| 1 | #include "erfa.h"
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| 2 |
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| 3 | void eraAper(double theta, eraASTROM *astrom)
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| 4 | /*
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| 5 | ** - - - - - - - -
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| 6 | ** e r a A p e r
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| 7 | ** - - - - - - - -
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| 8 | **
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| 9 | ** In the star-independent astrometry parameters, update only the
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| 10 | ** Earth rotation angle, supplied by the caller explicitly.
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| 11 | **
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| 12 | ** Given:
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| 13 | ** theta double Earth rotation angle (radians, Note 2)
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| 14 | ** astrom eraASTROM* star-independent astrometry parameters:
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| 15 | ** pmt double not used
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| 16 | ** eb double[3] not used
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| 17 | ** eh double[3] not used
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| 18 | ** em double not used
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| 19 | ** v double[3] not used
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| 20 | ** bm1 double not used
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| 21 | ** bpn double[3][3] not used
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| 22 | ** along double longitude + s' (radians)
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| 23 | ** xpl double not used
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| 24 | ** ypl double not used
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| 25 | ** sphi double not used
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| 26 | ** cphi double not used
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| 27 | ** diurab double not used
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| 28 | ** eral double not used
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| 29 | ** refa double not used
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| 30 | ** refb double not used
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| 31 | **
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| 32 | ** Returned:
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| 33 | ** astrom eraASTROM* star-independent astrometry parameters:
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| 34 | ** pmt double unchanged
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| 35 | ** eb double[3] unchanged
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| 36 | ** eh double[3] unchanged
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| 37 | ** em double unchanged
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| 38 | ** v double[3] unchanged
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| 39 | ** bm1 double unchanged
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| 40 | ** bpn double[3][3] unchanged
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| 41 | ** along double unchanged
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| 42 | ** xpl double unchanged
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| 43 | ** ypl double unchanged
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| 44 | ** sphi double unchanged
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| 45 | ** cphi double unchanged
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| 46 | ** diurab double unchanged
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| 47 | ** eral double "local" Earth rotation angle (radians)
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| 48 | ** refa double unchanged
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| 49 | ** refb double unchanged
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| 50 | **
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| 51 | ** Notes:
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| 52 | **
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| 53 | ** 1) This function exists to enable sidereal-tracking applications to
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| 54 | ** avoid wasteful recomputation of the bulk of the astrometry
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| 55 | ** parameters: only the Earth rotation is updated.
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| 56 | **
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| 57 | ** 2) For targets expressed as equinox based positions, such as
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| 58 | ** classical geocentric apparent (RA,Dec), the supplied theta can be
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| 59 | ** Greenwich apparent sidereal time rather than Earth rotation
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| 60 | ** angle.
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| 61 | **
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| 62 | ** 3) The function eraAper13 can be used instead of the present
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| 63 | ** function, and starts from UT1 rather than ERA itself.
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| 64 | **
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| 65 | ** 4) This is one of several functions that inserts into the astrom
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| 66 | ** structure star-independent parameters needed for the chain of
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| 67 | ** astrometric transformations ICRS <-> GCRS <-> CIRS <-> observed.
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| 68 | **
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| 69 | ** The various functions support different classes of observer and
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| 70 | ** portions of the transformation chain:
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| 71 | **
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| 72 | ** functions observer transformation
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| 73 | **
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| 74 | ** eraApcg eraApcg13 geocentric ICRS <-> GCRS
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| 75 | ** eraApci eraApci13 terrestrial ICRS <-> CIRS
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| 76 | ** eraApco eraApco13 terrestrial ICRS <-> observed
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| 77 | ** eraApcs eraApcs13 space ICRS <-> GCRS
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| 78 | ** eraAper eraAper13 terrestrial update Earth rotation
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| 79 | ** eraApio eraApio13 terrestrial CIRS <-> observed
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| 80 | **
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| 81 | ** Those with names ending in "13" use contemporary ERFA models to
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| 82 | ** compute the various ephemerides. The others accept ephemerides
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| 83 | ** supplied by the caller.
