#include "erfa.h" int eraTttdb(double tt1, double tt2, double dtr, double *tdb1, double *tdb2) /* ** - - - - - - - - - ** e r a T t t d b ** - - - - - - - - - ** ** Time scale transformation: Terrestrial Time, TT, to Barycentric ** Dynamical Time, TDB. ** ** Given: ** tt1,tt2 double TT as a 2-part Julian Date ** dtr double TDB-TT in seconds ** ** Returned: ** tdb1,tdb2 double TDB as a 2-part Julian Date ** ** Returned (function value): ** int status: 0 = OK ** ** Notes: ** ** 1) tt1+tt2 is Julian Date, apportioned in any convenient way between ** the two arguments, for example where tt1 is the Julian Day Number ** and tt2 is the fraction of a day. The returned tdb1,tdb2 follow ** suit. ** ** 2) The argument dtr represents the quasi-periodic component of the ** GR transformation between TT and TCB. It is dependent upon the ** adopted solar-system ephemeris, and can be obtained by numerical ** integration, by interrogating a precomputed time ephemeris or by ** evaluating a model such as that implemented in the ERFA function ** eraDtdb. The quantity is dominated by an annual term of 1.7 ms ** amplitude. ** ** 3) TDB is essentially the same as Teph, the time argument for the JPL ** solar system ephemerides. ** ** References: ** ** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003), ** IERS Technical Note No. 32, BKG (2004) ** ** IAU 2006 Resolution 3 ** ** Copyright (C) 2013-2017, NumFOCUS Foundation. ** Derived, with permission, from the SOFA library. See notes at end of file. */ { double dtrd; /* Result, safeguarding precision. */ dtrd = dtr / ERFA_DAYSEC; if ( tt1 > tt2 ) { *tdb1 = tt1; *tdb2 = tt2 + dtrd; } else { *tdb1 = tt1 + dtrd; *tdb2 = tt2; } /* Status (always OK). */ return 0; } /*---------------------------------------------------------------------- ** ** ** 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. ** */