| 1 | #include "erfa.h"
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| 2 |
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| 3 | double eraGmst82(double dj1, double dj2)
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| 4 | /*
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| 5 | ** - - - - - - - - - -
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| 6 | ** e r a G m s t 8 2
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| 7 | ** - - - - - - - - - -
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| 8 | **
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| 9 | ** Universal Time to Greenwich mean sidereal time (IAU 1982 model).
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| 10 | **
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| 11 | ** Given:
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| 12 | ** dj1,dj2 double UT1 Julian Date (see note)
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| 13 | **
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| 14 | ** Returned (function value):
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| 15 | ** double Greenwich mean sidereal time (radians)
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| 16 | **
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| 17 | ** Notes:
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| 18 | **
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| 19 | ** 1) The UT1 date dj1+dj2 is a Julian Date, apportioned in any
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| 20 | ** convenient way between the arguments dj1 and dj2. For example,
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| 21 | ** JD(UT1)=2450123.7 could be expressed in any of these ways,
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| 22 | ** among others:
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| 23 | **
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| 24 | ** dj1 dj2
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| 25 | **
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| 26 | ** 2450123.7 0 (JD method)
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| 27 | ** 2451545 -1421.3 (J2000 method)
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| 28 | ** 2400000.5 50123.2 (MJD method)
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| 29 | ** 2450123.5 0.2 (date & time method)
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| 30 | **
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| 31 | ** The JD method is the most natural and convenient to use in
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| 32 | ** cases where the loss of several decimal digits of resolution
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| 33 | ** is acceptable. The J2000 and MJD methods are good compromises
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| 34 | ** between resolution and convenience. The date & time method is
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| 35 | ** best matched to the algorithm used: maximum accuracy (or, at
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| 36 | ** least, minimum noise) is delivered when the dj1 argument is for
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| 37 | ** 0hrs UT1 on the day in question and the dj2 argument lies in the
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| 38 | ** range 0 to 1, or vice versa.
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| 39 | **
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| 40 | ** 2) The algorithm is based on the IAU 1982 expression. This is
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| 41 | ** always described as giving the GMST at 0 hours UT1. In fact, it
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| 42 | ** gives the difference between the GMST and the UT, the steady
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| 43 | ** 4-minutes-per-day drawing-ahead of ST with respect to UT. When
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| 44 | ** whole days are ignored, the expression happens to equal the GMST
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| 45 | ** at 0 hours UT1 each day.
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| 46 | **
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| 47 | ** 3) In this function, the entire UT1 (the sum of the two arguments
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| 48 | ** dj1 and dj2) is used directly as the argument for the standard
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| 49 | ** formula, the constant term of which is adjusted by 12 hours to
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| 50 | ** take account of the noon phasing of Julian Date. The UT1 is then
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| 51 | ** added, but omitting whole days to conserve accuracy.
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| 52 | **
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| 53 | ** Called:
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| 54 | ** eraAnp normalize angle into range 0 to 2pi
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| 55 | **
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| 56 | ** References:
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| 57 | **
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| 58 | ** Transactions of the International Astronomical Union,
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| 59 | ** XVIII B, 67 (1983).
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| 60 | **
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| 61 | ** Aoki et al., Astron. Astrophys. 105, 359-361 (1982).
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| 62 | **
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| 63 | ** Copyright (C) 2013-2017, NumFOCUS Foundation.
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| 64 | ** Derived, with permission, from the SOFA library. See notes at end of file.
