#include "sofa.h" #include "sofam.h" void iauAb(double pnat[3], double v[3], double s, double bm1, double ppr[3]) /* ** - - - - - - ** i a u A b ** - - - - - - ** ** Apply aberration to transform natural direction into proper ** direction. ** ** This function is part of the International Astronomical Union's ** SOFA (Standards of Fundamental Astronomy) software collection. ** ** Status: support function. ** ** Given: ** pnat double[3] natural direction to the source (unit vector) ** v double[3] observer barycentric velocity in units of c ** s double distance between the Sun and the observer (au) ** bm1 double sqrt(1-|v|^2): reciprocal of Lorenz factor ** ** Returned: ** ppr double[3] proper direction to source (unit vector) ** ** Notes: ** ** 1) The algorithm is based on Expr. (7.40) in the Explanatory ** Supplement (Urban & Seidelmann 2013), but with the following ** changes: ** ** o Rigorous rather than approximate normalization is applied. ** ** o The gravitational potential term from Expr. (7) in ** Klioner (2003) is added, taking into account only the Sun's ** contribution. This has a maximum effect of about ** 0.4 microarcsecond. ** ** 2) In almost all cases, the maximum accuracy will be limited by the ** supplied velocity. For example, if the SOFA iauEpv00 function is ** used, errors of up to 5 microarcseconds could occur. ** ** 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: ** iauPdp scalar product of two p-vectors ** ** This revision: 2021 February 24 ** ** SOFA release 2023-10-11 ** ** Copyright (C) 2023 IAU SOFA Board. See notes at end. */ { int i; double pdv, w1, w2, r2, w, p[3], r; pdv = iauPdp(pnat, v); w1 = 1.0 + pdv/(1.0 + bm1); w2 = SRS/s; r2 = 0.0; for (i = 0; i < 3; i++) { w = pnat[i]*bm1 + w1*v[i] + w2*(v[i] - pdv*pnat[i]); p[i] = w; r2 = r2 + w*w; } r = sqrt(r2); for (i = 0; i < 3; i++) { ppr[i] = p[i]/r; } /* Finished. */ /*---------------------------------------------------------------------- ** ** Copyright (C) 2023 ** Standards of Fundamental Astronomy Board ** of the International Astronomical Union. ** ** ===================== ** SOFA Software License ** ===================== ** ** NOTICE TO USER: ** ** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND ** CONDITIONS WHICH APPLY TO ITS USE. ** ** 1. The Software is owned by the IAU SOFA Board ("SOFA"). ** ** 2. Permission is granted to anyone to use the SOFA software for any ** purpose, including commercial applications, free of charge and ** without payment of royalties, subject to the conditions and ** restrictions listed below. ** ** 3. You (the user) may copy and distribute SOFA source code to others, ** and use and adapt its code and algorithms in your own software, ** on a world-wide, royalty-free basis. That portion of your ** distribution that does not consist of intact and unchanged copies ** of SOFA source code files is a "derived work" that must comply ** with the following requirements: ** ** a) Your work shall be marked or carry a statement that it ** (i) uses routines and computations derived by you from ** software provided by SOFA under license to you; and ** (ii) does not itself constitute software provided by and/or ** endorsed by SOFA. ** ** b) The source code of your derived work must contain descriptions ** of how the derived work is based upon, contains and/or differs ** from the original SOFA software. ** ** c) The names of all routines in your derived work shall not ** include the prefix "iau" or "sofa" or trivial modifications ** thereof such as changes of case. ** ** d) The origin of the SOFA components of your derived work must ** not be misrepresented; you must not claim that you wrote the ** original software, nor file a patent application for SOFA ** software or algorithms embedded in the SOFA software. ** ** e) These requirements must be reproduced intact in any source ** distribution and shall apply to anyone to whom you have ** granted a further right to modify the source code of your ** derived work. ** ** Note that, as originally distributed, the SOFA software is ** intended to be a definitive implementation of the IAU standards, ** and consequently third-party modifications are discouraged. All ** variations, no matter how minor, must be explicitly marked as ** such, as explained above. ** ** 4. You shall not cause the SOFA software to be brought into ** disrepute, either by misuse, or use for inappropriate tasks, or ** by inappropriate modification. ** ** 5. The SOFA software is provided "as is" and SOFA makes no warranty ** as to its use or performance. SOFA does not and cannot warrant ** the performance or results which the user may obtain by using the ** SOFA software. SOFA makes no warranties, express or implied, as ** to non-infringement of third party rights, merchantability, or ** fitness for any particular purpose. In no event will SOFA be ** liable to the user for any consequential, incidental, or special ** damages, including any lost profits or lost savings, even if a ** SOFA representative has been advised of such damages, or for any ** claim by any third party. ** ** 6. The provision of any version of the SOFA software under the terms ** and conditions specified herein does not imply that future ** versions will also be made available under the same terms and ** conditions. * ** In any published work or commercial product which uses the SOFA ** software directly, acknowledgement (see www.iausofa.org) is ** appreciated. ** ** Correspondence concerning SOFA software should be addressed as ** follows: ** ** By email: sofa@ukho.gov.uk ** By post: IAU SOFA Center ** HM Nautical Almanac Office ** UK Hydrographic Office ** Admiralty Way, Taunton ** Somerset, TA1 2DN ** United Kingdom ** **--------------------------------------------------------------------*/ }