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#include "erfa.h" |
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int eraJdcalf(int ndp, double dj1, double dj2, int iymdf[4]) |
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/* |
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** - - - - - - - - - - |
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** e r a J d c a l f |
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** - - - - - - - - - - |
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** |
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** Julian Date to Gregorian Calendar, expressed in a form convenient |
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** for formatting messages: rounded to a specified precision. |
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** |
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** Given: |
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** ndp int number of decimal places of days in fraction |
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** dj1,dj2 double dj1+dj2 = Julian Date (Note 1) |
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** |
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** Returned: |
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** iymdf int[4] year, month, day, fraction in Gregorian |
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** calendar |
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** |
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** Returned (function value): |
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** int status: |
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** -1 = date out of range |
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** 0 = OK |
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** +1 = NDP not 0-9 (interpreted as 0) |
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** |
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** Notes: |
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** |
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** 1) The Julian Date is apportioned in any convenient way between |
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** the arguments dj1 and dj2. For example, JD=2450123.7 could |
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** be expressed in any of these ways, among others: |
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** |
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** dj1 dj2 |
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** |
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** 2450123.7 0.0 (JD method) |
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** 2451545.0 -1421.3 (J2000 method) |
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** 2400000.5 50123.2 (MJD method) |
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** 2450123.5 0.2 (date & time method) |
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** |
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** 2) In early eras the conversion is from the "Proleptic Gregorian |
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** Calendar"; no account is taken of the date(s) of adoption of |
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** the Gregorian Calendar, nor is the AD/BC numbering convention |
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** observed. |
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** |
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** 3) Refer to the function eraJd2cal. |
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** |
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** 4) NDP should be 4 or less if internal overflows are to be |
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** avoided on machines which use 16-bit integers. |
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** |
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** Called: |
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** eraJd2cal JD to Gregorian calendar |
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** |
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** Reference: |
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** |
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** Explanatory Supplement to the Astronomical Almanac, |
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** P. Kenneth Seidelmann (ed), University Science Books (1992), |
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** Section 12.92 (p604). |
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** |
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** Copyright (C) 2013-2019, NumFOCUS Foundation. |
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** Derived, with permission, from the SOFA library. See notes at end of file. |
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*/ |
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{ |
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int j, js; |
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double denom, d1, d2, f1, f2, f; |
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/* Denominator of fraction (e.g. 100 for 2 decimal places). */ |
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if ((ndp >= 0) && (ndp <= 9)) { |
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j = 0; |
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denom = pow(10.0, ndp); |
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} else { |
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j = 1; |
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denom = 1.0; |
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} |
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/* Copy the date, big then small, and realign to midnight. */ |
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if (dj1 >= dj2) { |
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d1 = dj1; |
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d2 = dj2; |
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} else { |
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d1 = dj2; |
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d2 = dj1; |
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} |
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d2 -= 0.5; |
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/* Separate days and fractions. */ |
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f1 = fmod(d1, 1.0); |
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f2 = fmod(d2, 1.0); |
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d1 = ERFA_DNINT(d1-f1); |
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d2 = ERFA_DNINT(d2-f2); |
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/* Round the total fraction to the specified number of places. */ |
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f = ERFA_DNINT((f1+f2)*denom) / denom; |
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/* Re-assemble the rounded date and re-align to noon. */ |
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d2 += f + 0.5; |
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/* Convert to Gregorian calendar. */ |
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js = eraJd2cal(d1, d2, &iymdf[0], &iymdf[1], &iymdf[2], &f); |
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if (js == 0) { |
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iymdf[3] = (int) (f * denom); |
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} else { |
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j = js; |
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} |
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/* Return the status. */ |
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return j; |
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} |
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/*---------------------------------------------------------------------- |
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** |
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** |
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** Copyright (C) 2013-2019, NumFOCUS Foundation. |
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** All rights reserved. |
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** |
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** This library is derived, with permission, from the International |
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** Astronomical Union's "Standards of Fundamental Astronomy" library, |
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** available from http://www.iausofa.org. |
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** |
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** The ERFA version is intended to retain identical functionality to |
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** the SOFA library, but made distinct through different function and |
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** file names, as set out in the SOFA license conditions. The SOFA |
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** original has a role as a reference standard for the IAU and IERS, |
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** and consequently redistribution is permitted only in its unaltered |
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** state. The ERFA version is not subject to this restriction and |
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** therefore can be included in distributions which do not support the |
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** concept of "read only" software. |
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** |
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** Although the intent is to replicate the SOFA API (other than |
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** replacement of prefix names) and results (with the exception of |
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** bugs; any that are discovered will be fixed), SOFA is not |
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** responsible for any errors found in this version of the library. |
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** |
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** If you wish to acknowledge the SOFA heritage, please acknowledge |
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** that you are using a library derived from SOFA, rather than SOFA |
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** itself. |
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** |
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** |
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** TERMS AND CONDITIONS |
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** |
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** Redistribution and use in source and binary forms, with or without |
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** modification, are permitted provided that the following conditions |
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** are met: |
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** |
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** 1 Redistributions of source code must retain the above copyright |
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** notice, this list of conditions and the following disclaimer. |
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** |
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** 2 Redistributions in binary form must reproduce the above copyright |
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** notice, this list of conditions and the following disclaimer in |
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** the documentation and/or other materials provided with the |
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** distribution. |
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** |
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** 3 Neither the name of the Standards Of Fundamental Astronomy Board, |
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** the International Astronomical Union nor the names of its |
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** contributors may be used to endorse or promote products derived |
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** from this software without specific prior written permission. |
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** |
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** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS |
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** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT |
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** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS |
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** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE |
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** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT, |
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** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, |
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** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; |
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** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER |
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** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT |
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** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN |
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** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE |
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** POSSIBILITY OF SUCH DAMAGE. |
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** |
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*/ |