| 1 | #include "erfa.h" | 
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| 2 |  | 
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| 3 | double eraGst00b(double uta, double utb) | 
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| 4 | /* | 
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| 5 | **  - - - - - - - - - - | 
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| 6 | **   e r a G s t 0 0 b | 
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| 7 | **  - - - - - - - - - - | 
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| 8 | ** | 
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| 9 | **  Greenwich apparent sidereal time (consistent with IAU 2000 | 
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| 10 | **  resolutions but using the truncated nutation model IAU 2000B). | 
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| 11 | ** | 
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| 12 | **  Given: | 
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| 13 | **     uta,utb    double    UT1 as a 2-part Julian Date (Notes 1,2) | 
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| 14 | ** | 
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| 15 | **  Returned (function value): | 
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| 16 | **                double    Greenwich apparent sidereal time (radians) | 
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| 17 | ** | 
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| 18 | **  Notes: | 
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| 19 | ** | 
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| 20 | **  1) The UT1 date uta+utb is a Julian Date, apportioned in any | 
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| 21 | **     convenient way between the argument pair.  For example, | 
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| 22 | **     JD=2450123.7 could be expressed in any of these ways, among | 
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| 23 | **     others: | 
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| 24 | ** | 
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| 25 | **             uta            utb | 
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| 26 | ** | 
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| 27 | **         2450123.7           0.0       (JD method) | 
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| 28 | **         2451545.0       -1421.3       (J2000 method) | 
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| 29 | **         2400000.5       50123.2       (MJD method) | 
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| 30 | **         2450123.5           0.2       (date & time method) | 
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| 31 | ** | 
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| 32 | **     The JD method is the most natural and convenient to use in cases | 
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| 33 | **     where the loss of several decimal digits of resolution is | 
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| 34 | **     acceptable.  The J2000 and MJD methods are good compromises | 
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| 35 | **     between resolution and convenience.  For UT, the date & time | 
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| 36 | **     method is best matched to the algorithm that is used by the Earth | 
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| 37 | **     Rotation Angle function, called internally:  maximum precision is | 
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| 38 | **     delivered when the uta argument is for 0hrs UT1 on the day in | 
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| 39 | **     question and the utb argument lies in the range 0 to 1, or vice | 
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| 40 | **     versa. | 
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| 41 | ** | 
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| 42 | **  2) The result is compatible with the IAU 2000 resolutions, except | 
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| 43 | **     that accuracy has been compromised for the sake of speed and | 
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| 44 | **     convenience in two respects: | 
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| 45 | ** | 
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| 46 | **     . UT is used instead of TDB (or TT) to compute the precession | 
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| 47 | **       component of GMST and the equation of the equinoxes.  This | 
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| 48 | **       results in errors of order 0.1 mas at present. | 
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| 49 | ** | 
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| 50 | **     . The IAU 2000B abridged nutation model (McCarthy & Luzum, 2001) | 
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| 51 | **       is used, introducing errors of up to 1 mas. | 
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| 52 | ** | 
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| 53 | **  3) This GAST is compatible with the IAU 2000 resolutions and must be | 
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| 54 | **     used only in conjunction with other IAU 2000 compatible | 
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| 55 | **     components such as precession-nutation. | 
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| 56 | ** | 
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| 57 | **  4) The result is returned in the range 0 to 2pi. | 
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| 58 | ** | 
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| 59 | **  5) The algorithm is from Capitaine et al. (2003) and IERS | 
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| 60 | **     Conventions 2003. | 
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| 61 | ** | 
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| 62 | **  Called: | 
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| 63 | **     eraGmst00    Greenwich mean sidereal time, IAU 2000 | 
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| 64 | **     eraEe00b     equation of the equinoxes, IAU 2000B | 
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| 65 | **     eraAnp       normalize angle into range 0 to 2pi | 
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| 66 | ** | 
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| 67 | **  References: | 
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| 68 | ** | 
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| 69 | **     Capitaine, N., Wallace, P.T. and McCarthy, D.D., "Expressions to | 
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| 70 | **     implement the IAU 2000 definition of UT1", Astronomy & | 
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| 71 | **     Astrophysics, 406, 1135-1149 (2003) | 
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| 72 | ** | 
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| 73 | **     McCarthy, D.D. & Luzum, B.J., "An abridged model of the | 
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| 74 | **     precession-nutation of the celestial pole", Celestial Mechanics & | 
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| 75 | **     Dynamical Astronomy, 85, 37-49 (2003) | 
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| 76 | ** | 
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| 77 | **     McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003), | 
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| 78 | **     IERS Technical Note No. 32, BKG (2004) | 
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| 79 | ** | 
