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| 1 |  |  |  |  |  |  | #include "erfa.h" | 
| 2 |  |  |  |  |  |  |  | 
| 3 | 0 |  |  |  |  |  | int eraGc2gde ( double a, double f, double xyz[3], | 
| 4 |  |  |  |  |  |  | double *elong, double *phi, double *height ) | 
| 5 |  |  |  |  |  |  | /* | 
| 6 |  |  |  |  |  |  | **  - - - - - - - - - - | 
| 7 |  |  |  |  |  |  | **   e r a G c 2 g d e | 
| 8 |  |  |  |  |  |  | **  - - - - - - - - - - | 
| 9 |  |  |  |  |  |  | ** | 
| 10 |  |  |  |  |  |  | **  Transform geocentric coordinates to geodetic for a reference | 
| 11 |  |  |  |  |  |  | **  ellipsoid of specified form. | 
| 12 |  |  |  |  |  |  | ** | 
| 13 |  |  |  |  |  |  | **  Given: | 
| 14 |  |  |  |  |  |  | **     a       double     equatorial radius (Notes 2,4) | 
| 15 |  |  |  |  |  |  | **     f       double     flattening (Note 3) | 
| 16 |  |  |  |  |  |  | **     xyz     double[3]  geocentric vector (Note 4) | 
| 17 |  |  |  |  |  |  | ** | 
| 18 |  |  |  |  |  |  | **  Returned: | 
| 19 |  |  |  |  |  |  | **     elong   double     longitude (radians, east +ve) | 
| 20 |  |  |  |  |  |  | **     phi     double     latitude (geodetic, radians) | 
| 21 |  |  |  |  |  |  | **     height  double     height above ellipsoid (geodetic, Note 4) | 
| 22 |  |  |  |  |  |  | ** | 
| 23 |  |  |  |  |  |  | **  Returned (function value): | 
| 24 |  |  |  |  |  |  | **             int        status:  0 = OK | 
| 25 |  |  |  |  |  |  | **                                -1 = illegal f | 
| 26 |  |  |  |  |  |  | **                                -2 = illegal a | 
| 27 |  |  |  |  |  |  | ** | 
| 28 |  |  |  |  |  |  | **  Notes: | 
| 29 |  |  |  |  |  |  | ** | 
| 30 |  |  |  |  |  |  | **  1) This function is based on the GCONV2H Fortran subroutine by | 
| 31 |  |  |  |  |  |  | **     Toshio Fukushima (see reference). | 
| 32 |  |  |  |  |  |  | ** | 
| 33 |  |  |  |  |  |  | **  2) The equatorial radius, a, can be in any units, but meters is | 
| 34 |  |  |  |  |  |  | **     the conventional choice. | 
| 35 |  |  |  |  |  |  | ** | 
| 36 |  |  |  |  |  |  | **  3) The flattening, f, is (for the Earth) a value around 0.00335, | 
| 37 |  |  |  |  |  |  | **     i.e. around 1/298. | 
| 38 |  |  |  |  |  |  | ** | 
| 39 |  |  |  |  |  |  | **  4) The equatorial radius, a, and the geocentric vector, xyz, | 
| 40 |  |  |  |  |  |  | **     must be given in the same units, and determine the units of | 
| 41 |  |  |  |  |  |  | **     the returned height, height. | 
| 42 |  |  |  |  |  |  | ** | 
| 43 |  |  |  |  |  |  | **  5) If an error occurs (status < 0), elong, phi and height are | 
| 44 |  |  |  |  |  |  | **     unchanged. | 
| 45 |  |  |  |  |  |  | ** | 
| 46 |  |  |  |  |  |  | **  6) The inverse transformation is performed in the function | 
| 47 |  |  |  |  |  |  | **     eraGd2gce. | 
| 48 |  |  |  |  |  |  | ** | 
| 49 |  |  |  |  |  |  | **  7) The transformation for a standard ellipsoid (such as ERFA_WGS84) can | 
| 50 |  |  |  |  |  |  | **     more conveniently be performed by calling eraGc2gd, which uses a | 
