1 | #include "erfa.h"
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2 |
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3 | void eraPfw06(double date1, double date2,
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4 | double *gamb, double *phib, double *psib, double *epsa)
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5 | /*
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6 | ** - - - - - - - - -
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7 | ** e r a P f w 0 6
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8 | ** - - - - - - - - -
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9 | **
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10 | ** Precession angles, IAU 2006 (Fukushima-Williams 4-angle formulation).
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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 | ** gamb double F-W angle gamma_bar (radians)
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17 | ** phib double F-W angle phi_bar (radians)
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18 | ** psib double F-W angle psi_bar (radians)
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19 | ** epsa double F-W angle epsilon_A (radians)
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20 | **
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21 | ** Notes:
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22 | **
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23 | ** 1) The TT date date1+date2 is a Julian Date, apportioned in any
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24 | ** convenient way between the two arguments. For example,
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25 | ** JD(TT)=2450123.7 could be expressed in any of these ways,
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26 | ** among others:
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27 | **
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28 | ** date1 date2
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29 | **
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30 | ** 2450123.7 0.0 (JD method)
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31 | ** 2451545.0 -1421.3 (J2000 method)
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32 | ** 2400000.5 50123.2 (MJD method)
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33 | ** 2450123.5 0.2 (date & time method)
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34 | **
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35 | ** The JD method is the most natural and convenient to use in
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36 | ** cases where the loss of several decimal digits of resolution
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37 | ** is acceptable. The J2000 method is best matched to the way
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38 | ** the argument is handled internally and will deliver the
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39 | ** optimum resolution. The MJD method and the date & time methods
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40 | ** are both good compromises between resolution and convenience.
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41 | **
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42 | ** 2) Naming the following points:
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43 | **
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44 | ** e = J2000.0 ecliptic pole,
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45 | ** p = GCRS pole,
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46 | ** E = mean ecliptic pole of date,
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47 | ** and P = mean pole of date,
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48 | **
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49 | ** the four Fukushima-Williams angles are as follows:
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50 | **
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51 | ** gamb = gamma_bar = epE
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52 | ** phib = phi_bar = pE
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53 | ** psib = psi_bar = pEP
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54 | ** epsa = epsilon_A = EP
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55 | **
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56 | ** 3) The matrix representing the combined effects of frame bias and
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57 | ** precession is:
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58 | **
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59 | ** PxB = R_1(-epsa).R_3(-psib).R_1(phib).R_3(gamb)
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60 | **
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61 | ** 4) The matrix representing the combined effects of frame bias,
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62 | ** precession and nutation is simply:
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63 | **
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64 | ** NxPxB = R_1(-epsa-dE).R_3(-psib-dP).R_1(phib).R_3(gamb)
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65 | **
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66 | ** where dP and dE are the nutation components with respect to the
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67 | ** ecliptic of date.
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68 | **
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69 | ** Reference:
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70 | **
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71 | ** Hilton, J. et al., 2006, Celest.Mech.Dyn.Astron. 94, 351
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72 | **
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73 | ** Called:
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74 | ** eraObl06 mean obliquity, IAU 2006
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75 | **
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76 | ** Copyright (C) 2013-2017, NumFOCUS Foundation.
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77 | ** Derived, with permission, from the SOFA library. See notes at end of file.
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78 | */
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79 | {
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80 | double t;
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81 |
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82 |
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83 | /* Interval between fundamental date J2000.0 and given date (JC). */
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84 | t = ((date1 - ERFA_DJ00) + date2) / ERFA_DJC;
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85 |
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86 | /* P03 bias+precession angles. */
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87 | *gamb = ( -0.052928 +
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88 | ( 10.556378 +
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89 | ( 0.4932044 +
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90 | ( -0.00031238 +
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91 | ( -0.000002788 +
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92 | ( 0.0000000260 )
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93 | * t) * t) * t) * t) * t) * ERFA_DAS2R;
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94 | *phib = ( 84381.412819 +
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95 | ( -46.811016 +
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96 | ( 0.0511268 +
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97 | ( 0.00053289 +
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98 | ( -0.000000440 +
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99 | ( -0.0000000176 )
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100 | * t) * t) * t) * t) * t) * ERFA_DAS2R;
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101 | *psib = ( -0.041775 +
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102 | ( 5038.481484 +
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103 | ( 1.5584175 +
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104 | ( -0.00018522 +
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105 | ( -0.000026452 +
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106 | ( -0.0000000148 )
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107 | * t) * t) * t) * t) * t) * ERFA_DAS2R;
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108 | *epsa = eraObl06(date1, date2);
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109 |
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110 | return;
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111 |
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112 | }
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113 | /*----------------------------------------------------------------------
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114 | **
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115 | **
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116 | ** Copyright (C) 2013-2017, NumFOCUS Foundation.
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117 | ** All rights reserved.
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118 | **
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119 | ** This library is derived, with permission, from the International
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120 | ** Astronomical Union's "Standards of Fundamental Astronomy" library,
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121 | ** available from http://www.iausofa.org.
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122 | **
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123 | ** The ERFA version is intended to retain identical functionality to
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124 | ** the SOFA library, but made distinct through different function and
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125 | ** file names, as set out in the SOFA license conditions. The SOFA
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126 | ** original has a role as a reference standard for the IAU and IERS,
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127 | ** and consequently redistribution is permitted only in its unaltered
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128 | ** state. The ERFA version is not subject to this restriction and
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129 | ** therefore can be included in distributions which do not support the
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130 | ** concept of "read only" software.
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131 | **
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132 | ** Although the intent is to replicate the SOFA API (other than
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133 | ** replacement of prefix names) and results (with the exception of
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134 | ** bugs; any that are discovered will be fixed), SOFA is not
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135 | ** responsible for any errors found in this version of the library.
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136 | **
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137 | ** If you wish to acknowledge the SOFA heritage, please acknowledge
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138 | ** that you are using a library derived from SOFA, rather than SOFA
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139 | ** itself.
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140 | **
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141 | **
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142 | ** TERMS AND CONDITIONS
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143 | **
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144 | ** Redistribution and use in source and binary forms, with or without
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145 | ** modification, are permitted provided that the following conditions
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146 | ** are met:
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147 | **
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148 | ** 1 Redistributions of source code must retain the above copyright
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149 | ** notice, this list of conditions and the following disclaimer.
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150 | **
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151 | ** 2 Redistributions in binary form must reproduce the above copyright
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152 | ** notice, this list of conditions and the following disclaimer in
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153 | ** the documentation and/or other materials provided with the
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154 | ** distribution.
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155 | **
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156 | ** 3 Neither the name of the Standards Of Fundamental Astronomy Board,
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157 | ** the International Astronomical Union nor the names of its
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158 | ** contributors may be used to endorse or promote products derived
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159 | ** from this software without specific prior written permission.
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160 | **
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161 | ** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
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162 | ** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
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163 | ** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
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164 | ** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE
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165 | ** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
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166 | ** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
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167 | ** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
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168 | ** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
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169 | ** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
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170 | ** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
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171 | ** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
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172 | ** POSSIBILITY OF SUCH DAMAGE.
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173 | **
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174 | */
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