1 | #include "erfa.h"
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2 |
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3 | void eraAb(double pnat[3], double v[3], double s, double bm1,
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4 | double ppr[3])
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5 | /*
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6 | ** - - - - - -
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7 | ** e r a A b
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8 | ** - - - - - -
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9 | **
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10 | ** Apply aberration to transform natural direction into proper
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11 | ** direction.
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12 | **
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13 | ** Given:
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14 | ** pnat double[3] natural direction to the source (unit vector)
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15 | ** v double[3] observer barycentric velocity in units of c
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16 | ** s double distance between the Sun and the observer (au)
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17 | ** bm1 double sqrt(1-|v|^2): reciprocal of Lorenz factor
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18 | **
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19 | ** Returned:
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20 | ** ppr double[3] proper direction to source (unit vector)
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21 | **
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22 | ** Notes:
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23 | **
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24 | ** 1) The algorithm is based on Expr. (7.40) in the Explanatory
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25 | ** Supplement (Urban & Seidelmann 2013), but with the following
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26 | ** changes:
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27 | **
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28 | ** o Rigorous rather than approximate normalization is applied.
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29 | **
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30 | ** o The gravitational potential term from Expr. (7) in
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31 | ** Klioner (2003) is added, taking into account only the Sun's
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32 | ** contribution. This has a maximum effect of about
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33 | ** 0.4 microarcsecond.
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34 | **
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35 | ** 2) In almost all cases, the maximum accuracy will be limited by the
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36 | ** supplied velocity. For example, if the ERFA eraEpv00 function is
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37 | ** used, errors of up to 5 microarcseconds could occur.
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38 | **
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39 | ** References:
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40 | **
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41 | ** Urban, S. & Seidelmann, P. K. (eds), Explanatory Supplement to
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42 | ** the Astronomical Almanac, 3rd ed., University Science Books
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43 | ** (2013).
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44 | **
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45 | ** Klioner, Sergei A., "A practical relativistic model for micro-
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46 | ** arcsecond astrometry in space", Astr. J. 125, 1580-1597 (2003).
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47 | **
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48 | ** Called:
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49 | ** eraPdp scalar product of two p-vectors
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50 | **
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51 | ** Copyright (C) 2013-2016, NumFOCUS Foundation.
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52 | ** Derived, with permission, from the SOFA library. See notes at end of file.
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53 | */
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54 | {
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55 | int i;
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56 | double pdv, w1, w2, r2, w, p[3], r;
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57 |
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58 |
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59 | pdv = eraPdp(pnat, v);
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60 | w1 = 1.0 + pdv/(1.0 + bm1);
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61 | w2 = ERFA_SRS/s;
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62 | r2 = 0.0;
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63 | for (i = 0; i < 3; i++) {
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64 | w = pnat[i]*bm1 + w1*v[i] + w2*(v[i] - pdv*pnat[i]);
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65 | p[i] = w;
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66 | r2 = r2 + w*w;
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67 | }
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68 | r = sqrt(r2);
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69 | for (i = 0; i < 3; i++) {
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70 | ppr[i] = p[i]/r;
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71 | }
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72 |
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73 | /* Finished. */
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74 |
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75 | }
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76 | /*----------------------------------------------------------------------
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77 | **
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78 | **
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79 | ** Copyright (C) 2013-2016, NumFOCUS Foundation.
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80 | ** All rights reserved.
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81 | **
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82 | ** This library is derived, with permission, from the International
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83 | ** Astronomical Union's "Standards of Fundamental Astronomy" library,
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84 | ** available from http://www.iausofa.org.
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85 | **
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86 | ** The ERFA version is intended to retain identical functionality to
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87 | ** the SOFA library, but made distinct through different function and
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88 | ** file names, as set out in the SOFA license conditions. The SOFA
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89 | ** original has a role as a reference standard for the IAU and IERS,
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90 | ** and consequently redistribution is permitted only in its unaltered
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91 | ** state. The ERFA version is not subject to this restriction and
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92 | ** therefore can be included in distributions which do not support the
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93 | ** concept of "read only" software.
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94 | **
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95 | ** Although the intent is to replicate the SOFA API (other than
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96 | ** replacement of prefix names) and results (with the exception of
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97 | ** bugs; any that are discovered will be fixed), SOFA is not
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98 | ** responsible for any errors found in this version of the library.
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99 | **
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100 | ** If you wish to acknowledge the SOFA heritage, please acknowledge
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101 | ** that you are using a library derived from SOFA, rather than SOFA
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102 | ** itself.
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103 | **
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104 | **
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105 | ** TERMS AND CONDITIONS
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106 | **
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107 | ** Redistribution and use in source and binary forms, with or without
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108 | ** modification, are permitted provided that the following conditions
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109 | ** are met:
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110 | **
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111 | ** 1 Redistributions of source code must retain the above copyright
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112 | ** notice, this list of conditions and the following disclaimer.
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113 | **
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114 | ** 2 Redistributions in binary form must reproduce the above copyright
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115 | ** notice, this list of conditions and the following disclaimer in
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116 | ** the documentation and/or other materials provided with the
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117 | ** distribution.
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118 | **
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119 | ** 3 Neither the name of the Standards Of Fundamental Astronomy Board,
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120 | ** the International Astronomical Union nor the names of its
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121 | ** contributors may be used to endorse or promote products derived
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122 | ** from this software without specific prior written permission.
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123 | **
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124 | ** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
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125 | ** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
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126 | ** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
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127 | ** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE
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128 | ** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
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129 | ** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
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130 | ** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
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131 | ** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
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132 | ** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
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133 | ** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
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134 | ** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
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135 | ** POSSIBILITY OF SUCH DAMAGE.
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136 | **
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137 | */
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