#include "sofam.h"
 
void iauFk5hz(double r5, double d5, double date1, double date2,
              double *rh, double *dh)
/*
**  - - - - - - - - -
**   i a u F k 5 h z
**  - - - - - - - - -
**
**  Transform an FK5 (J2000) star position into the system of the
**  Hipparcos catalogue, assuming zero Hipparcos proper motion.
**
**  This function is part of the International Astronomical Union's
**  SOFA (Standards Of Fundamental Astronomy) software collection.
**
**  Status:  support function.
**
**  Given:
**     r5            double    FK5 RA (radians), equinox J2000, at date
**     d5            double    FK5 Dec (radians), equinox J2000, at date
**     date1,date2   double    TDB date (Notes 1,2)
**
**  Returned:
**     rh            double    Hipparcos RA (radians)
**     dh            double    Hipparcos Dec (radians)
**
**  Notes:
**
**  1) This function converts a star position from the FK5 system to
**     the Hipparcos system, in such a way that the Hipparcos proper
**     motion is zero.  Because such a star has, in general, a non-zero
**     proper motion in the FK5 system, the function requires the date
**     at which the position in the FK5 system was determined.
**
**  2) The TT date date1+date2 is a Julian Date, apportioned in any
**     convenient way between the two arguments.  For example,
**     JD(TT)=2450123.7 could be expressed in any of these ways,
**     among others:
**
**            date1          date2
**
**         2450123.7           0.0       (JD method)
**         2451545.0       -1421.3       (J2000 method)
**         2400000.5       50123.2       (MJD method)
**         2450123.5           0.2       (date & time method)
**
**     The JD method is the most natural and convenient to use in
**     cases where the loss of several decimal digits of resolution
**     is acceptable.  The J2000 method is best matched to the way
**     the argument is handled internally and will deliver the
**     optimum resolution.  The MJD method and the date & time methods
**     are both good compromises between resolution and convenience.
**
**  3) The FK5 to Hipparcos transformation is modeled as a pure
**     rotation and spin;  zonal errors in the FK5 catalogue are not
**     taken into account.
**
**  4) It was the intention that Hipparcos should be a close
**     approximation to an inertial frame, so that distant objects
**     have zero proper motion;  such objects have (in general)
**     non-zero proper motion in FK5, and this function returns those
**     fictitious proper motions.
**
**  5) The position returned by this function is in the FK5 J2000
**     reference system but at date date1+date2.
**
**  6) See also iauFk52h, iauH2fk5, iauHfk5z.
**
**  Called:
**     iauS2c       spherical coordinates to unit vector
**     iauFk5hip    FK5 to Hipparcos rotation and spin
**     iauSxp       multiply p-vector by scalar
**     iauRv2m      r-vector to r-matrix
**     iauTrxp      product of transpose of r-matrix and p-vector
**     iauPxp       vector product of two p-vectors
**     iauC2s       p-vector to spherical
**     iauAnp       normalize angle into range 0 to 2pi
**
**  Reference:
**
**     F.Mignard & M.Froeschle, 2000, Astron.Astrophys. 354, 732-739.
**
**  This revision:  2008 May 24
**
**  Copyright (C) 2008 IAU SOFA Review Board.  See notes at end.
*/
{
   double t, p5e[3], r5h[3][3], s5h[3], vst[3], rst[3][3], p5[3],
          ph[3], w;


/* Interval from given date to fundamental epoch J2000.0 (JY). */
   t = - ((date1 - DJ00) + date2) / DJY;
 
/* FK5 barycentric position vector. */
   iauS2c(r5, d5, p5e);
 
/* FK5 to Hipparcos orientation matrix and spin vector. */
   iauFk5hip(r5h, s5h);
 
/* Accumulated Hipparcos wrt FK5 spin over that interval. */
   iauSxp(t, s5h, vst);
 
/* Express the accumulated spin as a rotation matrix. */
   iauRv2m(vst, rst);
 
/* Derotate the vector's FK5 axes back to date. */
   iauTrxp(rst, p5e, p5);
 
/* Rotate the vector into the Hipparcos system. */
   iauRxp(r5h, p5, ph);
 
/* Hipparcos vector to spherical. */
   iauC2s(ph, &w, dh);
   *rh = iauAnp(w);
 
   return;

/*-----------------------------------------------------------------------
**
**  Copyright (C) 2008
**  Standards Of Fundamental Astronomy Review Board
**  of the International Astronomical Union.
**
**  =====================
**  SOFA Software License
**  =====================
**
**  NOTICE TO USER:
**
**  BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING TERMS AND CONDITIONS
**  WHICH APPLY TO ITS USE.
**
**  1. The Software is owned by the IAU SOFA Review Board ("the Board").
**
**  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 adapt the SOFA software and its 
**     algorithms for your own purposes and you may copy and distribute
**     a resulting "derived work" to others on a world-wide, royalty-free 
**     basis, provided that the derived work complies 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 contain
**        software provided by SOFA or software that has been distributed
**        by or endorsed by SOFA.
**
**     b) The source code of your derived work must contain descriptions
**        of how the derived work is based upon and/or differs from the
**        original SOFA software.
**
**     c) The name(s) of all routine(s) that you distribute shall differ
**        from the SOFA names, even when the SOFA content has not been
**        otherwise changed.
**
**     d) The routine-naming prefix "iau" shall not be used.
**
**     e) 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.
**
**     f) 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.
**
**  4. In any published work or commercial products which includes
**     results achieved by using the SOFA software, you shall acknowledge
**     that the SOFA software was used in obtaining those results.
**
**  5. You shall not cause the SOFA software to be brought into
**     disrepute, either by misuse, or use for inappropriate tasks, or by
**     inappropriate modification.
**
**  6. The SOFA software is provided "as is" and the Board makes no 
**     warranty as to its use or performance.   The Board does not and 
**     cannot warrant the performance or results which the user may obtain 
**     by using the SOFA software.  The Board 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 the Board be liable to the user for any consequential,
**     incidental, or special damages, including any lost profits or lost
**     savings, even if a Board representative has been advised of such
**     damages, or for any claim by any third party.
**
**  7. 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.
**
**  Correspondence concerning SOFA software should be addressed as
**  follows:
**
**     Internet email: sofa@rl.ac.uk
**     Postal address: IAU SOFA Center
**                     Rutherford Appleton Laboratory
**                     Chilton, Didcot, Oxon OX11 0QX
**                     United Kingdom
**
**---------------------------------------------------------------------*/
}