#include "erfa.h" void eraA2af(int ndp, double angle, char *sign, int idmsf[4]) /* ** - - - - - - - - ** e r a A 2 a f ** - - - - - - - - ** ** Decompose radians into degrees, arcminutes, arcseconds, fraction. ** ** Given: ** ndp int resolution (Note 1) ** angle double angle in radians ** ** Returned: ** sign char '+' or '-' ** idmsf int[4] degrees, arcminutes, arcseconds, fraction ** ** Called: ** eraD2tf decompose days to hms ** ** Notes: ** ** 1) The argument ndp is interpreted as follows: ** ** ndp resolution ** : ...0000 00 00 ** -7 1000 00 00 ** -6 100 00 00 ** -5 10 00 00 ** -4 1 00 00 ** -3 0 10 00 ** -2 0 01 00 ** -1 0 00 10 ** 0 0 00 01 ** 1 0 00 00.1 ** 2 0 00 00.01 ** 3 0 00 00.001 ** : 0 00 00.000... ** ** 2) The largest positive useful value for ndp is determined by the ** size of angle, the format of doubles on the target platform, and ** the risk of overflowing idmsf[3]. On a typical platform, for ** angle up to 2pi, the available floating-point precision might ** correspond to ndp=12. However, the practical limit is typically ** ndp=9, set by the capacity of a 32-bit int, or ndp=4 if int is ** only 16 bits. ** ** 3) The absolute value of angle may exceed 2pi. In cases where it ** does not, it is up to the caller to test for and handle the ** case where angle is very nearly 2pi and rounds up to 360 degrees, ** by testing for idmsf[0]=360 and setting idmsf[0-3] to zero. ** ** Copyright (C) 2013-2017, NumFOCUS Foundation. ** Derived, with permission, from the SOFA library. See notes at end of file. */ { /* Hours to degrees * radians to turns */ const double F = 15.0 / ERFA_D2PI; /* Scale then use days to h,m,s function. */ eraD2tf(ndp, angle*F, sign, idmsf); return; } /*---------------------------------------------------------------------- ** ** ** 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. ** */