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author | William Joye <wjoye@cfa.harvard.edu> | 2019-05-10 19:05:35 (GMT) |
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committer | William Joye <wjoye@cfa.harvard.edu> | 2019-05-10 19:05:35 (GMT) |
commit | 51cd8ee68a63edc414c0fe3344ba0589ac5849dd (patch) | |
tree | 662741d231423544a0c4d8bec55d7c457a18c17e /ast/erfa/atciqz.c | |
parent | beb90b7d3f526440250bba67e5ab07bb7eb7bbc3 (diff) | |
download | blt-51cd8ee68a63edc414c0fe3344ba0589ac5849dd.zip blt-51cd8ee68a63edc414c0fe3344ba0589ac5849dd.tar.gz blt-51cd8ee68a63edc414c0fe3344ba0589ac5849dd.tar.bz2 |
upgrade ast 8.7.1
Diffstat (limited to 'ast/erfa/atciqz.c')
-rw-r--r-- | ast/erfa/atciqz.c | 153 |
1 files changed, 153 insertions, 0 deletions
diff --git a/ast/erfa/atciqz.c b/ast/erfa/atciqz.c new file mode 100644 index 0000000..d141b91 --- /dev/null +++ b/ast/erfa/atciqz.c @@ -0,0 +1,153 @@ +#include "erfa.h" + +void eraAtciqz(double rc, double dc, eraASTROM *astrom, + double *ri, double *di) +/* +** - - - - - - - - - - +** e r a A t c i q z +** - - - - - - - - - - +** +** Quick ICRS to CIRS transformation, given precomputed star- +** independent astrometry parameters, and assuming zero parallax and +** proper motion. +** +** Use of this function is appropriate when efficiency is important and +** where many star positions are to be transformed for one date. The +** star-independent parameters can be obtained by calling one of the +** functions eraApci[13], eraApcg[13], eraApco[13] or eraApcs[13]. +** +** The corresponding function for the case of non-zero parallax and +** proper motion is eraAtciq. +** +** Given: +** rc,dc double ICRS astrometric RA,Dec (radians) +** astrom eraASTROM* star-independent astrometry parameters: +** pmt double PM time interval (SSB, Julian years) +** eb double[3] SSB to observer (vector, au) +** eh double[3] Sun to observer (unit vector) +** em double distance from Sun to observer (au) +** v double[3] barycentric observer velocity (vector, c) +** bm1 double sqrt(1-|v|^2): reciprocal of Lorenz factor +** bpn double[3][3] bias-precession-nutation matrix +** along double longitude + s' (radians) +** xpl double polar motion xp wrt local meridian (radians) +** ypl double polar motion yp wrt local meridian (radians) +** sphi double sine of geodetic latitude +** cphi double cosine of geodetic latitude +** diurab double magnitude of diurnal aberration vector +** eral double "local" Earth rotation angle (radians) +** refa double refraction constant A (radians) +** refb double refraction constant B (radians) +** +** Returned: +** ri,di double CIRS RA,Dec (radians) +** +** Note: +** +** All the vectors are with respect to BCRS axes. +** +** References: +** +** Urban, S. & Seidelmann, P. K. (eds), Explanatory Supplement to +** the Astronomical Almanac, 3rd ed., University Science Books +** (2013). +** +** Klioner, Sergei A., "A practical relativistic model for micro- +** arcsecond astrometry in space", Astr. J. 125, 1580-1597 (2003). +** +** Called: +** eraS2c spherical coordinates to unit vector +** eraLdsun light deflection due to Sun +** eraAb stellar aberration +** eraRxp product of r-matrix and p-vector +** eraC2s p-vector to spherical +** eraAnp normalize angle into range +/- pi +** +** Copyright (C) 2013-2016, NumFOCUS Foundation. +** Derived, with permission, from the SOFA library. See notes at end of file. +*/ +{ + double pco[3], pnat[3], ppr[3], pi[3], w; + + +/* BCRS coordinate direction (unit vector). */ + eraS2c(rc, dc, pco); + +/* Light deflection by the Sun, giving BCRS natural direction. */ + eraLdsun(pco, astrom->eh, astrom->em, pnat); + +/* Aberration, giving GCRS proper direction. */ + eraAb(pnat, astrom->v, astrom->em, astrom->bm1, ppr); + +/* Bias-precession-nutation, giving CIRS proper direction. */ + eraRxp(astrom->bpn, ppr, pi); + +/* CIRS RA,Dec. */ + eraC2s(pi, &w, di); + *ri = eraAnp(w); + +/* Finished. */ + +} +/*---------------------------------------------------------------------- +** +** +** Copyright (C) 2013-2016, NumFOCUS Foundation. +** All rights reserved. +** +** This library is derived, with permission, from the International +** Astronomical Union's "Standards of Fundamental Astronomy" library, +** available from http://www.iausofa.org. +** +** The ERFA version is intended to retain identical functionality to +** the SOFA library, but made distinct through different function and +** file names, as set out in the SOFA license conditions. The SOFA +** original has a role as a reference standard for the IAU and IERS, +** and consequently redistribution is permitted only in its unaltered +** state. The ERFA version is not subject to this restriction and +** therefore can be included in distributions which do not support the +** concept of "read only" software. +** +** Although the intent is to replicate the SOFA API (other than +** replacement of prefix names) and results (with the exception of +** bugs; any that are discovered will be fixed), SOFA is not +** responsible for any errors found in this version of the library. +** +** If you wish to acknowledge the SOFA heritage, please acknowledge +** that you are using a library derived from SOFA, rather than SOFA +** itself. +** +** +** TERMS AND CONDITIONS +** +** Redistribution and use in source and binary forms, with or without +** modification, are permitted provided that the following conditions +** are met: +** +** 1 Redistributions of source code must retain the above copyright +** notice, this list of conditions and the following disclaimer. +** +** 2 Redistributions in binary form must reproduce the above copyright +** notice, this list of conditions and the following disclaimer in +** the documentation and/or other materials provided with the +** distribution. +** +** 3 Neither the name of the Standards Of Fundamental Astronomy Board, +** the International Astronomical Union nor the names of its +** contributors may be used to endorse or promote products derived +** from this software without specific prior written permission. +** +** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS +** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT +** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS +** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE +** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT, +** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, +** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; +** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER +** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT +** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN +** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE +** POSSIBILITY OF SUCH DAMAGE. +** +*/ |