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| 65 | */
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| 66 | {
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| 67 | /* Coefficients of IAU 1982 GMST-UT1 model */
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| 68 | double A = 24110.54841 - ERFA_DAYSEC / 2.0;
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| 69 | double B = 8640184.812866;
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| 70 | double C = 0.093104;
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| 71 | double D = -6.2e-6;
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| 72 |
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| 73 | /* Note: the first constant, A, has to be adjusted by 12 hours */
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| 74 | /* because the UT1 is supplied as a Julian date, which begins */
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| 75 | /* at noon. */
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| 76 |
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| 77 | double d1, d2, t, f, gmst;
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| 78 |
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| 79 |
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| 80 | /* Julian centuries since fundamental epoch. */
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| 81 | if (dj1 < dj2) {
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| 82 | d1 = dj1;
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| 83 | d2 = dj2;
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| 84 | } else {
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| 85 | d1 = dj2;
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| 86 | d2 = dj1;
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| 87 | }
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| 88 | t = (d1 + (d2 - ERFA_DJ00)) / ERFA_DJC;
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| 89 |
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| 90 | /* Fractional part of JD(UT1), in seconds. */
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| 91 | f = ERFA_DAYSEC * (fmod(d1, 1.0) + fmod(d2, 1.0));
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| 92 |
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| 93 | /* GMST at this UT1. */
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| 94 | gmst = eraAnp(ERFA_DS2R * ((A + (B + (C + D * t) * t) * t) + f));
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| 95 |
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| 96 | return gmst;
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| 97 |
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| 98 | }
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| 99 | /*----------------------------------------------------------------------
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| 100 | **
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| 101 | **
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| 102 | ** Copyright (C) 2013-2017, NumFOCUS Foundation.
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| 103 | ** All rights reserved.
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| 104 | **
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| 105 | ** This library is derived, with permission, from the International
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| 106 | ** Astronomical Union's "Standards of Fundamental Astronomy" library,
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| 107 | ** available from http://www.iausofa.org.
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| 108 | **
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| 109 | ** The ERFA version is intended to retain identical functionality to
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| 110 | ** the SOFA library, but made distinct through different function and
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| 111 | ** file names, as set out in the SOFA license conditions. The SOFA
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| 112 | ** original has a role as a reference standard for the IAU and IERS,
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| 113 | ** and consequently redistribution is permitted only in its unaltered
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| 114 | ** state. The ERFA version is not subject to this restriction and
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| 115 | ** therefore can be included in distributions which do not support the
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| 116 | ** concept of "read only" software.
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| 117 | **
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| 118 | ** Although the intent is to replicate the SOFA API (other than
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| 119 | ** replacement of prefix names) and results (with the exception of
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| 120 | ** bugs; any that are discovered will be fixed), SOFA is not
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| 121 | ** responsible for any errors found in this version of the library.
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| 122 | **
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| 123 | ** If you wish to acknowledge the SOFA heritage, please acknowledge
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| 124 | ** that you are using a library derived from SOFA, rather than SOFA
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| 125 | ** itself.
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| 126 | **
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| 127 | **
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| 128 | ** TERMS AND CONDITIONS
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| 129 | **
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| 130 | ** Redistribution and use in source and binary forms, with or without
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| 131 | ** modification, are permitted provided that the following conditions
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| 132 | ** are met:
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| 133 | **
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| 134 | ** 1 Redistributions of source code must retain the above copyright
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| 135 | ** notice, this list of conditions and the following disclaimer.
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| 136 | **
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| 137 | ** 2 Redistributions in binary form must reproduce the above copyright
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| 138 | ** notice, this list of conditions and the following disclaimer in
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| 139 | ** the documentation and/or other materials provided with the
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| 140 | ** distribution.
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| 141 | **
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| 142 | ** 3 Neither the name of the Standards Of Fundamental Astronomy Board,
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| 143 | ** the International Astronomical Union nor the names of its
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| 144 | ** contributors may be used to endorse or promote products derived
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| 145 | ** from this software without specific prior written permission.
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| 146 | **
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| 147 | ** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
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| 148 | ** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
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| 149 | ** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
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| 150 | ** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE
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| 151 | ** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
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| 152 | ** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
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| 153 | ** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
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| 154 | ** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
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| 155 | ** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
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| 156 | ** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
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| 157 | ** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
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| 158 | ** POSSIBILITY OF SUCH DAMAGE.
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| 159 | **
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| 160 | */
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