#include "sofa.h"

int iauTpxev(double v[3], double v0[3], double *xi, double *eta)
/*
**  - - - - - - - - -
**   i a u T p x e v
**  - - - - - - - - -
**
**  In the tangent plane projection, given celestial direction cosines
**  for a star and the tangent point, solve for the star's rectangular
**  coordinates in the tangent plane.
**
**  This function is part of the International Astronomical Union's
**  SOFA (Standards of Fundamental Astronomy) software collection.
**
**  Status:  support function.
**
**  Given:
**     v         double[3]  direction cosines of star (Note 4)
**     v0        double[3]  direction cosines of tangent point (Note 4)
**
**  Returned:
**     *xi,*eta  double     tangent plane coordinates of star
**
**  Returned (function value):
**               int        status: 0 = OK
**                                  1 = star too far from axis
**                                  2 = antistar on tangent plane
**                                  3 = antistar too far from axis
**
**  Notes:
**
**  1) The tangent plane projection is also called the "gnomonic
**     projection" and the "central projection".
**
**  2) The eta axis points due north in the adopted coordinate system.
**     If the direction cosines represent observed (RA,Dec), the tangent
**     plane coordinates (xi,eta) are conventionally called the
**     "standard coordinates".  If the direction cosines are with
**     respect to a right-handed triad, (xi,eta) are also right-handed.
**     The units of (xi,eta) are, effectively, radians at the tangent
**     point.
**
**  3) The method used is to extend the star vector to the tangent
**     plane and then rotate the triad so that (x,y) becomes (xi,eta).
**     Writing (a,b) for the celestial spherical coordinates of the
**     star, the sequence of rotations is (a+pi/2) around the z-axis
**     followed by (pi/2-b) around the x-axis.
**
**  4) If vector v0 is not of unit length, or if vector v is of zero
**     length, the results will be wrong.
**
**  5) If v0 points at a pole, the returned (xi,eta) will be based on
**     the arbitrary assumption that the longitude coordinate of the
**     tangent point is zero.
**
**  6) This function is a member of the following set:
**
**         spherical      vector         solve for
**
**         iauTpxes    > iauTpxev <       xi,eta
**         iauTpsts      iauTpstv          star
**         iauTpors      iauTporv         origin
**
**  References:
**
**     Calabretta M.R. & Greisen, E.W., 2002, "Representations of
**     celestial coordinates in FITS", Astron.Astrophys. 395, 1077
**
**     Green, R.M., "Spherical Astronomy", Cambridge University Press,
**     1987, Chapter 13.
**
**  This revision:   2018 January 2
**
**  SOFA release 2018-01-30
**
**  Copyright (C) 2018 IAU SOFA Board.  See notes at end.
*/
{
   const double TINY = 1e-6;
   int j;
   double x, y, z, x0, y0, z0, r2, r, w, d;


/* Star and tangent point. */
   x = v[0];
   y = v[1];
   z = v[2];
   x0 = v0[0];
   y0 = v0[1];
   z0 = v0[2];

/* Deal with polar case. */
   r2 = x0*x0 + y0*y0;
   r = sqrt(r2);
   if ( r == 0.0 ) {
      r = 1e-20;
      x0 = r;
   }

/* Reciprocal of star vector length to tangent plane. */
   w = x*x0 + y*y0;
   d = w + z*z0;

/* Check for error cases. */
   if ( d > TINY ) {
      j = 0;
   } else if ( d >= 0.0 ) {
      j = 1;
      d = TINY;
   } else if ( d > -TINY ) {
      j = 2;
      d = -TINY;
   } else {
      j = 3;
   }

/* Return the tangent plane coordinates (even in dubious cases). */
   d *= r;
   *xi = (y*x0 - x*y0) / d;
   *eta = (z*r2 - z0*w) / d;

/* Return the status. */
   return j;

/* Finished. */

/*----------------------------------------------------------------------
**
**  Copyright (C) 2018
**  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
**
**--------------------------------------------------------------------*/

}