1 | #include "erfa.h"
|
---|
2 |
|
---|
3 | void eraPmat76(double date1, double date2, double rmatp[3][3])
|
---|
4 | /*
|
---|
5 | ** - - - - - - - - - -
|
---|
6 | ** e r a P m a t 7 6
|
---|
7 | ** - - - - - - - - - -
|
---|
8 | **
|
---|
9 | ** Precession matrix from J2000.0 to a specified date, IAU 1976 model.
|
---|
10 | **
|
---|
11 | ** Given:
|
---|
12 | ** date1,date2 double ending date, TT (Note 1)
|
---|
13 | **
|
---|
14 | ** Returned:
|
---|
15 | ** rmatp double[3][3] precession matrix, J2000.0 -> date1+date2
|
---|
16 | **
|
---|
17 | ** Notes:
|
---|
18 | **
|
---|
19 | ** 1) The TT date date1+date2 is a Julian Date, apportioned in any
|
---|
20 | ** convenient way between the two arguments. For example,
|
---|
21 | ** JD(TT)=2450123.7 could be expressed in any of these ways,
|
---|
22 | ** among others:
|
---|
23 | **
|
---|
24 | ** date1 date2
|
---|
25 | **
|
---|
26 | ** 2450123.7 0.0 (JD method)
|
---|
27 | ** 2451545.0 -1421.3 (J2000 method)
|
---|
28 | ** 2400000.5 50123.2 (MJD method)
|
---|
29 | ** 2450123.5 0.2 (date & time method)
|
---|
30 | **
|
---|
31 | ** The JD method is the most natural and convenient to use in
|
---|
32 | ** cases where the loss of several decimal digits of resolution
|
---|
33 | ** is acceptable. The J2000 method is best matched to the way
|
---|
34 | ** the argument is handled internally and will deliver the
|
---|
35 | ** optimum resolution. The MJD method and the date & time methods
|
---|
36 | ** are both good compromises between resolution and convenience.
|
---|
37 | **
|
---|
38 | ** 2) The matrix operates in the sense V(date) = RMATP * V(J2000),
|
---|
39 | ** where the p-vector V(J2000) is with respect to the mean
|
---|
40 | ** equatorial triad of epoch J2000.0 and the p-vector V(date)
|
---|
41 | ** is with respect to the mean equatorial triad of the given
|
---|
42 | ** date.
|
---|
43 | **
|
---|
44 | ** 3) Though the matrix method itself is rigorous, the precession
|
---|
45 | ** angles are expressed through canonical polynomials which are
|
---|
46 | ** valid only for a limited time span. In addition, the IAU 1976
|
---|
47 | ** precession rate is known to be imperfect. The absolute accuracy
|
---|
48 | ** of the present formulation is better than 0.1 arcsec from
|
---|
49 | ** 1960AD to 2040AD, better than 1 arcsec from 1640AD to 2360AD,
|
---|
50 | ** and remains below 3 arcsec for the whole of the period
|
---|
51 | ** 500BC to 3000AD. The errors exceed 10 arcsec outside the
|
---|
52 | ** range 1200BC to 3900AD, exceed 100 arcsec outside 4200BC to
|
---|
53 | ** 5600AD and exceed 1000 arcsec outside 6800BC to 8200AD.
|
---|
54 | **
|
---|
55 | ** Called:
|
---|
56 | ** eraPrec76 accumulated precession angles, IAU 1976
|
---|
57 | ** eraIr initialize r-matrix to identity
|
---|
58 | ** eraRz rotate around Z-axis
|
---|
59 | ** eraRy rotate around Y-axis
|
---|
60 | ** eraCr copy r-matrix
|
---|
61 | **
|
---|
62 | ** References:
|
---|
63 | **
|
---|
64 | ** Lieske, J.H., 1979, Astron.Astrophys. 73, 282.
|
---|
65 | ** equations (6) & (7), p283.
|
---|
66 | **
|
---|
67 | ** Kaplan,G.H., 1981. USNO circular no. 163, pA2.
|
---|
68 | **
|
---|
69 | ** Copyright (C) 2013-2015, NumFOCUS Foundation.
