| 1 | /* | 
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| 2 | *+ | 
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| 3 | *  Name: | 
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| 4 | *     palEcmat | 
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| 5 |  | 
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| 6 | *  Purpose: | 
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| 7 | *     Form the equatorial to ecliptic rotation matrix - IAU 2006 | 
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| 8 | *     precession model. | 
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| 9 |  | 
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| 10 | *  Language: | 
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| 11 | *     Starlink ANSI C | 
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| 12 |  | 
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| 13 | *  Type of Module: | 
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| 14 | *     Library routine | 
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| 15 |  | 
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| 16 | *  Invocation: | 
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| 17 | *     palEcmat( double date, double rmat[3][3] ) | 
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| 18 |  | 
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| 19 | *  Arguments: | 
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| 20 | *     date = double (Given) | 
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| 21 | *        TT as Modified Julian Date (JD-2400000.5). The difference | 
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| 22 | *        between TT and TDB is of the order of a millisecond or two | 
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| 23 | *        (i.e. about 0.02 arc-seconds). | 
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| 24 | *     rmat = double[3][3] (Returned) | 
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| 25 | *        Rotation matrix | 
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| 26 |  | 
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| 27 | *  Description: | 
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| 28 | *     The equatorial to ecliptic rotation matrix is found and returned. | 
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| 29 | *     The matrix is in the sense   V(ecl)  =  RMAT * V(equ);  the | 
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| 30 | *     equator, equinox and ecliptic are mean of date. | 
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| 31 |  | 
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| 32 | *  Authors: | 
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| 33 | *     PTW: Pat Wallace (STFC) | 
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| 34 | *     DSB: David Berry (JAC, Hawaii) | 
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| 35 | *     {enter_new_authors_here} | 
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| 36 |  | 
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| 37 | *  History: | 
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| 38 | *     2012-02-10 (DSB): | 
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| 39 | *        Initial version with documentation taken from Fortran SLA | 
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| 40 | *        Adapted with permission from the Fortran SLALIB library. | 
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| 41 | *     {enter_further_changes_here} | 
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| 42 |  | 
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| 43 | *  Copyright: | 
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| 44 | *     Copyright (C) 1996 Rutherford Appleton Laboratory | 
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| 45 | *     Copyright (C) 2012 Science and Technology Facilities Council. | 
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| 46 | *     All Rights Reserved. | 
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| 47 |  | 
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| 48 | *  Licence: | 
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| 49 | *     This program is free software: you can redistribute it and/or | 
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| 50 | *     modify it under the terms of the GNU Lesser General Public | 
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| 51 | *     License as published by the Free Software Foundation, either | 
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| 52 | *     version 3 of the License, or (at your option) any later | 
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| 53 | *     version. | 
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| 54 | * | 
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| 55 | *     This program is distributed in the hope that it will be useful, | 
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| 56 | *     but WITHOUT ANY WARRANTY; without even the implied warranty of | 
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| 57 | *     MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE.  See the | 
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| 58 | *     GNU Lesser General Public License for more details. | 
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| 59 | * | 
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| 60 | *     You should have received a copy of the GNU Lesser General | 
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| 61 | *     License along with this program.  If not, see | 
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| 62 | *     <http://www.gnu.org/licenses/>. | 
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| 63 |  | 
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| 64 | *  Bugs: | 
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| 65 | *     {note_any_bugs_here} | 
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| 66 | *- | 
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| 67 | */ | 
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| 68 |  | 
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| 69 | #include "pal.h" | 
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| 70 | #include "palmac.h" | 
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| 71 | #include "pal1sofa.h" | 
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| 72 |  | 
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| 73 | void palEcmat( double date, double rmat[3][3] ) { | 
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| 74 |  | 
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| 75 | /* Mean obliquity (the angle between the ecliptic and mean equator of | 
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| 76 | date). */ | 
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| 77 | double eps0 = eraObl06( PAL__MJD0, date ); | 
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| 78 |  | 
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| 79 | /* Matrix */ | 
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| 80 | palDeuler( "X", eps0, 0.0, 0.0, rmat ); | 
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| 81 |  | 
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| 82 | } | 
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