#include "erfa.h" int eraUtctai(double utc1, double utc2, double *tai1, double *tai2) /* ** - - - - - - - - - - ** e r a U t c t a i ** - - - - - - - - - - ** ** Time scale transformation: Coordinated Universal Time, UTC, to ** International Atomic Time, TAI. ** ** Given: ** utc1,utc2 double UTC as a 2-part quasi Julian Date (Notes 1-4) ** ** Returned: ** tai1,tai2 double TAI as a 2-part Julian Date (Note 5) ** ** Returned (function value): ** int status: +1 = dubious year (Note 3) ** 0 = OK ** -1 = unacceptable date ** ** Notes: ** ** 1) utc1+utc2 is quasi Julian Date (see Note 2), apportioned in any ** convenient way between the two arguments, for example where utc1 ** is the Julian Day Number and utc2 is the fraction of a day. ** ** 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 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. ** ** 4) The function eraDtf2d converts from calendar date and time of day ** into 2-part Julian Date, and in the case of UTC implements the ** leap-second-ambiguity convention described above. ** ** 5) The returned TAI1,TAI2 are such that their sum is the TAI Julian ** Date. ** ** Called: ** eraJd2cal JD to Gregorian calendar ** eraDat delta(AT) = TAI-UTC ** eraCal2jd Gregorian calendar to JD ** ** 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 iy, im, id, j, iyt, imt, idt; double u1, u2, fd, dat0, dat12, w, dat24, dlod, dleap, z1, z2, a2; /* Put the two parts of the UTC into big-first order. */ big1 = ( utc1 >= utc2 ); if ( big1 ) { u1 = utc1; u2 = utc2; } else { u1 = utc2; u2 = utc1; } /* Get TAI-UTC at 0h today. */ j = eraJd2cal(u1, u2, &iy, &im, &id, &fd); if ( j ) return j; j = eraDat(iy, im, id, 0.0, &dat0); if ( j < 0 ) return j; /* Get TAI-UTC at 12h today (to detect drift). */ j = eraDat(iy, im, id, 0.5, &dat12); if ( j < 0 ) return j; /* Get TAI-UTC at 0h tomorrow (to detect jumps). */ j = eraJd2cal(u1+1.5, u2-fd, &iyt, &imt, &idt, &w); if ( j ) return j; j = eraDat(iyt, imt, idt, 0.0, &dat24); if ( j < 0 ) return j; /* Separate TAI-UTC change into per-day (DLOD) and any jump (DLEAP). */ dlod = 2.0 * (dat12 - dat0); dleap = dat24 - (dat0 + dlod); /* Remove any scaling applied to spread leap into preceding day. */ fd *= (ERFA_DAYSEC+dleap)/ERFA_DAYSEC; /* Scale from (pre-1972) UTC seconds to SI seconds. */ fd *= (ERFA_DAYSEC+dlod)/ERFA_DAYSEC; /* Today's calendar date to 2-part JD. */ if ( eraCal2jd(iy, im, id, &z1, &z2) ) return -1; /* Assemble the TAI result, preserving the UTC split and order. */ a2 = z1 - u1; a2 += z2; a2 += fd + dat0/ERFA_DAYSEC; if ( big1 ) { *tai1 = u1; *tai2 = a2; } else { *tai1 = a2; *tai2 = 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. IN NO EVENT SHALL THE ** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT, ** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, ** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; ** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER ** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT ** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE ** POSSIBILITY OF SUCH DAMAGE. ** */