Astro-PAL
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erfasrc/src/jd2cal.c view on Meta::CPAN
#include "erfa.h"
#include <float.h>
int eraJd2cal(double dj1, double dj2,
int *iy, int *im, int *id, double *fd)
/*
** - - - - - - - - - -
** e r a J d 2 c a l
** - - - - - - - - - -
**
** Julian Date to Gregorian year, month, day, and fraction of a day.
**
** Given:
** dj1,dj2 double Julian Date (Notes 1, 2)
**
** Returned (arguments):
** iy int year
** im int month
** id int day
** fd double fraction of day
**
** Returned (function value):
** int status:
** 0 = OK
** -1 = unacceptable date (Note 1)
**
** Notes:
**
** 1) The earliest valid date is -68569.5 (-4900 March 1). The
** largest value accepted is 1e9.
**
** 2) The Julian Date is apportioned in any convenient way between
** the arguments dj1 and dj2. For example, JD=2450123.7 could
** be expressed in any of these ways, among others:
**
** dj1 dj2
**
** 2450123.7 0.0 (JD method)
** 2451545.0 -1421.3 (J2000 method)
** 2400000.5 50123.2 (MJD method)
** 2450123.5 0.2 (date & time method)
**
** Separating integer and fraction uses the "compensated summation"
** algorithm of Kahan-Neumaier to preserve as much precision as
** possible irrespective of the jd1+jd2 apportionment.
**
** 3) In early eras the conversion is from the "proleptic Gregorian
** calendar"; no account is taken of the date(s) of adoption of
** the Gregorian calendar, nor is the AD/BC numbering convention
** observed.
**
** References:
**
** Explanatory Supplement to the Astronomical Almanac,
** P. Kenneth Seidelmann (ed), University Science Books (1992),
** Section 12.92 (p604).
**
** Klein, A., A Generalized Kahan-Babuska-Summation-Algorithm.
** Computing 76, 279-293 (2006), Section 3.
**
** Copyright (C) 2013-2020, NumFOCUS Foundation.
** Derived, with permission, from the SOFA library. See notes at end of file.
*/
{
/* Minimum and maximum allowed JD */
const double DJMIN = -68569.5;
const double DJMAX = 1e9;
long jd, i, l, n, k;
double dj, f1, f2, d, s, cs, v[2], x, t, f;
/* Verify date is acceptable. */
dj = dj1 + dj2;
if (dj < DJMIN || dj > DJMAX) return -1;
/* Separate day and fraction (where -0.5 <= fraction < 0.5). */
d = ERFA_DNINT(dj1);
f1 = dj1 - d;
jd = (long) d;
d = ERFA_DNINT(dj2);
f2 = dj2 - d;
jd += (long) d;
/* Compute f1+f2+0.5 using compensated summation (Klein 2006). */
s = 0.5;
cs = 0.0;
v[0] = f1;
v[1] = f2;
for ( i = 0; i < 2; i++ ) {
x = v[i];
t = s + x;
cs += fabs(s) >= fabs(x) ? (s-t) + x : (x-t) + s;
s = t;
if ( s >= 1.0 ) {
jd++;
s -= 1.0;
}
}
f = s + cs;
cs = f - s;
/* Deal with negative f. */
if ( f < 0.0 ) {
/* Compensated summation: assume that |s| <= 1.0. */
f = s + 1.0;
cs += (1.0-f) + s;
s = f;
f = s + cs;
cs = f - s;
jd--;
}
/* Deal with f that is 1.0 or more (when rounded to double). */
if ( (f-1.0) >= -DBL_EPSILON/4.0 ) {
/* Compensated summation: assume that |s| <= 1.0. */
t = s - 1.0;
cs += (s-t) - 1.0;
s = t;
f = s + cs;
if ( -DBL_EPSILON/2.0 < f ) {
jd++;
f = ERFA_GMAX(f, 0.0);
}
}
/* Express day in Gregorian calendar. */
l = jd + 68569L;
n = (4L * l) / 146097L;
l -= (146097L * n + 3L) / 4L;
i = (4000L * (l + 1L)) / 1461001L;
l -= (1461L * i) / 4L - 31L;
k = (80L * l) / 2447L;
*id = (int) (l - (2447L * k) / 80L);
l = k / 11L;
*im = (int) (k + 2L - 12L * l);
*iy = (int) (100L * (n - 49L) + i + l);
*fd = f;
return 0;
}
/*----------------------------------------------------------------------
**
**
** Copyright (C) 2013-2020, 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
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