jd2cal

erfa.jd2cal(dj1, dj2)[source]

Julian Date to Gregorian year, month, day, and fraction of a day.

Parameters:
dj1double array
dj2double array
Returns:
iyint array
imint array
idint array
fddouble array

Notes

Wraps ERFA function eraJd2cal. The ERFA documentation is:

- - - - - - - - - -
 e r a J d 2 c a l
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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.

This revision:  2021 May 11

Copyright (C) 2013-2023, NumFOCUS Foundation.
Derived, with permission, from the SOFA library.  See notes at end of file.