|
---|
70 | ** Derived, with permission, from the SOFA library. See notes at end of file.
|
---|
71 | */
|
---|
72 | {
|
---|
73 | double zeta, z, theta, wmat[3][3];
|
---|
74 |
|
---|
75 | /* Precession Euler angles, J2000.0 to specified date. */
|
---|
76 | eraPrec76(ERFA_DJ00, 0.0, date1, date2, &zeta, &z, &theta);
|
---|
77 |
|
---|
78 | /* Form the rotation matrix. */
|
---|
79 | eraIr( wmat);
|
---|
80 | eraRz( -zeta, wmat);
|
---|
81 | eraRy( theta, wmat);
|
---|
82 | eraRz( -z, wmat);
|
---|
83 | eraCr( wmat, rmatp);
|
---|
84 |
|
---|
85 | return;
|
---|
86 |
|
---|
87 | }
|
---|
88 | /*----------------------------------------------------------------------
|
---|
89 | **
|
---|
90 | **
|
---|
91 | ** Copyright (C) 2013-2015, NumFOCUS Foundation.
|
---|
92 | ** All rights reserved.
|
---|
93 | **
|
---|
94 | ** This library is derived, with permission, from the International
|
---|
95 | ** Astronomical Union's "Standards of Fundamental Astronomy" library,
|
---|
96 | ** available from http://www.iausofa.org.
|
---|
97 | **
|
---|
98 | ** The ERFA version is intended to retain identical functionality to
|
---|
99 | ** the SOFA library, but made distinct through different function and
|
---|
100 | ** file names, as set out in the SOFA license conditions. The SOFA
|
---|
101 | ** original has a role as a reference standard for the IAU and IERS,
|
---|
102 | ** and consequently redistribution is permitted only in its unaltered
|
---|
103 | ** state. The ERFA version is not subject to this restriction and
|
---|
104 | ** therefore can be included in distributions which do not support the
|
---|
105 | ** concept of "read only" software.
|
---|
106 | **
|
---|
107 | ** Although the intent is to replicate the SOFA API (other than
|
---|
108 | ** replacement of prefix names) and results (with the exception of
|
---|
109 | ** bugs; any that are discovered will be fixed), SOFA is not
|
---|
110 | ** responsible for any errors found in this version of the library.
|
---|
111 | **
|
---|
112 | ** If you wish to acknowledge the SOFA heritage, please acknowledge
|
---|
113 | ** that you are using a library derived from SOFA, rather than SOFA
|
---|
114 | ** itself.
|
---|
115 | **
|
---|
116 | **
|
---|
117 | ** TERMS AND CONDITIONS
|
---|
118 | **
|
---|
119 | ** Redistribution and use in source and binary forms, with or without
|
---|
120 | ** modification, are permitted provided that the following conditions
|
---|
121 | ** are met:
|
---|
122 | **
|
---|
123 | ** 1 Redistributions of source code must retain the above copyright
|
---|
124 | ** notice, this list of conditions and the following disclaimer.
|
---|
125 | **
|
---|
126 | ** 2 Redistributions in binary form must reproduce the above copyright
|
---|
127 | ** notice, this list of conditions and the following disclaimer in
|
---|
128 | ** the documentation and/or other materials provided with the
|
---|
129 | ** distribution.
|
---|
130 | **
|
---|
131 | ** 3 Neither the name of the Standards Of Fundamental Astronomy Board,
|
---|
132 | ** the International Astronomical Union nor the names of its
|
---|
133 | ** contributors may be used to endorse or promote products derived
|
---|
134 | ** from this software without specific prior written permission.
|
---|
135 | **
|
---|
136 | ** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
|
---|
137 | ** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
|
---|
138 | ** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
|
---|
139 | ** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE
|
---|
140 | ** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
|
---|
141 | ** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
|
---|
142 | ** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
|
---|
143 | ** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
|
---|
144 | ** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
|
---|
145 | ** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
|
---|
146 | ** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
|
---|
147 | ** POSSIBILITY OF SUCH DAMAGE.
|
---|
148 | **
|
---|
149 | */
|
---|