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erfasrc/src/taiutc.c  view on Meta::CPAN

**  Returned (function value):
**                int      status: +1 = dubious year (Note 4)
**                                  0 = OK
**                                 -1 = unacceptable date
**
**  Notes:
**
**  1) tai1+tai2 is Julian Date, apportioned in any convenient way
**     between the two arguments, for example where tai1 is the Julian
**     Day Number and tai2 is the fraction of a day.  The returned utc1
**     and utc2 form an analogous pair, except that a special convention
**     is used, to deal with the problem of leap seconds - see the next
**     note.
**
**  2) JD cannot unambiguously represent UTC during a leap second unless
**     special measures are taken.  The convention in the present
**     function is that the JD day represents UTC days whether the
**     length is 86399, 86400 or 86401 SI seconds.  In the 1960-1972 era
**     there were smaller jumps (in either direction) each time the
**     linear UTC(TAI) expression was changed, and these "mini-leaps"
**     are also included in the ERFA convention.
**
**  3) The function eraD2dtf can be used to transform the UTC quasi-JD
**     into calendar date and clock time, including UTC leap second
**     handling.
**
**  4) The warning status "dubious year" flags UTCs that predate the
**     introduction of the time scale or that are too far in the future
**     to be trusted.  See eraDat for further details.
**
**  Called:
**     eraUtctai    UTC to TAI
**
**  References:
**
**     McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
**     IERS Technical Note No. 32, BKG (2004)
**
**     Explanatory Supplement to the Astronomical Almanac,
**     P. Kenneth Seidelmann (ed), University Science Books (1992)
**
**  Copyright (C) 2013-2020, NumFOCUS Foundation.
**  Derived, with permission, from the SOFA library.  See notes at end of file.
*/
{
   int big1;
   int i, j;
   double a1, a2, u1, u2, g1, g2;


/* Put the two parts of the TAI into big-first order. */
   big1 = ( fabs(tai1) >= fabs(tai2) );
   if ( big1 ) {
      a1 = tai1;
      a2 = tai2;
   } else {
      a1 = tai2;
      a2 = tai1;
   }

/* Initial guess for UTC. */
   u1 = a1;
   u2 = a2;

/* Iterate (though in most cases just once is enough). */
   for ( i = 0; i < 3; i++ ) {

   /* Guessed UTC to TAI. */
      j = eraUtctai(u1, u2, &g1, &g2);
      if ( j < 0 ) return j;

   /* Adjust guessed UTC. */
      u2 += a1 - g1;
      u2 += a2 - g2;
   }

/* Return the UTC result, preserving the TAI order. */
   if ( big1 ) {
      *utc1 = u1;
      *utc2 = u2;
   } else {
      *utc1 = u2;
      *utc2 = u1;
   }

/* Status. */
   return j;

}
/*----------------------------------------------------------------------
**  
**  
**  Copyright (C) 2013-2020, NumFOCUS Foundation.
**  All rights reserved.
**  
**  This library is derived, with permission, from the International
**  Astronomical Union's "Standards of Fundamental Astronomy" library,
**  available from http://www.iausofa.org.
**  
**  The ERFA version is intended to retain identical functionality to
**  the SOFA library, but made distinct through different function and
**  file names, as set out in the SOFA license conditions.  The SOFA
**  original has a role as a reference standard for the IAU and IERS,
**  and consequently redistribution is permitted only in its unaltered
**  state.  The ERFA version is not subject to this restriction and
**  therefore can be included in distributions which do not support the
**  concept of "read only" software.
**  
**  Although the intent is to replicate the SOFA API (other than
**  replacement of prefix names) and results (with the exception of
**  bugs;  any that are discovered will be fixed), SOFA is not
**  responsible for any errors found in this version of the library.
**  
**  If you wish to acknowledge the SOFA heritage, please acknowledge
**  that you are using a library derived from SOFA, rather than SOFA
**  itself.
**  
**  
**  TERMS AND CONDITIONS
**  
**  Redistribution and use in source and binary forms, with or without
**  modification, are permitted provided that the following conditions
**  are met:
**  
**  1 Redistributions of source code must retain the above copyright
**    notice, this list of conditions and the following disclaimer.
**  
**  2 Redistributions in binary form must reproduce the above copyright
**    notice, this list of conditions and the following disclaimer in
**    the documentation and/or other materials provided with the
**    distribution.
**