1 #include "erfa.h"
2 
eraPnm00a(double date1,double date2,double rbpn[3][3])3 void eraPnm00a(double date1, double date2, double rbpn[3][3])
4 /*
5 **  - - - - - - - - - -
6 **   e r a P n m 0 0 a
7 **  - - - - - - - - - -
8 **
9 **  Form the matrix of precession-nutation for a given date (including
10 **  frame bias), equinox-based, IAU 2000A model.
11 **
12 **  Given:
13 **     date1,date2  double     TT as a 2-part Julian Date (Note 1)
14 **
15 **  Returned:
16 **     rbpn         double[3][3]    classical NPB matrix (Note 2)
17 **
18 **  Notes:
19 **
20 **  1) The TT date date1+date2 is a Julian Date, apportioned in any
21 **     convenient way between the two arguments.  For example,
22 **     JD(TT)=2450123.7 could be expressed in any of these ways,
23 **     among others:
24 **
25 **            date1          date2
26 **
27 **         2450123.7           0.0       (JD method)
28 **         2451545.0       -1421.3       (J2000 method)
29 **         2400000.5       50123.2       (MJD method)
30 **         2450123.5           0.2       (date & time method)
31 **
32 **     The JD method is the most natural and convenient to use in
33 **     cases where the loss of several decimal digits of resolution
34 **     is acceptable.  The J2000 method is best matched to the way
35 **     the argument is handled internally and will deliver the
36 **     optimum resolution.  The MJD method and the date & time methods
37 **     are both good compromises between resolution and convenience.
38 **
39 **  2) The matrix operates in the sense V(date) = rbpn * V(GCRS), where
40 **     the p-vector V(date) is with respect to the true equatorial triad
41 **     of date date1+date2 and the p-vector V(GCRS) is with respect to
42 **     the Geocentric Celestial Reference System (IAU, 2000).
43 **
44 **  3) A faster, but slightly less accurate result (about 1 mas), can be
45 **     obtained by using instead the eraPnm00b function.
46 **
47 **  Called:
48 **     eraPn00a     bias/precession/nutation, IAU 2000A
49 **
50 **  Reference:
51 **
52 **     IAU: Trans. International Astronomical Union, Vol. XXIVB;  Proc.
53 **     24th General Assembly, Manchester, UK.  Resolutions B1.3, B1.6.
54 **     (2000)
55 **
56 **  Copyright (C) 2013-2020, NumFOCUS Foundation.
57 **  Derived, with permission, from the SOFA library.  See notes at end of file.
58 */
59 {
60    double dpsi, deps, epsa, rb[3][3], rp[3][3], rbp[3][3], rn[3][3];
61 
62 
63 /* Obtain the required matrix (discarding other results). */
64    eraPn00a(date1, date2, &dpsi, &deps, &epsa, rb, rp, rbp, rn, rbpn);
65 
66    return;
67 
68 }
69 /*----------------------------------------------------------------------
70 **
71 **
72 **  Copyright (C) 2013-2020, NumFOCUS Foundation.
73 **  All rights reserved.
74 **
75 **  This library is derived, with permission, from the International
76 **  Astronomical Union's "Standards of Fundamental Astronomy" library,
77 **  available from http://www.iausofa.org.
78 **
79 **  The ERFA version is intended to retain identical functionality to
80 **  the SOFA library, but made distinct through different function and
81 **  file names, as set out in the SOFA license conditions.  The SOFA
82 **  original has a role as a reference standard for the IAU and IERS,
83 **  and consequently redistribution is permitted only in its unaltered
84 **  state.  The ERFA version is not subject to this restriction and
85 **  therefore can be included in distributions which do not support the
86 **  concept of "read only" software.
87 **
88 **  Although the intent is to replicate the SOFA API (other than
89 **  replacement of prefix names) and results (with the exception of
90 **  bugs;  any that are discovered will be fixed), SOFA is not
91 **  responsible for any errors found in this version of the library.
92 **
93 **  If you wish to acknowledge the SOFA heritage, please acknowledge
94 **  that you are using a library derived from SOFA, rather than SOFA
95 **  itself.
96 **
97 **
98 **  TERMS AND CONDITIONS
99 **
100 **  Redistribution and use in source and binary forms, with or without
101 **  modification, are permitted provided that the following conditions
102 **  are met:
103 **
104 **  1 Redistributions of source code must retain the above copyright
105 **    notice, this list of conditions and the following disclaimer.
106 **
107 **  2 Redistributions in binary form must reproduce the above copyright
108 **    notice, this list of conditions and the following disclaimer in
109 **    the documentation and/or other materials provided with the
110 **    distribution.
111 **
112 **  3 Neither the name of the Standards Of Fundamental Astronomy Board,
113 **    the International Astronomical Union nor the names of its
114 **    contributors may be used to endorse or promote products derived
115 **    from this software without specific prior written permission.
116 **
117 **  THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
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131