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palDtps2c.c
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palDtps2c.c
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/*
*+
* Name:
* palDtps2c
* Purpose:
* Determine RA,Dec of tangent point from coordinates
* Language:
* Starlink ANSI C
* Type of Module:
* Library routine
* Invocation:
* palDtps2c( double xi, double eta, double ra, double dec,
* double * raz1, double decz1,
* double * raz2, double decz2, int *n);
* Arguments:
* xi = double (Given)
* First rectangular coordinate on tangent plane (radians)
* eta = double (Given)
* Second rectangular coordinate on tangent plane (radians)
* ra = double (Given)
* RA spherical coordinate of star (radians)
* dec = double (Given)
* Dec spherical coordinate of star (radians)
* raz1 = double * (Returned)
* RA spherical coordinate of tangent point, solution 1 (radians)
* decz1 = double * (Returned)
* Dec spherical coordinate of tangent point, solution 1 (radians)
* raz2 = double * (Returned)
* RA spherical coordinate of tangent point, solution 2 (radians)
* decz2 = double * (Returned)
* Dec spherical coordinate of tangent point, solution 2 (radians)
* n = int * (Returned)
* number of solutions: 0 = no solutions returned (note 2)
* 1 = only the first solution is useful (note 3)
* 2 = both solutions are useful (note 3)
* Description:
* From the tangent plane coordinates of a star of known RA,Dec,
* determine the RA,Dec of the tangent point.
* Authors:
* PTW: Pat Wallace (STFC)
* TIMJ: Tim Jenness (JAC, Hawaii)
* {enter_new_authors_here}
* Notes:
* - The RAZ1 and RAZ2 values are returned in the range 0-2pi.
* - Cases where there is no solution can only arise near the poles.
* For example, it is clearly impossible for a star at the pole
* itself to have a non-zero XI value, and hence it is
* meaningless to ask where the tangent point would have to be
* to bring about this combination of XI and DEC.
* - Also near the poles, cases can arise where there are two useful
* solutions. The argument N indicates whether the second of the
* two solutions returned is useful. N=1 indicates only one useful
* solution, the usual case; under these circumstances, the second
* solution corresponds to the "over-the-pole" case, and this is
* reflected in the values of RAZ2 and DECZ2 which are returned.
* - The DECZ1 and DECZ2 values are returned in the range +/-pi, but
* in the usual, non-pole-crossing, case, the range is +/-pi/2.
* - This routine is the spherical equivalent of the routine sla_DTPV2C.
* History:
* 2012-02-08 (TIMJ):
* Initial version with documentation taken from Fortran SLA
* 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 Lesser 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 Lesser General Public License for more details.
*
* You should have received a copy of the GNU Lesser General
* License along with this program. If not, see
* <http://www.gnu.org/licenses/>.
* Bugs:
* {note_any_bugs_here}
*-
*/
#include "pal.h"
#include "pal1sofa.h"
#include <math.h>
void
palDtps2c( double xi, double eta, double ra, double dec,
double * raz1, double * decz1,
double * raz2, double * decz2, int *n) {
double x2;
double y2;
double sd;
double cd;
double sdf;
double r2;
x2 = xi * xi;
y2 = eta * eta;
sd = sin(dec);
cd = cos(dec);
sdf = sd * sqrt(x2 + 1. + y2);
r2 = cd * cd * (y2 + 1.) - sd * sd * x2;
if (r2 >= 0.) {
double r;
double s;
double c;
r = sqrt(r2);
s = sdf - eta * r;
c = sdf * eta + r;
if (xi == 0. && r == 0.) {
r = 1.;
}
*raz1 = eraAnp(ra - atan2(xi, r));
*decz1 = atan2(s, c);
r = -r;
s = sdf - eta * r;
c = sdf * eta + r;
*raz2 = eraAnp(ra - atan2(xi, r));
*decz2 = atan2(s, c);
if (fabs(sdf) < 1.) {
*n = 1;
} else {
*n = 2;
}
} else {
*n = 0;
}
return;
}