| 1 | #include "erfa.h"
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| 2 |
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| 3 | double eraSp00(double date1, double date2)
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| 4 | /*
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| 5 | ** - - - - - - - -
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| 6 | ** e r a S p 0 0
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| 7 | ** - - - - - - - -
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| 8 | **
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| 9 | ** The TIO locator s', positioning the Terrestrial Intermediate Origin
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| 10 | ** on the equator of the Celestial Intermediate Pole.
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| 11 | **
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| 12 | ** Given:
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| 13 | ** date1,date2 double TT as a 2-part Julian Date (Note 1)
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| 14 | **
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| 15 | ** Returned (function value):
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| 16 | ** double the TIO locator s' in radians (Note 2)
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| 17 | **
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| 18 | ** Notes:
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| 19 | **
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| 20 | ** 1) The TT date date1+date2 is a Julian Date, apportioned in any
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| 21 | ** convenient way between the two arguments. For example,
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| 22 | ** JD(TT)=2450123.7 could be expressed in any of these ways,
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| 23 | ** among others:
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| 24 | **
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| 25 | ** date1 date2
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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
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| 33 | ** cases where the loss of several decimal digits of resolution
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| 34 | ** is acceptable. The J2000 method is best matched to the way
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| 35 | ** the argument is handled internally and will deliver the
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| 36 | ** optimum resolution. The MJD method and the date & time methods
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| 37 | ** are both good compromises between resolution and convenience.
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| 38 | **
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| 39 | ** 2) The TIO locator s' is obtained from polar motion observations by
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| 40 | ** numerical integration, and so is in essence unpredictable.
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| 41 | ** However, it is dominated by a secular drift of about
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| 42 | ** 47 microarcseconds per century, which is the approximation
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| 43 | ** evaluated by the present function.
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| 44 | **
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| 45 | ** Reference:
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| 46 | **
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| 47 | ** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
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| 48 | ** IERS Technical Note No. 32, BKG (2004)
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| 49 | **
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| 50 | ** Copyright (C) 2013-2016, NumFOCUS Foundation.
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| 51 | ** Derived, with permission, from the SOFA library. See notes at end of file.
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| 52 | */
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| 53 | {
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| 54 | double t, sp;
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| 55 |
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| 56 |
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| 57 | /* Interval between fundamental epoch J2000.0 and current date (JC). */
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| 58 | t = ((date1 - ERFA_DJ00) + date2) / ERFA_DJC;
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| 59 |
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| 60 | /* Approximate s'. */
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| 61 | sp = -47e-6 * t * ERFA_DAS2R;
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| 62 |
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| 63 | return sp;
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| 64 |
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| 65 | }
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| 66 | /*----------------------------------------------------------------------
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| 67 | **
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| 68 | **
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| 69 | ** Copyright (C) 2013-2016, NumFOCUS Foundation.
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| 70 | ** All rights reserved.
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| 71 | **
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| 72 | ** This library is derived, with permission, from the International
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| 73 | ** Astronomical Union's "Standards of Fundamental Astronomy" library,
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| 74 | ** available from http://www.iausofa.org.
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| 75 | **
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| 76 | ** The ERFA version is intended to retain identical functionality to
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| 77 | ** the SOFA library, but made distinct through different function and
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| 78 | ** file names, as set out in the SOFA license conditions. The SOFA
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| 79 | ** original has a role as a reference standard for the IAU and IERS,
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| 80 | ** and consequently redistribution is permitted only in its unaltered
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| 81 | ** state. The ERFA version is not subject to this restriction and
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| 82 | ** therefore can be included in distributions which do not support the
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| 83 | ** concept of "read only" software.
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| 84 | **
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| 85 | ** Although the intent is to replicate the SOFA API (other than
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| 86 | ** replacement of prefix names) and results (with the exception of
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| 87 | ** bugs; any that are discovered will be fixed), SOFA is not
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| 88 | ** responsible for any errors found in this version of the library.
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| 89 | **
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| 90 | ** If you wish to acknowledge the SOFA heritage, please acknowledge
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| 91 | ** that you are using a library derived from SOFA, rather than SOFA
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| 92 | ** itself.
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| 93 | **
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| 94 | **
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| 95 | ** TERMS AND CONDITIONS
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| 96 | **
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| 97 | ** Redistribution and use in source and binary forms, with or without
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| 98 | ** modification, are permitted provided that the following conditions
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| 99 | ** are met:
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| 100 | **
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| 101 | ** 1 Redistributions of source code must retain the above copyright
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| 102 | ** notice, this list of conditions and the following disclaimer.
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| 103 | **
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| 104 | ** 2 Redistributions in binary form must reproduce the above copyright
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| 105 | ** notice, this list of conditions and the following disclaimer in
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| 106 | ** the documentation and/or other materials provided with the
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| 107 | ** distribution.
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| 108 | **
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| 109 | ** 3 Neither the name of the Standards Of Fundamental Astronomy Board,
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| 110 | ** the International Astronomical Union nor the names of its
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| 111 | ** contributors may be used to endorse or promote products derived
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| 112 | ** from this software without specific prior written permission.
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| 113 | **
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| 114 | ** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
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| 115 | ** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
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| 116 | ** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
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| 117 | ** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE
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| 118 | ** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
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| 119 | ** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
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| 120 | ** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
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| 121 | ** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
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| 122 | ** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
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| 123 | ** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
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| 124 | ** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
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| 125 | ** POSSIBILITY OF SUCH DAMAGE.
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| 126 | **
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| 127 | */
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