| 51 |  |  |  |  |  |  | **     numerical code to identify the required A and F values. | 
| 52 |  |  |  |  |  |  | ** | 
| 53 |  |  |  |  |  |  | **  Reference: | 
| 54 |  |  |  |  |  |  | ** | 
| 55 |  |  |  |  |  |  | **     Fukushima, T., "Transformation from Cartesian to geodetic | 
| 56 |  |  |  |  |  |  | **     coordinates accelerated by Halley's method", J.Geodesy (2006) | 
| 57 |  |  |  |  |  |  | **     79: 689-693 | 
| 58 |  |  |  |  |  |  | ** | 
| 59 |  |  |  |  |  |  | **  Copyright (C) 2013-2019, NumFOCUS Foundation. | 
| 60 |  |  |  |  |  |  | **  Derived, with permission, from the SOFA library.  See notes at end of file. | 
| 61 |  |  |  |  |  |  | */ | 
| 62 |  |  |  |  |  |  | { | 
| 63 |  |  |  |  |  |  | double aeps2, e2, e4t, ec2, ec, b, x, y, z, p2, absz, p, s0, pn, zc, | 
| 64 |  |  |  |  |  |  | c0, c02, c03, s02, s03, a02, a0, a03, d0, f0, b0, s1, | 
| 65 |  |  |  |  |  |  | cc, s12, cc2; | 
| 66 |  |  |  |  |  |  |  | 
| 67 |  |  |  |  |  |  |  | 
| 68 |  |  |  |  |  |  | /* ------------- */ | 
| 69 |  |  |  |  |  |  | /* Preliminaries */ | 
| 70 |  |  |  |  |  |  | /* ------------- */ | 
| 71 |  |  |  |  |  |  |  | 
| 72 |  |  |  |  |  |  | /* Validate ellipsoid parameters. */ | 
| 73 | 0 | 0 |  |  |  |  | if ( f < 0.0 || f >= 1.0 ) return -1; | 
|  |  | 0 |  |  |  |  |  | 
| 74 | 0 | 0 |  |  |  |  | if ( a <= 0.0 ) return -2; | 
| 75 |  |  |  |  |  |  |  | 
| 76 |  |  |  |  |  |  | /* Functions of ellipsoid parameters (with further validation of f). */ | 
| 77 | 0 |  |  |  |  |  | aeps2 = a*a * 1e-32; | 
| 78 | 0 |  |  |  |  |  | e2 = (2.0 - f) * f; | 
| 79 | 0 |  |  |  |  |  | e4t = e2*e2 * 1.5; | 
| 80 | 0 |  |  |  |  |  | ec2 = 1.0 - e2; | 
| 81 | 0 | 0 |  |  |  |  | if ( ec2 <= 0.0 ) return -1; | 
| 82 | 0 |  |  |  |  |  | ec = sqrt(ec2); | 
| 83 | 0 |  |  |  |  |  | b = a * ec; | 
| 84 |  |  |  |  |  |  |  | 
| 85 |  |  |  |  |  |  | /* Cartesian components. */ | 
| 86 | 0 |  |  |  |  |  | x = xyz[0]; | 
| 87 | 0 |  |  |  |  |  | y = xyz[1]; | 
| 88 | 0 |  |  |  |  |  | z = xyz[2]; | 
| 89 |  |  |  |  |  |  |  | 
| 90 |  |  |  |  |  |  | /* Distance from polar axis squared. */ | 
| 91 | 0 |  |  |  |  |  | p2 = x*x + y*y; | 
| 92 |  |  |  |  |  |  |  | 
| 93 |  |  |  |  |  |  | /* Longitude. */ | 
| 94 | 0 | 0 |  |  |  |  | *elong = p2 > 0.0 ? atan2(y, x) : 0.0; | 
| 95 |  |  |  |  |  |  |  | 
| 96 |  |  |  |  |  |  | /* Unsigned z-coordinate. */ | 
| 97 | 0 |  |  |  |  |  | absz = fabs(z); | 
| 98 |  |  |  |  |  |  |  | 
| 99 |  |  |  |  |  |  | /* Proceed unless polar case. */ | 
| 100 | 0 | 0 |  |  |  |  | if ( p2 > aeps2 ) { | 
| 101 |  |  |  |  |  |  |  | 
| 102 |  |  |  |  |  |  | /* Distance from polar axis. */ | 
| 103 | 0 |  |  |  |  |  | p = sqrt(p2); | 
| 104 |  |  |  |  |  |  |  | 
| 105 |  |  |  |  |  |  | /* Normalization. */ | 
| 106 | 0 |  |  |  |  |  | s0 = absz / a; | 
| 107 | 0 |  |  |  |  |  | pn = p / a; | 
| 108 | 0 |  |  |  |  |  | zc = ec * s0; | 
| 109 |  |  |  |  |  |  |  | 
| 110 |  |  |  |  |  |  | /* Prepare Newton correction factors. */ | 
| 111 | 0 |  |  |  |  |  | c0 = ec * pn; | 
| 112 | 0 |  |  |  |  |  | c02 = c0 * c0; | 
