1 #include "erfa.h"
2 
eraNum06a(double date1,double date2,double rmatn[3][3])3 void eraNum06a(double date1, double date2, double rmatn[3][3])
4 /*
5 **  - - - - - - - - - -
6 **   e r a N u m 0 6 a
7 **  - - - - - - - - - -
8 **
9 **  Form the matrix of nutation for a given date, IAU 2006/2000A model.
10 **
11 **  Given:
12 **     date1,date2   double          TT as a 2-part Julian Date (Note 1)
13 **
14 **  Returned:
15 **     rmatn         double[3][3]    nutation matrix
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(true) = rmatn * V(mean), where
39 **     the p-vector V(true) is with respect to the true equatorial triad
40 **     of date and the p-vector V(mean) is with respect to the mean
41 **     equatorial triad of date.
42 **
43 **  Called:
44 **     eraObl06     mean obliquity, IAU 2006
45 **     eraNut06a    nutation, IAU 2006/2000A
46 **     eraNumat     form nutation matrix
47 **
48 **  Reference:
49 **
50 **     Explanatory Supplement to the Astronomical Almanac,
51 **     P. Kenneth Seidelmann (ed), University Science Books (1992),
52 **     Section 3.222-3 (p114).
53 **
54 **  This revision:  2021 May 11
55 **
56 **  Copyright (C) 2013-2021, NumFOCUS Foundation.
57 **  Derived, with permission, from the SOFA library.  See notes at end of file.
58 */
59 {
60    double eps, dp, de;
61 
62 
63 /* Mean obliquity. */
64    eps = eraObl06(date1, date2);
65 
66 /* Nutation components. */
67    eraNut06a(date1, date2, &dp, &de);
68 
69 /* Nutation matrix. */
70    eraNumat(eps, dp, de, rmatn);
71 
72 /* Finished. */
73 
74 }
75 /*----------------------------------------------------------------------
76 **
77 **
78 **  Copyright (C) 2013-2021, NumFOCUS Foundation.
79 **  All rights reserved.
80 **
81 **  This library is derived, with permission, from the International
82 **  Astronomical Union's "Standards of Fundamental Astronomy" library,
83 **  available from http://www.iausofa.org.
84 **
85 **  The ERFA version is intended to retain identical functionality to
86 **  the SOFA library, but made distinct through different function and
87 **  file names, as set out in the SOFA license conditions.  The SOFA
88 **  original has a role as a reference standard for the IAU and IERS,
89 **  and consequently redistribution is permitted only in its unaltered
90 **  state.  The ERFA version is not subject to this restriction and
91 **  therefore can be included in distributions which do not support the
92 **  concept of "read only" software.
93 **
94 **  Although the intent is to replicate the SOFA API (other than
95 **  replacement of prefix names) and results (with the exception of
96 **  bugs;  any that are discovered will be fixed), SOFA is not
97 **  responsible for any errors found in this version of the library.
98 **
99 **  If you wish to acknowledge the SOFA heritage, please acknowledge
100 **  that you are using a library derived from SOFA, rather than SOFA
101 **  itself.
102 **
103 **
104 **  TERMS AND CONDITIONS
105 **
106 **  Redistribution and use in source and binary forms, with or without
107 **  modification, are permitted provided that the following conditions
108 **  are met:
109 **
110 **  1 Redistributions of source code must retain the above copyright
111 **    notice, this list of conditions and the following disclaimer.
112 **
113 **  2 Redistributions in binary form must reproduce the above copyright
114 **    notice, this list of conditions and the following disclaimer in
115 **    the documentation and/or other materials provided with the
116 **    distribution.
117 **
118 **  3 Neither the name of the Standards Of Fundamental Astronomy Board,
119 **    the International Astronomical Union nor the names of its
120 **    contributors may be used to endorse or promote products derived
121 **    from this software without specific prior written permission.
122 **
123 **  THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
124 **  "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
125 **  LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
126 **  FOR A PARTICULAR PURPOSE ARE DISCLAIMED.  IN NO EVENT SHALL THE
127 **  COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
128 **  INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
129 **  BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
130 **  LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
131 **  CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
132 **  LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
133 **  ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
134 **  POSSIBILITY OF SUCH DAMAGE.
135 **
136 */
137