1 | #include "erfa.h"
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2 |
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3 | void eraPnm06a(double date1, double date2, double rnpb[3][3])
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4 | /*
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5 | ** - - - - - - - - - -
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6 | ** e r a P n m 0 6 a
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7 | ** - - - - - - - - - -
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8 | **
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9 | ** Form the matrix of precession-nutation for a given date (including
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10 | ** frame bias), IAU 2006 precession and IAU 2000A nutation models.
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11 | **
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12 | ** Given:
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13 | ** date1,date2 double TT as a 2-part Julian Date (Note 1)
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14 | **
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15 | ** Returned:
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16 | ** rnpb double[3][3] bias-precession-nutation matrix (Note 2)
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17 | **
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18 | ** Notes:
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19 | **
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20 | ** 1) The TT date date1+date2 is a Julian Date, apportioned in any
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21 | ** convenient way between the two arguments. For example,
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22 | ** JD(TT)=2450123.7 could be expressed in any of these ways,
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23 | ** among others:
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24 | **
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25 | ** date1 date2
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26 | **
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27 | ** 2450123.7 0.0 (JD method)
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28 | ** 2451545.0 -1421.3 (J2000 method)
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29 | ** 2400000.5 50123.2 (MJD method)
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30 | ** 2450123.5 0.2 (date & time method)
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31 | **
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32 | ** The JD method is the most natural and convenient to use in
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33 | ** cases where the loss of several decimal digits of resolution
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34 | ** is acceptable. The J2000 method is best matched to the way
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35 | ** the argument is handled internally and will deliver the
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36 | ** optimum resolution. The MJD method and the date & time methods
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37 | ** are both good compromises between resolution and convenience.
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38 | **
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39 | ** 2) The matrix operates in the sense V(date) = rnpb * V(GCRS), where
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40 | ** the p-vector V(date) is with respect to the true equatorial triad
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41 | ** of date date1+date2 and the p-vector V(GCRS) is with respect to
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42 | ** the Geocentric Celestial Reference System (IAU, 2000).
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43 | **
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44 | ** Called:
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45 | ** eraPfw06 bias-precession F-W angles, IAU 2006
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46 | ** eraNut06a nutation, IAU 2006/2000A
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47 | ** eraFw2m F-W angles to r-matrix
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48 | **
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49 | ** Reference:
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50 | **
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51 | ** Capitaine, N. & Wallace, P.T., 2006, Astron.Astrophys. 450, 855.
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52 | **
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53 | ** Copyright (C) 2013-2015, NumFOCUS Foundation.
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54 | ** Derived, with permission, from the SOFA library. See notes at end of file.
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55 | */
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56 | {
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57 | double gamb, phib, psib, epsa, dp, de;
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58 |
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59 | /* Fukushima-Williams angles for frame bias and precession. */
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60 | eraPfw06(date1, date2, &gamb, &phib, &psib, &epsa);
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61 |
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62 | /* Nutation components. */
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63 | eraNut06a(date1, date2, &dp, &de);
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64 |
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65 | /* Equinox based nutation x precession x bias matrix. */
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66 | eraFw2m(gamb, phib, psib + dp, epsa + de, rnpb);
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67 |
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68 | return;
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69 |
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70 | }
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71 | /*----------------------------------------------------------------------
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72 | **
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73 | **
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74 | ** Copyright (C) 2013-2015, NumFOCUS Foundation.
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75 | ** All rights reserved.
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76 | **
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77 | ** This library is derived, with permission, from the International
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78 | ** Astronomical Union's "Standards of Fundamental Astronomy" library,
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79 | ** available from http://www.iausofa.org.
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80 | **
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81 | ** The ERFA version is intended to retain identical functionality to
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82 | ** the SOFA library, but made distinct through different function and
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83 | ** file names, as set out in the SOFA license conditions. The SOFA
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84 | ** original has a role as a reference standard for the IAU and IERS,
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85 | ** and consequently redistribution is permitted only in its unaltered
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86 | ** state. The ERFA version is not subject to this restriction and
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87 | ** therefore can be included in distributions which do not support the
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88 | ** concept of "read only" software.
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89 | **
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90 | ** Although the intent is to replicate the SOFA API (other than
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91 | ** replacement of prefix names) and results (with the exception of
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92 | ** bugs; any that are discovered will be fixed), SOFA is not
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93 | ** responsible for any errors found in this version of the library.
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94 | **
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95 | ** If you wish to acknowledge the SOFA heritage, please acknowledge
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96 | ** that you are using a library derived from SOFA, rather than SOFA
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97 | ** itself.
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98 | **
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99 | **
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100 | ** TERMS AND CONDITIONS
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101 | **
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102 | ** Redistribution and use in source and binary forms, with or without
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103 | ** modification, are permitted provided that the following conditions
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104 | ** are met:
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105 | **
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106 | ** 1 Redistributions of source code must retain the above copyright
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107 | ** notice, this list of conditions and the following disclaimer.
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108 | **
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109 | ** 2 Redistributions in binary form must reproduce the above copyright
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110 | ** notice, this list of conditions and the following disclaimer in
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111 | ** the documentation and/or other materials provided with the
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112 | ** distribution.
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113 | **
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114 | ** 3 Neither the name of the Standards Of Fundamental Astronomy Board,
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115 | ** the International Astronomical Union nor the names of its
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116 | ** contributors may be used to endorse or promote products derived
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117 | ** from this software without specific prior written permission.
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118 | **
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119 | ** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
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120 | ** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
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121 | ** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
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122 | ** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE
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123 | ** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
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124 | ** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
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125 | ** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
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126 | ** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
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127 | ** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
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128 | ** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
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129 | ** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
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130 | ** POSSIBILITY OF SUCH DAMAGE.
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131 | **
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132 | */
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