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palGe50.c
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palGe50.c
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/*
*+
* Name:
* palGe50
* Purpose:
* Transform Galactic Coordinate to B1950 FK4
* Language:
* Starlink ANSI C
* Type of Module:
* Library routine
* Invocation:
* palGe50( double dl, double db, double *dr, double *dd );
* Arguments:
* dl = double (Given)
* Galactic longitude (radians)
* db = double (Given)
* Galactic latitude (radians)
* dr = double * (Returned)
* B9150.0 FK4 RA.
* dd = double * (Returned)
* B1950.0 FK4 Dec.
* Description:
* Transformation from IAU 1958 galactic coordinates to
* B1950.0 'FK4' equatorial coordinates.
* Authors:
* PTW: Patrick T. Wallace
* TIMJ: Tim Jenness (JAC, Hawaii)
* {enter_new_authors_here}
* Notes:
* - The equatorial coordinates are B1950.0 'FK4'. Use the routine
* palGaleq if conversion to J2000.0 coordinates is required.
* See Also:
* - Blaauw et al, Mon.Not.R.Astron.Soc.,121,123 (1960)
* History:
* 2012-03-23 (TIMJ):
* Initial version
* Adapted with permission from the Fortran SLALIB library.
* {enter_further_changes_here}
* Copyright:
* Copyright (C) 1995 Rutherford Appleton Laboratory
* Copyright (C) 2012 Science and Technology Facilities Council.
* All Rights Reserved.
* Licence:
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 3 of
* the License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be
* useful, but WITHOUT ANY WARRANTY; without even the implied
* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
* PURPOSE. See the GNU General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston,
* MA 02110-1301, USA.
* Bugs:
* {note_any_bugs_here}
*-
*/
#include "pal.h"
#include "pal1sofa.h"
void palGe50 ( double dl, double db, double * dr, double * dd ) {
/*
* L2,B2 system of galactic coordinates
*
* P = 192.25 RA of galactic north pole (mean B1950.0)
* Q = 62.6 inclination of galactic to mean B1950.0 equator
* R = 33 longitude of ascending node
*
* P,Q,R are degrees
*
*
* Equatorial to galactic rotation matrix
*
* The Euler angles are P, Q, 90-R, about the z then y then
* z axes.
*
* +CP.CQ.SR-SP.CR +SP.CQ.SR+CP.CR -SQ.SR
*
* -CP.CQ.CR-SP.SR -SP.CQ.CR+CP.SR +SQ.CR
*
* +CP.SQ +SP.SQ +CQ
*
*/
double rmat[3][3] = {
{ -0.066988739415,-0.872755765852,-0.483538914632 },
{ +0.492728466075,-0.450346958020,+0.744584633283 },
{ -0.867600811151,-0.188374601723,+0.460199784784 }
};
double v1[3], v2[3], r, d, re, de;
/* Spherical to cartesian */
eraS2c( dl, db, v1 );
/* Rotate to mean B1950.0 */
eraTrxp( rmat, v1, v2 );
/* Cartesian to spherical */
eraC2s( v2, &r, &d );
/* Introduce E-terms */
palAddet( r, d, 1950.0, &re, &de );
/* Express in conventional ranges */
*dr = eraAnp( re );
*dd = eraAnpm( de );
}