| 113 | 0 |  |  |  |  |  | c03 = c02 * c0; | 
| 114 | 0 |  |  |  |  |  | s02 = s0 * s0; | 
| 115 | 0 |  |  |  |  |  | s03 = s02 * s0; | 
| 116 | 0 |  |  |  |  |  | a02 = c02 + s02; | 
| 117 | 0 |  |  |  |  |  | a0 = sqrt(a02); | 
| 118 | 0 |  |  |  |  |  | a03 = a02 * a0; | 
| 119 | 0 |  |  |  |  |  | d0 = zc*a03 + e2*s03; | 
| 120 | 0 |  |  |  |  |  | f0 = pn*a03 - e2*c03; | 
| 121 |  |  |  |  |  |  |  | 
| 122 |  |  |  |  |  |  | /* Prepare Halley correction factor. */ | 
| 123 | 0 |  |  |  |  |  | b0 = e4t * s02 * c02 * pn * (a0 - ec); | 
| 124 | 0 |  |  |  |  |  | s1 = d0*f0 - b0*s0; | 
| 125 | 0 |  |  |  |  |  | cc = ec * (f0*f0 - b0*c0); | 
| 126 |  |  |  |  |  |  |  | 
| 127 |  |  |  |  |  |  | /* Evaluate latitude and height. */ | 
| 128 | 0 |  |  |  |  |  | *phi = atan(s1/cc); | 
| 129 | 0 |  |  |  |  |  | s12 = s1 * s1; | 
| 130 | 0 |  |  |  |  |  | cc2 = cc * cc; | 
| 131 | 0 |  |  |  |  |  | *height = (p*cc + absz*s1 - a * sqrt(ec2*s12 + cc2)) / | 
| 132 | 0 |  |  |  |  |  | sqrt(s12 + cc2); | 
| 133 |  |  |  |  |  |  | } else { | 
| 134 |  |  |  |  |  |  |  | 
| 135 |  |  |  |  |  |  | /* Exception: pole. */ | 
| 136 | 0 |  |  |  |  |  | *phi = ERFA_DPI / 2.0; | 
| 137 | 0 |  |  |  |  |  | *height = absz - b; | 
| 138 |  |  |  |  |  |  | } | 
| 139 |  |  |  |  |  |  |  | 
| 140 |  |  |  |  |  |  | /* Restore sign of latitude. */ | 
| 141 | 0 | 0 |  |  |  |  | if ( z < 0 ) *phi = -*phi; | 
| 142 |  |  |  |  |  |  |  | 
| 143 |  |  |  |  |  |  | /* OK status. */ | 
| 144 |  |  |  |  |  |  | return 0; | 
| 145 |  |  |  |  |  |  |  | 
| 146 |  |  |  |  |  |  | } | 
| 147 |  |  |  |  |  |  | /*---------------------------------------------------------------------- | 
| 148 |  |  |  |  |  |  | ** | 
| 149 |  |  |  |  |  |  | ** | 
| 150 |  |  |  |  |  |  | **  Copyright (C) 2013-2019, NumFOCUS Foundation. | 
| 151 |  |  |  |  |  |  | **  All rights reserved. | 
| 152 |  |  |  |  |  |  | ** | 
| 153 |  |  |  |  |  |  | **  This library is derived, with permission, from the International | 
| 154 |  |  |  |  |  |  | **  Astronomical Union's "Standards of Fundamental Astronomy" library, | 
| 155 |  |  |  |  |  |  | **  available from http://www.iausofa.org. | 
| 156 |  |  |  |  |  |  | ** | 
| 157 |  |  |  |  |  |  | **  The ERFA version is intended to retain identical functionality to | 
| 158 |  |  |  |  |  |  | **  the SOFA library, but made distinct through different function and | 
| 159 |  |  |  |  |  |  | **  file names, as set out in the SOFA license conditions.  The SOFA | 
| 160 |  |  |  |  |  |  | **  original has a role as a reference standard for the IAU and IERS, | 
| 161 |  |  |  |  |  |  | **  and consequently redistribution is permitted only in its unaltered | 
| 162 |  |  |  |  |  |  | **  state.  The ERFA version is not subject to this restriction and | 
| 163 |  |  |  |  |  |  | **  therefore can be included in distributions which do not support the | 
| 164 |  |  |  |  |  |  | **  concept of "read only" software. | 
| 165 |  |  |  |  |  |  | ** | 
| 166 |  |  |  |  |  |  | **  Although the intent is to replicate the SOFA API (other than | 
