#include "sofam.h"
 
void iauPn06a(double date1, double date2,
              double *dpsi, double *deps, double *epsa,
              double rb[3][3], double rp[3][3], double rbp[3][3],
              double rn[3][3], double rbpn[3][3])
/*
**  - - - - - - - - -
**   i a u P n 0 6 a
**  - - - - - - - - -
**
**  Precession-nutation, IAU 2006/2000A models:  a multi-purpose function,
**  supporting classical (equinox-based) use directly and CIO-based use
**  indirectly.
**
**  This function is part of the International Astronomical Union's
**  SOFA (Standards Of Fundamental Astronomy) software collection.
**
**  Status:  support function.
**
**  Given:
**     date1,date2  double          TT as a 2-part Julian Date (Note 1)
**
**  Returned:
**     dpsi,deps    double          nutation (Note 2)
**     epsa         double          mean obliquity (Note 3)
**     rb           double[3][3]    frame bias matrix (Note 4)
**     rp           double[3][3]    precession matrix (Note 5)
**     rbp          double[3][3]    bias-precession matrix (Note 6)
**     rn           double[3][3]    nutation matrix (Note 7)
**     rbpn         double[3][3]    GCRS-to-true matrix (Notes 8,9)
**
**  Notes:
**
**  1)  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.
**
**  2)  The nutation components (luni-solar + planetary, IAU 2000A) in
**      longitude and obliquity are in radians and with respect to the
**      equinox and ecliptic of date.  Free core nutation is omitted;
**      for the utmost accuracy, use the iauPn06 function, where the
**      nutation components are caller-specified.
**
**  3)  The mean obliquity is consistent with the IAU 2006 precession.
**
**  4)  The matrix rb transforms vectors from GCRS to mean J2000 by
**      applying frame bias.
**
**  5)  The matrix rp transforms vectors from mean J2000 to mean of date
**      by applying precession.
**
**  6)  The matrix rbp transforms vectors from GCRS to mean of date by
**      applying frame bias then precession.  It is the product rp x rb.
**
**  7)  The matrix rn transforms vectors from mean of date to true of
**      date by applying the nutation (luni-solar + planetary).
**
**  8)  The matrix rbpn transforms vectors from GCRS to true of date
**      (CIP/equinox).  It is the product rn x rbp, applying frame bias,
**      precession and nutation in that order.
**
**  9)  The X,Y,Z coordinates of the IAU 2006/2000A Celestial
**      Intermediate Pole are elements (1,1-3) of the matrix rbpn.
**
**  10) It is permissible to re-use the same array in the returned
**      arguments.  The arrays are filled in the stated order.
**
**  Called:
**     iauNut06a    nutation, IAU 2006/2000A
**     iauPn06      bias/precession/nutation results, IAU 2006
**
**  Reference:
**
**     Capitaine, N. & Wallace, P.T., 2006, Astron.Astrophys. 450, 855
**
**  This revision:  2008 November 18
**
**  Copyright (C) 2008 IAU SOFA Review Board.  See notes at end.
*/
{
/* Nutation. */
   iauNut06a(date1, date2, dpsi, deps);
 
/* Remaining results. */
   iauPn06(date1, date2, *dpsi, *deps, epsa, rb, rp, rbp, rn, rbpn);
 
   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
**
**---------------------------------------------------------------------*/
}