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author | William Joye <wjoye@cfa.harvard.edu> | 2018-01-09 19:06:17 (GMT) |
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committer | William Joye <wjoye@cfa.harvard.edu> | 2018-01-09 19:06:17 (GMT) |
commit | d64cf9c0bd23e752867b149be636d1bbd4501cf4 (patch) | |
tree | ec600c696fe3dbf15f166d22a95c47a1c0867509 /ast/erfa/a2af.c | |
parent | 62d555c8f989ab6eb026387cbf52bb46ebb2dfea (diff) | |
download | blt-d64cf9c0bd23e752867b149be636d1bbd4501cf4.zip blt-d64cf9c0bd23e752867b149be636d1bbd4501cf4.tar.gz blt-d64cf9c0bd23e752867b149be636d1bbd4501cf4.tar.bz2 |
update ast 8.6.2
Diffstat (limited to 'ast/erfa/a2af.c')
-rw-r--r-- | ast/erfa/a2af.c | 129 |
1 files changed, 0 insertions, 129 deletions
diff --git a/ast/erfa/a2af.c b/ast/erfa/a2af.c deleted file mode 100644 index 0101630..0000000 --- a/ast/erfa/a2af.c +++ /dev/null @@ -1,129 +0,0 @@ -#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) 2013-2016, 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) 2013-2016, 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. -** -*/ |