      DOUBLE PRECISION FUNCTION iau_GMST82 ( DJ1, DJ2 )
*+
*  - - - - - - - - - - -
*   i a u _ G M S T 8 2
*  - - - - - - - - - - -
*
*  Universal Time to Greenwich Mean Sidereal Time (IAU 1982 model).
*
*  This routine is part of the International Astronomical Union's
*  SOFA (Standards of Fundamental Astronomy) software collection.
*
*  Status:  canonical model.
*
*  Given:
*     DJ1, DJ2     d      UT1 Julian Date (see note)
*
*  Returned:
*     iau_GMST82   d      Greenwich mean sidereal time (radians)
*
*  Notes:
*
*  1) The UT1 epoch DJ1+DJ2 is a Julian Date, apportioned in any
*     convenient way between the arguments DJ1 and DJ2.  For example,
*     JD(UT1)=2450123.7 could be expressed in any of these ways,
*     among others:
*
*             DJ1            DJ2
*
*         2450123.7D0        0D0        (JD method)
*          2451545D0      -1421.3D0     (J2000 method)
*         2400000.5D0     50123.2D0     (MJD method)
*         2450123.5D0       0.2D0       (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 and MJD methods are good compromises
*     between resolution and convenience.  The date & time method is
*     best matched to the algorithm used:  maximum accuracy (or, at
*     least, minimum noise) is delivered when the DJ1 argument is for
*     0hrs UT1 on the day in question and the DJ2 argument lies in the
*     range 0 to 1, or vice versa.
*
*  2) The algorithm is based on the IAU 1982 expression.  This is always
*     described as giving the GMST at 0 hours UT1.  In fact, it gives the
*     difference between the GMST and the UT, the steady 4-minutes-per-day
*     drawing-ahead of ST with respect to UT.  When whole days are ignored,
*     the expression happens to equal the GMST at 0 hours UT1 each day.
*
*  3) In this routine, the entire UT1 (the sum of the two arguments DJ1
*     and DJ2) is used directly as the argument for the standard formula,
*     the constant term of which is adjusted by 12 hours to take account
*     of the noon phasing of Julian Date.  The UT1 is then added, but
*     omitting whole days to conserve accuracy.
*
*  4) The result is returned in the range 0 to 2pi.
*
*  Called:
*     iau_ANP      normalize angle into range 0 to 2pi
*
*  References:
*
*     Transactions of the International Astronomical Union,
*     XVIII B, 67 (1983).
*
*     Aoki et al., Astron. Astrophys. 105, 359-361 (1982).
*
*  This revision:  2008 May 24
*
*  Copyright (C) 2008 IAU SOFA Review Board.  See notes at end.
*
*-----------------------------------------------------------------------

      IMPLICIT NONE

      DOUBLE PRECISION DJ1, DJ2

      DOUBLE PRECISION DS2R
      PARAMETER ( DS2R = 7.272205216643039903848712D-5 )

*  Reference epoch (J2000), JD
      DOUBLE PRECISION DJ00
      PARAMETER ( DJ00 = 2451545D0 )

*  Seconds per day, days per Julian century
      DOUBLE PRECISION D2S, DJC
      PARAMETER ( D2S = 86400D0, DJC = 36525D0 )

*  Coefficients of IAU 1982 GMST-UT1 model
      DOUBLE PRECISION A, B, C, D
      PARAMETER ( A = 24110.54841D0 - D2S/2D0,
     :            B = 8640184.812866D0,
     :            C = 0.093104D0,
     :            D = -6.2D-6 )

*  Note: the first constant, A, has to be adjusted by 12 hours because
*  the UT1 is supplied as a Julian date, which begins at noon.

      DOUBLE PRECISION D1, D2, T, F

      DOUBLE PRECISION iau_ANP

* - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -

*  Julian centuries since fundamental epoch.
      IF ( DJ1 .LT. DJ2 ) THEN
         D1 = DJ1
         D2 = DJ2
      ELSE
         D1 = DJ2
         D2 = DJ1
      END IF
      T = ( D1 + ( D2-DJ00 ) ) / DJC

*  Fractional part of JD(UT1), in seconds.
      F = D2S * ( MOD(D1,1D0) + MOD(D2,1D0) )

*  GMST at this UT1.
      iau_GMST82 = iau_ANP ( DS2R * ( (A+(B+(C+D*T)*T)*T) + F ) )

*  Finished.

*+-----------------------------------------------------------------------
*
*  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
*
*-----------------------------------------------------------------------

      END
