1 | #include "erfa.h"
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2 |
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3 | void eraPv2s(double pv[2][3],
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4 | double *theta, double *phi, double *r,
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5 | double *td, double *pd, double *rd)
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6 | /*
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7 | ** - - - - - - - -
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8 | ** e r a P v 2 s
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9 | ** - - - - - - - -
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10 | **
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11 | ** Convert position/velocity from Cartesian to spherical coordinates.
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12 | **
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13 | ** Given:
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14 | ** pv double[2][3] pv-vector
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15 | **
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16 | ** Returned:
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17 | ** theta double longitude angle (radians)
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18 | ** phi double latitude angle (radians)
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19 | ** r double radial distance
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20 | ** td double rate of change of theta
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21 | ** pd double rate of change of phi
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22 | ** rd double rate of change of r
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23 | **
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24 | ** Notes:
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25 | **
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26 | ** 1) If the position part of pv is null, theta, phi, td and pd
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27 | ** are indeterminate. This is handled by extrapolating the
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28 | ** position through unit time by using the velocity part of
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29 | ** pv. This moves the origin without changing the direction
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30 | ** of the velocity component. If the position and velocity
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31 | ** components of pv are both null, zeroes are returned for all
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32 | ** six results.
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33 | **
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34 | ** 2) If the position is a pole, theta, td and pd are indeterminate.
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35 | ** In such cases zeroes are returned for all three.
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36 | **
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37 | ** Copyright (C) 2013-2015, NumFOCUS Foundation.
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38 | ** Derived, with permission, from the SOFA library. See notes at end of file.
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39 | */
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40 | {
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41 | double x, y, z, xd, yd, zd, rxy2, rxy, r2, rtrue, rw, xyp;
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42 |
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43 | /* Components of position/velocity vector. */
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44 | x = pv[0][0];
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45 | y = pv[0][1];
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46 | z = pv[0][2];
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47 | xd = pv[1][0];
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48 | yd = pv[1][1];
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49 | zd = pv[1][2];
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50 |
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51 | /* Component of r in XY plane squared. */
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52 | rxy2 = x*x + y*y;
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53 |
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54 | /* Modulus squared. */
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55 | r2 = rxy2 + z*z;
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56 |
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57 | /* Modulus. */
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58 | rtrue = sqrt(r2);
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59 |
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60 | /* If null vector, move the origin along the direction of movement. */
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61 | rw = rtrue;
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62 | if (rtrue == 0.0) {
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63 | x = xd;
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64 | y = yd;
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65 | z = zd;
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66 | rxy2 = x*x + y*y;
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67 | r2 = rxy2 + z*z;
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68 | rw = sqrt(r2);
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69 | }
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70 |
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71 | /* Position and velocity in spherical coordinates. */
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72 | rxy = sqrt(rxy2);
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73 | xyp = x*xd + y*yd;
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74 | if (rxy2 != 0.0) {
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75 | *theta = atan2(y, x);
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76 | *phi = atan2(z, rxy);
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77 | *td = (x*yd - y*xd) / rxy2;
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78 | *pd = (zd*rxy2 - z*xyp) / (r2*rxy);
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79 | } else {
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80 | *theta = 0.0;
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81 | *phi = (z != 0.0) ? atan2(z, rxy) : 0.0;
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82 | *td = 0.0;
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83 | *pd = 0.0;
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84 | }
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85 | *r = rtrue;
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86 | *rd = (rw != 0.0) ? (xyp + z*zd) / rw : 0.0;
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87 |
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88 | return;
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89 |
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90 | }
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91 | /*----------------------------------------------------------------------
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92 | **
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93 | **
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94 | ** Copyright (C) 2013-2015, NumFOCUS Foundation.
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95 | ** All rights reserved.
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96 | **
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97 | ** This library is derived, with permission, from the International
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98 | ** Astronomical Union's "Standards of Fundamental Astronomy" library,
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99 | ** available from http://www.iausofa.org.
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100 | **
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101 | ** The ERFA version is intended to retain identical functionality to
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102 | ** the SOFA library, but made distinct through different function and
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103 | ** file names, as set out in the SOFA license conditions. The SOFA
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104 | ** original has a role as a reference standard for the IAU and IERS,
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105 | ** and consequently redistribution is permitted only in its unaltered
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106 | ** state. The ERFA version is not subject to this restriction and
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107 | ** therefore can be included in distributions which do not support the
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108 | ** concept of "read only" software.
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109 | **
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110 | ** Although the intent is to replicate the SOFA API (other than
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111 | ** replacement of prefix names) and results (with the exception of
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112 | ** bugs; any that are discovered will be fixed), SOFA is not
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113 | ** responsible for any errors found in this version of the library.
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114 | **
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115 | ** If you wish to acknowledge the SOFA heritage, please acknowledge
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116 | ** that you are using a library derived from SOFA, rather than SOFA
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117 | ** itself.
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118 | **
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119 | **
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120 | ** TERMS AND CONDITIONS
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121 | **
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122 | ** Redistribution and use in source and binary forms, with or without
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123 | ** modification, are permitted provided that the following conditions
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124 | ** are met:
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125 | **
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126 | ** 1 Redistributions of source code must retain the above copyright
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127 | ** notice, this list of conditions and the following disclaimer.
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128 | **
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129 | ** 2 Redistributions in binary form must reproduce the above copyright
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130 | ** notice, this list of conditions and the following disclaimer in
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131 | ** the documentation and/or other materials provided with the
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132 | ** distribution.
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133 | **
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134 | ** 3 Neither the name of the Standards Of Fundamental Astronomy Board,
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135 | ** the International Astronomical Union nor the names of its
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136 | ** contributors may be used to endorse or promote products derived
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137 | ** from this software without specific prior written permission.
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138 | **
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139 | ** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
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140 | ** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
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141 | ** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
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142 | ** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE
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143 | ** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
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144 | ** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
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145 | ** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
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146 | ** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
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147 | ** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
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148 | ** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
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149 | ** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
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150 | ** POSSIBILITY OF SUCH DAMAGE.
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151 | **
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152 | */
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