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| 84 | **
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| 85 | ** The transformation from ICRS to GCRS covers space motion,
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| 86 | ** parallax, light deflection, and aberration. From GCRS to CIRS
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| 87 | ** comprises frame bias and precession-nutation. From CIRS to
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| 88 | ** observed takes account of Earth rotation, polar motion, diurnal
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| 89 | ** aberration and parallax (unless subsumed into the ICRS <-> GCRS
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| 90 | ** transformation), and atmospheric refraction.
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| 91 | **
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| 92 | ** Copyright (C) 2013-2016, NumFOCUS Foundation.
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| 93 | ** Derived, with permission, from the SOFA library. See notes at end of file.
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| 94 | */
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| 95 | {
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| 96 | astrom->eral = theta + astrom->along;
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| 97 |
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| 98 | /* Finished. */
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| 99 |
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| 100 | }
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| 101 | /*----------------------------------------------------------------------
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| 102 | **
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| 103 | **
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| 104 | ** Copyright (C) 2013-2016, NumFOCUS Foundation.
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| 105 | ** All rights reserved.
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| 106 | **
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| 107 | ** This library is derived, with permission, from the International
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| 108 | ** Astronomical Union's "Standards of Fundamental Astronomy" library,
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| 109 | ** available from http://www.iausofa.org.
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| 110 | **
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| 111 | ** The ERFA version is intended to retain identical functionality to
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| 112 | ** the SOFA library, but made distinct through different function and
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| 113 | ** file names, as set out in the SOFA license conditions. The SOFA
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| 114 | ** original has a role as a reference standard for the IAU and IERS,
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| 115 | ** and consequently redistribution is permitted only in its unaltered
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| 116 | ** state. The ERFA version is not subject to this restriction and
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| 117 | ** therefore can be included in distributions which do not support the
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| 118 | ** concept of "read only" software.
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| 119 | **
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| 120 | ** Although the intent is to replicate the SOFA API (other than
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| 121 | ** replacement of prefix names) and results (with the exception of
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| 122 | ** bugs; any that are discovered will be fixed), SOFA is not
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| 123 | ** responsible for any errors found in this version of the library.
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| 124 | **
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| 125 | ** If you wish to acknowledge the SOFA heritage, please acknowledge
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| 126 | ** that you are using a library derived from SOFA, rather than SOFA
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| 127 | ** itself.
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| 128 | **
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| 129 | **
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| 130 | ** TERMS AND CONDITIONS
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| 131 | **
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| 132 | ** Redistribution and use in source and binary forms, with or without
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| 133 | ** modification, are permitted provided that the following conditions
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| 134 | ** are met:
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| 135 | **
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| 136 | ** 1 Redistributions of source code must retain the above copyright
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| 137 | ** notice, this list of conditions and the following disclaimer.
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| 138 | **
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| 139 | ** 2 Redistributions in binary form must reproduce the above copyright
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| 140 | ** notice, this list of conditions and the following disclaimer in
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| 141 | ** the documentation and/or other materials provided with the
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| 142 | ** distribution.
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| 143 | **
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| 144 | ** 3 Neither the name of the Standards Of Fundamental Astronomy Board,
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| 145 | ** the International Astronomical Union nor the names of its
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| 146 | ** contributors may be used to endorse or promote products derived
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| 147 | ** from this software without specific prior written permission.
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| 148 | **
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| 149 | ** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
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| 150 | ** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
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| 151 | ** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
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| 152 | ** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE
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| 153 | ** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
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| 154 | ** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
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| 155 | ** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
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| 156 | ** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
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| 157 | ** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
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| 158 | ** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
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| 159 | ** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
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| 160 | ** POSSIBILITY OF SUCH DAMAGE.
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| 161 | **
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| 162 | */
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