant code change except the leap second at the beginning of 2017)
File size: 5.5 KB
Line 
1#include "erfa.h"
2
3void eraPmpx(double rc, double dc, double pr, double pd,
4 double px, double rv, double pmt, double pob[3],
5 double pco[3])
6/*
7** - - - - - - - -
8** e r a P m p x
9** - - - - - - - -
10**
11** Proper motion and parallax.
12**
13** Given:
14** rc,dc double ICRS RA,Dec at catalog epoch (radians)
15** pr double RA proper motion (radians/year; Note 1)
16** pd double Dec proper motion (radians/year)
17** px double parallax (arcsec)
18** rv double radial velocity (km/s, +ve if receding)
19** pmt double proper motion time interval (SSB, Julian years)
20** pob double[3] SSB to observer vector (au)
21**
22** Returned:
23** pco double[3] coordinate direction (BCRS unit vector)
24**
25** Notes:
26**
27** 1) The proper motion in RA is dRA/dt rather than cos(Dec)*dRA/dt.
28**
29** 2) The proper motion time interval is for when the starlight
30** reaches the solar system barycenter.
31**
32** 3) To avoid the need for iteration, the Roemer effect (i.e. the
33** small annual modulation of the proper motion coming from the
34** changing light time) is applied approximately, using the
35** direction of the star at the catalog epoch.
36**
37** References:
38**
39** 1984 Astronomical Almanac, pp B39-B41.
40**
41** Urban, S. & Seidelmann, P. K. (eds), Explanatory Supplement to
42** the Astronomical Almanac, 3rd ed., University Science Books
43** (2013), Section 7.2.
44**
45** Called:
46** eraPdp scalar product of two p-vectors
47** eraPn decompose p-vector into modulus and direction
48**
49** Copyright (C) 2013-2016, NumFOCUS Foundation.
50** Derived, with permission, from the SOFA library. See notes at end of file.
51*/
52{
53/* Km/s to au/year */
54 const double VF = ERFA_DAYSEC*ERFA_DJM/ERFA_DAU;
55
56/* Light time for 1 au, Julian years */
57 const double AULTY = ERFA_AULT/ERFA_DAYSEC/ERFA_DJY;
58
59 int i;
60 double sr, cr, sd, cd, x, y, z, p[3], dt, pxr, w, pdz, pm[3];
61
62
63/* Spherical coordinates to unit vector (and useful functions). */
64 sr = sin(rc);
65 cr = cos(rc);
66 sd = sin(dc);
67 cd = cos(dc);
68 p[0] = x = cr*cd;
69 p[1] = y = sr*cd;
70 p[2] = z = sd;
71
72/* Proper motion time interval (y) including Roemer effect. */
73 dt = pmt + eraPdp(p,pob)*AULTY;
74
75/* Space motion (radians per year). */
76 pxr = px * ERFA_DAS2R;
77 w = VF * rv * pxr;
78 pdz = pd * z;
79 pm[0] = - pr*y - pdz*cr + w*x;
80 pm[1] = pr*x - pdz*sr + w*y;
81 pm[2] = pd*cd + w*z;
82
83/* Coordinate direction of star (unit vector, BCRS). */
84 for (i = 0; i < 3; i++) {
85 p[i] += dt*pm[i] - pxr*pob[i];
86 }
87 eraPn(p, &w, pco);
88
89/* Finished. */
90
91}
92/*----------------------------------------------------------------------
93**
94**
95** Copyright (C) 2013-2016, NumFOCUS Foundation.
96** All rights reserved.
97**
98** This library is derived, with permission, from the International
99** Astronomical Union's "Standards of Fundamental Astronomy" library,
100** available from http://www.iausofa.org.
101**
102** The ERFA version is intended to retain identical functionality to
103** the SOFA library, but made distinct through different function and
104** file names, as set out in the SOFA license conditions. The SOFA
105** original has a role as a reference standard for the IAU and IERS,
106** and consequently redistribution is permitted only in its unaltered
107** state. The ERFA version is not subject to this restriction and
108** therefore can be included in distributions which do not support the
109** concept of "read only" software.
110**
111** Although the intent is to replicate the SOFA API (other than
112** replacement of prefix names) and results (with the exception of
113** bugs; any that are discovered will be fixed), SOFA is not
114** responsible for any errors found in this version of the library.
115**
116** If you wish to acknowledge the SOFA heritage, please acknowledge
117** that you are using a library derived from SOFA, rather than SOFA
118** itself.
119**
120**
121** TERMS AND CONDITIONS
122**
123** Redistribution and use in source and binary forms, with or without
124** modification, are permitted provided that the following conditions
125** are met:
126**
127** 1 Redistributions of source code must retain the above copyright
128** notice, this list of conditions and the following disclaimer.
129**
130** 2 Redistributions in binary form must reproduce the above copyright
131** notice, this list of conditions and the following disclaimer in
132** the documentation and/or other materials provided with the
133** distribution.
134**
135** 3 Neither the name of the Standards Of Fundamental Astronomy Board,
136** the International Astronomical Union nor the names of its
137** contributors may be used to endorse or promote products derived
138** from this software without specific prior written permission.
139**
140** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
141** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
142** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
143** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE
144** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
145** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
146** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
147** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
148** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
149** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
150** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
151** POSSIBILITY OF SUCH DAMAGE.
152**
153*/
Note: See TracBrowser for help on using the repository browser.