| 167 |  |  |  |  |  |  | **  replacement of prefix names) and results (with the exception of | 
| 168 |  |  |  |  |  |  | **  bugs;  any that are discovered will be fixed), SOFA is not | 
| 169 |  |  |  |  |  |  | **  responsible for any errors found in this version of the library. | 
| 170 |  |  |  |  |  |  | ** | 
| 171 |  |  |  |  |  |  | **  If you wish to acknowledge the SOFA heritage, please acknowledge | 
| 172 |  |  |  |  |  |  | **  that you are using a library derived from SOFA, rather than SOFA | 
| 173 |  |  |  |  |  |  | **  itself. | 
| 174 |  |  |  |  |  |  | ** | 
| 175 |  |  |  |  |  |  | ** | 
| 176 |  |  |  |  |  |  | **  TERMS AND CONDITIONS | 
| 177 |  |  |  |  |  |  | ** | 
| 178 |  |  |  |  |  |  | **  Redistribution and use in source and binary forms, with or without | 
| 179 |  |  |  |  |  |  | **  modification, are permitted provided that the following conditions | 
| 180 |  |  |  |  |  |  | **  are met: | 
| 181 |  |  |  |  |  |  | ** | 
| 182 |  |  |  |  |  |  | **  1 Redistributions of source code must retain the above copyright | 
| 183 |  |  |  |  |  |  | **    notice, this list of conditions and the following disclaimer. | 
| 184 |  |  |  |  |  |  | ** | 
| 185 |  |  |  |  |  |  | **  2 Redistributions in binary form must reproduce the above copyright | 
| 186 |  |  |  |  |  |  | **    notice, this list of conditions and the following disclaimer in | 
| 187 |  |  |  |  |  |  | **    the documentation and/or other materials provided with the | 
| 188 |  |  |  |  |  |  | **    distribution. | 
| 189 |  |  |  |  |  |  | ** | 
| 190 |  |  |  |  |  |  | **  3 Neither the name of the Standards Of Fundamental Astronomy Board, | 
| 191 |  |  |  |  |  |  | **    the International Astronomical Union nor the names of its | 
| 192 |  |  |  |  |  |  | **    contributors may be used to endorse or promote products derived | 
| 193 |  |  |  |  |  |  | **    from this software without specific prior written permission. | 
| 194 |  |  |  |  |  |  | ** | 
| 195 |  |  |  |  |  |  | **  THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS | 
| 196 |  |  |  |  |  |  | **  "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT | 
| 197 |  |  |  |  |  |  | **  LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS | 
| 198 |  |  |  |  |  |  | **  FOR A PARTICULAR PURPOSE ARE DISCLAIMED.  IN NO EVENT SHALL THE | 
| 199 |  |  |  |  |  |  | **  COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT, | 
| 200 |  |  |  |  |  |  | **  INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, | 
| 201 |  |  |  |  |  |  | **  BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; | 
| 202 |  |  |  |  |  |  | **  LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER | 
| 203 |  |  |  |  |  |  | **  CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT | 
| 204 |  |  |  |  |  |  | **  LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN | 
| 205 |  |  |  |  |  |  | **  ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE | 
| 206 |  |  |  |  |  |  | **  POSSIBILITY OF SUCH DAMAGE. | 
| 207 |  |  |  |  |  |  | ** | 
| 208 |  |  |  |  |  |  | */ |