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| 80 | **  Copyright (C) 2013-2017, NumFOCUS Foundation. | 
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| 81 | **  Derived, with permission, from the SOFA library.  See notes at end of file. | 
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| 82 | */ | 
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| 83 | { | 
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| 84 | double gmst00, ee00b, gst; | 
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| 85 |  | 
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| 86 |  | 
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| 87 | gmst00 = eraGmst00(uta, utb, uta, utb); | 
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| 88 | ee00b = eraEe00b(uta, utb); | 
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| 89 | gst = eraAnp(gmst00 + ee00b); | 
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| 90 |  | 
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| 91 | return gst; | 
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| 92 |  | 
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| 93 | } | 
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| 94 | /*---------------------------------------------------------------------- | 
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| 95 | ** | 
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| 96 | ** | 
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| 97 | **  Copyright (C) 2013-2017, NumFOCUS Foundation. | 
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| 98 | **  All rights reserved. | 
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| 99 | ** | 
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| 100 | **  This library is derived, with permission, from the International | 
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| 101 | **  Astronomical Union's "Standards of Fundamental Astronomy" library, | 
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| 102 | **  available from http://www.iausofa.org. | 
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| 103 | ** | 
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| 104 | **  The ERFA version is intended to retain identical functionality to | 
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| 105 | **  the SOFA library, but made distinct through different function and | 
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| 106 | **  file names, as set out in the SOFA license conditions.  The SOFA | 
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| 107 | **  original has a role as a reference standard for the IAU and IERS, | 
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| 108 | **  and consequently redistribution is permitted only in its unaltered | 
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| 109 | **  state.  The ERFA version is not subject to this restriction and | 
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| 110 | **  therefore can be included in distributions which do not support the | 
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| 111 | **  concept of "read only" software. | 
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| 112 | ** | 
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| 113 | **  Although the intent is to replicate the SOFA API (other than | 
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| 114 | **  replacement of prefix names) and results (with the exception of | 
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| 115 | **  bugs;  any that are discovered will be fixed), SOFA is not | 
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| 116 | **  responsible for any errors found in this version of the library. | 
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| 117 | ** | 
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| 118 | **  If you wish to acknowledge the SOFA heritage, please acknowledge | 
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| 119 | **  that you are using a library derived from SOFA, rather than SOFA | 
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| 120 | **  itself. | 
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| 121 | ** | 
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| 122 | ** | 
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| 123 | **  TERMS AND CONDITIONS | 
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| 124 | ** | 
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| 125 | **  Redistribution and use in source and binary forms, with or without | 
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| 126 | **  modification, are permitted provided that the following conditions | 
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| 127 | **  are met: | 
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| 128 | ** | 
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| 129 | **  1 Redistributions of source code must retain the above copyright | 
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| 130 | **    notice, this list of conditions and the following disclaimer. | 
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| 131 | ** | 
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| 132 | **  2 Redistributions in binary form must reproduce the above copyright | 
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| 133 | **    notice, this list of conditions and the following disclaimer in | 
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| 134 | **    the documentation and/or other materials provided with the | 
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| 135 | **    distribution. | 
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| 136 | ** | 
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| 137 | **  3 Neither the name of the Standards Of Fundamental Astronomy Board, | 
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| 138 | **    the International Astronomical Union nor the names of its | 
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| 139 | **    contributors may be used to endorse or promote products derived | 
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| 140 | **    from this software without specific prior written permission. | 
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| 141 | ** | 
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| 142 | **  THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS | 
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| 143 | **  "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT | 
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| 144 | **  LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS | 
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| 145 | **  FOR A PARTICULAR PURPOSE ARE DISCLAIMED.  IN NO EVENT SHALL THE | 
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| 146 | **  COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT, | 
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| 147 | **  INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, | 
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| 148 | **  BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; | 
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| 149 | **  LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER | 
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| 150 | **  CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT | 
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| 151 | **  LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN | 
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| 152 | **  ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE | 
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| 153 | **  POSSIBILITY OF SUCH DAMAGE. | 
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| 154 | ** | 
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| 155 | */ | 
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