#include "sofam.h"
 
void iauPrec76(double ep01, double ep02, double ep11, double ep12,
               double *zeta, double *z, double *theta)
/*
**  - - - - - - - - - -
**   i a u P r e c 7 6
**  - - - - - - - - - -
**
**  IAU 1976 precession model.
**
**  This function forms the three Euler angles which implement general
**  precession between two epochs, using the IAU 1976 model (as for
**  the FK5 catalog).
**
**  This function is part of the International Astronomical Union's
**  SOFA (Standards Of Fundamental Astronomy) software collection.
**
**  Status:  canonical model.
**
**  Given:
**     ep01,ep02   double    TDB starting epoch (Note 1)
**     ep11,ep12   double    TDB ending epoch (Note 1)
**
**  Returned:
**     zeta        double    1st rotation: radians cw around z
**     z           double    3rd rotation: radians cw around z
**     theta       double    2nd rotation: radians ccw around y
**
**  Notes:
**
**  1) The epochs ep01+ep02 and ep11+ep12 are Julian Dates, apportioned
**     in any convenient way between the arguments epn1 and epn2.  For
**     example, JD(TDB)=2450123.7 could be expressed in any of these
**     ways, among others:
**
**             epn1          epn2
**
**         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
**     optimum resolution.  The MJD method and the date & time methods
**     are both good compromises between resolution and convenience.
**     The two epochs may be expressed using different methods, but at
**     the risk of losing some resolution.
**
**  2) The accumulated precession angles zeta, z, theta are expressed
**     through canonical polynomials which are valid only for a limited
**     time span.  In addition, the IAU 1976 precession rate is known to
**     be imperfect.  The absolute accuracy of the present formulation
**     is better than 0.1 arcsec from 1960AD to 2040AD, better than
**     1 arcsec from 1640AD to 2360AD, and remains below 3 arcsec for
**     the whole of the period 500BC to 3000AD.  The errors exceed
**     10 arcsec outside the range 1200BC to 3900AD, exceed 100 arcsec
**     outside 4200BC to 5600AD and exceed 1000 arcsec outside 6800BC to
**     8200AD.
**
**  3) The three angles are returned in the conventional order, which
**     is not the same as the order of the corresponding Euler
**     rotations.  The precession matrix is
**     R_3(-z) x R_2(+theta) x R_3(-zeta).
**
**  Reference:
**
**     Lieske, J.H., 1979, Astron.Astrophys. 73, 282, equations
**     (6) & (7), p283.
**
**  This revision:  2008 May 24
**
**  Copyright (C) 2008 IAU SOFA Review Board.  See notes at end.
*/
{
   double t0, t, tas2r, w;


/* Interval between fundamental epoch J2000.0 and beginning epoch (JC). */
   t0 = ((ep01 - DJ00) + ep02) / DJC;
 
/* Interval over which precession required (JC). */
   t = ((ep11 - ep01) + (ep12 - ep02)) / DJC;
 
/* Euler angles. */
   tas2r = t * DAS2R;
   w = 2306.2181 + (1.39656 - 0.000139 * t0) * t0;
 
   *zeta = (w + ((0.30188 - 0.000344 * t0) + 0.017998 * t) * t) * tas2r;
 
   *z = (w + ((1.09468 + 0.000066 * t0) + 0.018203 * t) * t) * tas2r;
 
   *theta = ((2004.3109 + (-0.85330 - 0.000217 * t0) * t0)
          + ((-0.42665 - 0.000217 * t0) - 0.041833 * t) * t) * tas2r;
 
   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
**
**---------------------------------------------------------------------*/
}