1 | #include "erfa.h"
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2 |
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3 | void eraAticq(double ri, double di, eraASTROM *astrom,
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4 | double *rc, double *dc)
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5 | /*
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6 | ** - - - - - - - - -
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7 | ** e r a A t i c q
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8 | ** - - - - - - - - -
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9 | **
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10 | ** Quick CIRS RA,Dec to ICRS astrometric place, given the star-
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11 | ** independent astrometry parameters.
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12 | **
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13 | ** Use of this function is appropriate when efficiency is important and
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14 | ** where many star positions are all to be transformed for one date.
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15 | ** The star-independent astrometry parameters can be obtained by
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16 | ** calling one of the functions eraApci[13], eraApcg[13], eraApco[13]
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17 | ** or eraApcs[13].
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18 | **
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19 | ** Given:
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20 | ** ri,di double CIRS RA,Dec (radians)
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21 | ** astrom eraASTROM* star-independent astrometry parameters:
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22 | ** pmt double PM time interval (SSB, Julian years)
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23 | ** eb double[3] SSB to observer (vector, au)
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24 | ** eh double[3] Sun to observer (unit vector)
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25 | ** em double distance from Sun to observer (au)
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26 | ** v double[3] barycentric observer velocity (vector, c)
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27 | ** bm1 double sqrt(1-|v|^2): reciprocal of Lorenz factor
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28 | ** bpn double[3][3] bias-precession-nutation matrix
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29 | ** along double longitude + s' (radians)
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30 | ** xpl double polar motion xp wrt local meridian (radians)
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31 | ** ypl double polar motion yp wrt local meridian (radians)
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32 | ** sphi double sine of geodetic latitude
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33 | ** cphi double cosine of geodetic latitude
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34 | ** diurab double magnitude of diurnal aberration vector
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35 | ** eral double "local" Earth rotation angle (radians)
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36 | ** refa double refraction constant A (radians)
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37 | ** refb double refraction constant B (radians)
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38 | **
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39 | ** Returned:
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40 | ** rc,dc double ICRS astrometric RA,Dec (radians)
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41 | **
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42 | ** Notes:
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43 | **
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44 | ** 1) Only the Sun is taken into account in the light deflection
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45 | ** correction.
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46 | **
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47 | ** 2) Iterative techniques are used for the aberration and light
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48 | ** deflection corrections so that the functions eraAtic13 (or
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49 | ** eraAticq) and eraAtci13 (or eraAtciq) are accurate inverses;
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50 | ** even at the edge of the Sun's disk the discrepancy is only about
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51 | ** 1 nanoarcsecond.
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52 | **
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53 | ** Called:
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54 | ** eraS2c spherical coordinates to unit vector
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55 | ** eraTrxp product of transpose of r-matrix and p-vector
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56 | ** eraZp zero p-vector
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57 | ** eraAb stellar aberration
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58 | ** eraLdsun light deflection by the Sun
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59 | ** eraC2s p-vector to spherical
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60 | ** eraAnp normalize angle into range +/- pi
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61 | **
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62 | ** Copyright (C) 2013-2015, NumFOCUS Foundation.
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63 | ** Derived, with permission, from the SOFA library. See notes at end of file.
