#include "erfa.h" int eraTaiutc(double tai1, double tai2, double *utc1, double *utc2) /* ** - - - - - - - - - - ** e r a T a i u t c ** - - - - - - - - - - ** ** Time scale transformation: International Atomic Time, TAI, to ** Coordinated Universal Time, UTC. ** ** Given: ** tai1,tai2 double TAI as a 2-part Julian Date (Note 1) ** ** Returned: ** utc1,utc2 double UTC as a 2-part quasi Julian Date (Notes 1-3) ** ** 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) 2013-2017, 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 = ( tai1 >= 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) 2013-2017, 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. ** ** 3 Neither the name of the Standards Of Fundamental Astronomy Board, ** the International Astronomical Union nor the names of its ** contributors may be used to endorse or promote products derived ** from this software without specific prior written permission. ** ** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS ** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT ** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS ** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. 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