| 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) 2013-2017, 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 |
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| 44 | /* Components of position/velocity vector. */
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| 45 | x = pv[0][0];
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| 46 | y = pv[0][1];
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| 47 | z = pv[0][2];
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| 48 | xd = pv[1][0];
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| 49 | yd = pv[1][1];
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| 50 | zd = pv[1][2];
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| 51 |
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| 52 | /* Component of r in XY plane squared. */
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| 53 | rxy2 = x*x + y*y;
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| 54 |
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| 55 | /* Modulus squared. */
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| 56 | r2 = rxy2 + z*z;
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| 57 |
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| 58 | /* Modulus. */
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| 59 | rtrue = sqrt(r2);
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| 60 |
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| 61 | /* If null vector, move the origin along the direction of movement. */
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| 62 | rw = rtrue;
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| 63 | if (rtrue == 0.0) {
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| 64 | x = xd;
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| 65 | y = yd;
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| 66 | z = zd;
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| 67 | rxy2 = x*x + y*y;
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| 68 | r2 = rxy2 + z*z;
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| 69 | rw = sqrt(r2);
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| 70 | }
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| 71 |
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| 72 | /* Position and velocity in spherical coordinates. */
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| 73 | rxy = sqrt(rxy2);
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| 74 | xyp = x*xd + y*yd;
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| 75 | if (rxy2 != 0.0) {
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| 76 | *theta = atan2(y, x);
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| 77 | *phi = atan2(z, rxy);
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| 78 | *td = (x*yd - y*xd) / rxy2;
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| 79 | *pd = (zd*rxy2 - z*xyp) / (r2*rxy);
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| 80 | } else {
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| 81 | *theta = 0.0;
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| 82 | *phi = (z != 0.0) ? atan2(z, rxy) : 0.0;
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| 83 | *td = 0.0;
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| 84 | *pd = 0.0;
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| 85 | }
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| 86 | *r = rtrue;
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| 87 | *rd = (rw != 0.0) ? (xyp + z*zd) / rw : 0.0;
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| 88 |
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| 89 | return;
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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 | **
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| 95 | ** Copyright (C) 2013-2017, NumFOCUS Foundation.
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| 96 | ** All rights reserved.
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| 97 | **
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| 98 | ** This library is derived, with permission, from the International
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| 99 | ** Astronomical Union's "Standards of Fundamental Astronomy" library,
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| 100 | ** available from http://www.iausofa.org.
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| 101 | **
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| 102 | ** The ERFA version is intended to retain identical functionality to
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| 103 | ** the SOFA library, but made distinct through different function and
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| 104 | ** file names, as set out in the SOFA license conditions. The SOFA
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| 105 | ** original has a role as a reference standard for the IAU and IERS,
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| 106 | ** and consequently redistribution is permitted only in its unaltered
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| 107 | ** state. The ERFA version is not subject to this restriction and
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| 108 | ** therefore can be included in distributions which do not support the
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| 109 | ** concept of "read only" software.
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| 110 | **
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| 111 | ** Although the intent is to replicate the SOFA API (other than
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| 112 | ** replacement of prefix names) and results (with the exception of
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| 113 | ** bugs; any that are discovered will be fixed), SOFA is not
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| 114 | ** responsible for any errors found in this version of the library.
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| 115 | **
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| 116 | ** If you wish to acknowledge the SOFA heritage, please acknowledge
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| 117 | ** that you are using a library derived from SOFA, rather than SOFA
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| 118 | ** itself.
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| 119 | **
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| 120 | **
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| 121 | ** TERMS AND CONDITIONS
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| 122 | **
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| 123 | ** Redistribution and use in source and binary forms, with or without
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| 124 | ** modification, are permitted provided that the following conditions
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| 125 | ** are met:
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| 126 | **
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| 127 | ** 1 Redistributions of source code must retain the above copyright
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| 128 | ** notice, this list of conditions and the following disclaimer.
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| 129 | **
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| 130 | ** 2 Redistributions in binary form must reproduce the above copyright
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| 131 | ** notice, this list of conditions and the following disclaimer in
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| 132 | ** the documentation and/or other materials provided with the
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| 133 | ** distribution.
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| 134 | **
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| 135 | ** 3 Neither the name of the Standards Of Fundamental Astronomy Board,
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| 136 | ** the International Astronomical Union nor the names of its
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| 137 | ** contributors may be used to endorse or promote products derived
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| 138 | ** from this software without specific prior written permission.
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| 139 | **
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| 140 | ** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
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| 141 | ** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
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| 142 | ** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
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| 143 | ** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE
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| 144 | ** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
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| 145 | ** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
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| 146 | ** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
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| 147 | ** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
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| 148 | ** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
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| 149 | ** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
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| 150 | ** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
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| 151 | ** POSSIBILITY OF SUCH DAMAGE.
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| 152 | **
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| 153 | */
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