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64 | */
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65 | {
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66 | int j, i;
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67 | double pi[3], ppr[3], pnat[3], pco[3], w, d[3], before[3], r2, r,
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68 | after[3];
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69 |
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70 | /* CIRS RA,Dec to Cartesian. */
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71 | eraS2c(ri, di, pi);
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72 |
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73 | /* Bias-precession-nutation, giving GCRS proper direction. */
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74 | eraTrxp(astrom->bpn, pi, ppr);
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75 |
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76 | /* Aberration, giving GCRS natural direction. */
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77 | eraZp(d);
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78 | for (j = 0; j < 2; j++) {
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79 | r2 = 0.0;
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80 | for (i = 0; i < 3; i++) {
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81 | w = ppr[i] - d[i];
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82 | before[i] = w;
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83 | r2 += w*w;
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84 | }
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85 | r = sqrt(r2);
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86 | for (i = 0; i < 3; i++) {
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87 | before[i] /= r;
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88 | }
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89 | eraAb(before, astrom->v, astrom->em, astrom->bm1, after);
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90 | r2 = 0.0;
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91 | for (i = 0; i < 3; i++) {
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92 | d[i] = after[i] - before[i];
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93 | w = ppr[i] - d[i];
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94 | pnat[i] = w;
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95 | r2 += w*w;
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96 | }
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97 | r = sqrt(r2);
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98 | for (i = 0; i < 3; i++) {
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99 | pnat[i] /= r;
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100 | }
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101 | }
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102 |
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103 | /* Light deflection by the Sun, giving BCRS coordinate direction. */
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104 | eraZp(d);
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105 | for (j = 0; j < 5; j++) {
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106 | r2 = 0.0;
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107 | for (i = 0; i < 3; i++) {
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108 | w = pnat[i] - d[i];
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109 | before[i] = w;
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110 | r2 += w*w;
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111 | }
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112 | r = sqrt(r2);
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113 | for (i = 0; i < 3; i++) {
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114 | before[i] /= r;
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115 | }
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116 | eraLdsun(before, astrom->eh, astrom->em, after);
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117 | r2 = 0.0;
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118 | for (i = 0; i < 3; i++) {
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119 | d[i] = after[i] - before[i];
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120 | w = pnat[i] - d[i];
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121 | pco[i] = w;
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122 | r2 += w*w;
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123 | }
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124 | r = sqrt(r2);
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125 | for (i = 0; i < 3; i++) {
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126 | pco[i] /= r;
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127 | }
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128 | }
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129 |
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130 | /* ICRS astrometric RA,Dec. */
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131 | eraC2s(pco, &w, dc);
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132 | *rc = eraAnp(w);
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133 |
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134 | /* Finished. */
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135 |
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136 | }
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137 | /*----------------------------------------------------------------------
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138 | **
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139 | **
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140 | ** Copyright (C) 2013-2015, NumFOCUS Foundation.
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141 | ** All rights reserved.
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142 | **
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143 | ** This library is derived, with permission, from the International
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144 | ** Astronomical Union's "Standards of Fundamental Astronomy" library,
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145 | ** available from http://www.iausofa.org.
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146 | **
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147 | ** The ERFA version is intended to retain identical functionality to
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148 | ** the SOFA library, but made distinct through different function and
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149 | ** file names, as set out in the SOFA license conditions. The SOFA
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150 | ** original has a role as a reference standard for the IAU and IERS,
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151 | ** and consequently redistribution is permitted only in its unaltered
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152 | ** state. The ERFA version is not subject to this restriction and
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153 | ** therefore can be included in distributions which do not support the
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154 | ** concept of "read only" software.
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155 | **
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156 | ** Although the intent is to replicate the SOFA API (other than
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157 | ** replacement of prefix names) and results (with the exception of
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158 | ** bugs; any that are discovered will be fixed), SOFA is not
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159 | ** responsible for any errors found in this version of the library.
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160 | **
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161 | ** If you wish to acknowledge the SOFA heritage, please acknowledge
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162 | ** that you are using a library derived from SOFA, rather than SOFA
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163 | ** itself.
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164 | **
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165 | **
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166 | ** TERMS AND CONDITIONS
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167 | **
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168 | ** Redistribution and use in source and binary forms, with or without
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169 | ** modification, are permitted provided that the following conditions
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170 | ** are met:
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171 | **
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172 | ** 1 Redistributions of source code must retain the above copyright
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173 | ** notice, this list of conditions and the following disclaimer.
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174 | **
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175 | ** 2 Redistributions in binary form must reproduce the above copyright
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176 | ** notice, this list of conditions and the following disclaimer in
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177 | ** the documentation and/or other materials provided with the
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178 | ** distribution.
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179 | **
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180 | ** 3 Neither the name of the Standards Of Fundamental Astronomy Board,
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181 | ** the International Astronomical Union nor the names of its
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182 | ** contributors may be used to endorse or promote products derived
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183 | ** from this software without specific prior written permission.
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184 | **
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185 | ** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
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186 | ** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
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187 | ** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
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188 | ** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE
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189 | ** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
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190 | ** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
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191 | ** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
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192 | ** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
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193 | ** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
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194 | ** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
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195 | ** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
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196 | ** POSSIBILITY OF SUCH DAMAGE.
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197 | **
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198 | */
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