#include "erfa.h"

void eraLd(double bm, double p[3], double q[3], double e[3],
           double em, double dlim, double p1[3])
/*
**  - - - - - -
**   e r a L d
**  - - - - - -
**
**  Apply light deflection by a solar-system body, as part of
**  transforming coordinate direction into natural direction.
**
**  Given:
**     bm     double     mass of the gravitating body (solar masses)
**     p      double[3]  direction from observer to source (unit vector)
**     q      double[3]  direction from body to source (unit vector)
**     e      double[3]  direction from body to observer (unit vector)
**     em     double     distance from body to observer (au)
**     dlim   double     deflection limiter (Note 4)
**
**  Returned:
**     p1     double[3]  observer to deflected source (unit vector)
**
**  Notes:
**
**  1) The algorithm is based on Expr. (70) in Klioner (2003) and
**     Expr. (7.63) in the Explanatory Supplement (Urban & Seidelmann
**     2013), with some rearrangement to minimize the effects of machine
**     precision.
**
**  2) The mass parameter bm can, as required, be adjusted in order to
**     allow for such effects as quadrupole field.
**
**  3) The barycentric position of the deflecting body should ideally
**     correspond to the time of closest approach of the light ray to
**     the body.
**
**  4) The deflection limiter parameter dlim is phi^2/2, where phi is
**     the angular separation (in radians) between source and body at
**     which limiting is applied.  As phi shrinks below the chosen
**     threshold, the deflection is artificially reduced, reaching zero
**     for phi = 0.
**
**  5) The returned vector p1 is not normalized, but the consequential
**     departure from unit magnitude is always negligible.
**
**  6) The arguments p and p1 can be the same array.
**
**  7) To accumulate total light deflection taking into account the
**     contributions from several bodies, call the present function for
**     each body in succession, in decreasing order of distance from the
**     observer.
**
**  8) For efficiency, validation is omitted.  The supplied vectors must
**     be of unit magnitude, and the deflection limiter non-zero and
**     positive.
**
**  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:
**     eraPdp       scalar product of two p-vectors
**     eraPxp       vector product of two p-vectors
**
**  Copyright (C) 2013-2016, NumFOCUS Foundation.
**  Derived, with permission, from the SOFA library.  See notes at end of file.
*/
{
   int i;
   double qpe[3], qdqpe, w, eq[3], peq[3];


/* q . (q + e). */
   for (i = 0; i < 3; i++) {
      qpe[i] = q[i] + e[i];
   }
   qdqpe = eraPdp(q, qpe);

/* 2 x G x bm / ( em x c^2 x ( q . (q + e) ) ). */
   w = bm * ERFA_SRS / em / ERFA_GMAX(qdqpe,dlim);

/* p x (e x q). */
   eraPxp(e, q, eq);
   eraPxp(p, eq, peq);

/* Apply the deflection. */
   for (i = 0; i < 3; i++) {
      p1[i] = p[i] + w*peq[i];
   }

/* 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,
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**  CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
**  LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
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**  
*/