summaryrefslogtreecommitdiffstats
path: root/ast/erfa/d2dtf.c
diff options
context:
space:
mode:
Diffstat (limited to 'ast/erfa/d2dtf.c')
-rw-r--r--ast/erfa/d2dtf.c245
1 files changed, 0 insertions, 245 deletions
diff --git a/ast/erfa/d2dtf.c b/ast/erfa/d2dtf.c
deleted file mode 100644
index 4476970..0000000
--- a/ast/erfa/d2dtf.c
+++ /dev/null
@@ -1,245 +0,0 @@
-#include "erfa.h"
-#include <string.h>
-
-int eraD2dtf(const char *scale, int ndp, double d1, double d2,
- int *iy, int *im, int *id, int ihmsf[4])
-/*
-** - - - - - - - - -
-** e r a D 2 d t f
-** - - - - - - - - -
-**
-** Format for output a 2-part Julian Date (or in the case of UTC a
-** quasi-JD form that includes special provision for leap seconds).
-**
-** Given:
-** scale char[] time scale ID (Note 1)
-** ndp int resolution (Note 2)
-** d1,d2 double time as a 2-part Julian Date (Notes 3,4)
-**
-** Returned:
-** iy,im,id int year, month, day in Gregorian calendar (Note 5)
-** ihmsf int[4] hours, minutes, seconds, fraction (Note 1)
-**
-** Returned (function value):
-** int status: +1 = dubious year (Note 5)
-** 0 = OK
-** -1 = unacceptable date (Note 6)
-**
-** Notes:
-**
-** 1) scale identifies the time scale. Only the value "UTC" (in upper
-** case) is significant, and enables handling of leap seconds (see
-** Note 4).
-**
-** 2) ndp is the number of decimal places in the seconds field, and can
-** have negative as well as positive values, such as:
-**
-** ndp resolution
-** -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
-**
-** The limits are platform dependent, but a safe range is -5 to +9.
-**
-** 3) d1+d2 is Julian Date, apportioned in any convenient way between
-** the two arguments, for example where d1 is the Julian Day Number
-** and d2 is the fraction of a day. In the case of UTC, where the
-** use of JD is problematical, special conventions apply: see the
-** next note.
-**
-** 4) JD cannot unambiguously represent UTC during a leap second unless
-** special measures are taken. The ERFA internal convention is that
-** the quasi-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.
-**
-** 5) 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.
-**
-** 6) For calendar conventions and limitations, see eraCal2jd.
-**
-** Called:
-** eraJd2cal JD to Gregorian calendar
-** eraD2tf decompose days to hms
-** eraDat delta(AT) = TAI-UTC
-**
-** Copyright (C) 2013-2016, NumFOCUS Foundation.
-** Derived, with permission, from the SOFA library. See notes at end of file.
-*/
-{
- int leap;
- char s;
- int iy1, im1, id1, js, iy2, im2, id2, ihmsf1[4], i;
- double a1, b1, fd, dat0, dat12, w, dat24, dleap;
-
-
-/* The two-part JD. */
- a1 = d1;
- b1 = d2;
-
-/* Provisional calendar date. */
- js = eraJd2cal(a1, b1, &iy1, &im1, &id1, &fd);
- if ( js ) return -1;
-
-/* Is this a leap second day? */
- leap = 0;
- if ( ! strcmp(scale,"UTC") ) {
-
- /* TAI-UTC at 0h today. */
- js = eraDat(iy1, im1, id1, 0.0, &dat0);
- if ( js < 0 ) return -1;
-
- /* TAI-UTC at 12h today (to detect drift). */
- js = eraDat(iy1, im1, id1, 0.5, &dat12);
- if ( js < 0 ) return -1;
-
- /* TAI-UTC at 0h tomorrow (to detect jumps). */
- js = eraJd2cal(a1+1.5, b1-fd, &iy2, &im2, &id2, &w);
- if ( js ) return -1;
- js = eraDat(iy2, im2, id2, 0.0, &dat24);
- if ( js < 0 ) return -1;
-
- /* Any sudden change in TAI-UTC (seconds). */
- dleap = dat24 - (2.0*dat12 - dat0);
-
- /* If leap second day, scale the fraction of a day into SI. */
- leap = (dleap != 0.0);
- if (leap) fd += fd * dleap/ERFA_DAYSEC;
- }
-
-/* Provisional time of day. */
- eraD2tf ( ndp, fd, &s, ihmsf1 );
-
-/* Has the (rounded) time gone past 24h? */
- if ( ihmsf1[0] > 23 ) {
-
- /* Yes. We probably need tomorrow's calendar date. */
- js = eraJd2cal(a1+1.5, b1-fd, &iy2, &im2, &id2, &w);
- if ( js ) return -1;
-
- /* Is today a leap second day? */
- if ( ! leap ) {
-
- /* No. Use 0h tomorrow. */
- iy1 = iy2;
- im1 = im2;
- id1 = id2;
- ihmsf1[0] = 0;
- ihmsf1[1] = 0;
- ihmsf1[2] = 0;
-
- } else {
-
- /* Yes. Are we past the leap second itself? */
- if ( ihmsf1[2] > 0 ) {
-
- /* Yes. Use tomorrow but allow for the leap second. */
- iy1 = iy2;
- im1 = im2;
- id1 = id2;
- ihmsf1[0] = 0;
- ihmsf1[1] = 0;
- ihmsf1[2] = 0;
-
- } else {
-
- /* No. Use 23 59 60... today. */
- ihmsf1[0] = 23;
- ihmsf1[1] = 59;
- ihmsf1[2] = 60;
- }
-
- /* If rounding to 10s or coarser always go up to new day. */
- if ( ndp < 0 && ihmsf1[2] == 60 ) {
- iy1 = iy2;
- im1 = im2;
- id1 = id2;
- ihmsf1[0] = 0;
- ihmsf1[1] = 0;
- ihmsf1[2] = 0;
- }
- }
- }
-
-/* Results. */
- *iy = iy1;
- *im = im1;
- *id = id1;
- for ( i = 0; i < 4; i++ ) {
- ihmsf[i] = ihmsf1[i];
- }
-
-/* Status. */
- return js;
-
-}
-/*----------------------------------------------------------------------
-**
-**
-** 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.
-**
-*/