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author | William Joye <wjoye@cfa.harvard.edu> | 2016-10-26 21:13:00 (GMT) |
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committer | William Joye <wjoye@cfa.harvard.edu> | 2016-10-26 21:13:00 (GMT) |
commit | da2e3d212171bbe64c1af39114fd067308656990 (patch) | |
tree | 9601f7ed15fa1394762124630c12a792bc073ec2 /funtools/wcs/sph.c | |
parent | 76b109ad6d97d19ab835596dc70149ef379f3733 (diff) | |
download | blt-da2e3d212171bbe64c1af39114fd067308656990.zip blt-da2e3d212171bbe64c1af39114fd067308656990.tar.gz blt-da2e3d212171bbe64c1af39114fd067308656990.tar.bz2 |
rm funtools for update
Diffstat (limited to 'funtools/wcs/sph.c')
-rw-r--r-- | funtools/wcs/sph.c | 234 |
1 files changed, 0 insertions, 234 deletions
diff --git a/funtools/wcs/sph.c b/funtools/wcs/sph.c deleted file mode 100644 index b8ba23d..0000000 --- a/funtools/wcs/sph.c +++ /dev/null @@ -1,234 +0,0 @@ -/*============================================================================ -* -* WCSLIB - an implementation of the FITS WCS proposal. -* Copyright (C) 1995-2002, Mark Calabretta -* -* This library 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 2 of the License, or (at your option) any later version. -* -* This library 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 Public -* License along with this library; if not, write to the Free Software -* Foundation, Inc., 59 Temple Place, Suite 330, Boston, MA 02111-1307 USA -* -* Correspondence concerning WCSLIB may be directed to: -* Internet email: mcalabre@atnf.csiro.au -* Postal address: Dr. Mark Calabretta, -* Australia Telescope National Facility, -* P.O. Box 76, -* Epping, NSW, 2121, -* AUSTRALIA -* -*============================================================================= -* -* C routines for the spherical coordinate transformations used by the FITS -* "World Coordinate System" (WCS) convention. -* -* Summary of routines -* ------------------- -* The spherical coordinate transformations are implemented via separate -* functions for the transformation in each direction. -* -* Forward transformation; sphfwd() -* -------------------------------- -* Transform celestial coordinates to the native coordinates of a projection. -* -* Given: -* lng,lat double Celestial longitude and latitude, in degrees. -* eul[5] double Euler angles for the transformation: -* 0: Celestial longitude of the native pole, in -* degrees. -* 1: Celestial colatitude of the native pole, or -* native colatitude of the celestial pole, in -* degrees. -* 2: Native longitude of the celestial pole, in -* degrees. -* 3: cos(eul[1]) -* 4: sin(eul[1]) -* -* Returned: -* phi, double Longitude and latitude in the native coordinate -* theta system of the projection, in degrees. -* -* Function return value: -* int Error status -* 0: Success. -* -* Reverse transformation; sphrev() -* -------------------------------- -* Transform native coordinates of a projection to celestial coordinates. -* -* Given: -* phi, double Longitude and latitude in the native coordinate -* theta system of the projection, in degrees. -* eul[5] double Euler angles for the transformation: -* 0: Celestial longitude of the native pole, in -* degrees. -* 1: Celestial colatitude of the native pole, or -* native colatitude of the celestial pole, in -* degrees. -* 2: Native longitude of the celestial pole, in -* degrees. -* 3: cos(eul[1]) -* 4: sin(eul[1]) -* -* Returned: -* lng,lat double Celestial longitude and latitude, in degrees. -* -* Function return value: -* int Error status -* 0: Success. -* -* Author: Mark Calabretta, Australia Telescope National Facility -* $Id: sph.c,v 2.7 2002/04/03 01:25:29 mcalabre Exp $ -*===========================================================================*/ - -#include <math.h> -#include "wcslib.h" - -#ifndef __STDC__ -#ifndef const -#define const -#endif -#endif - -const double tol = 1.0e-5; - -int sphfwd (lng, lat, eul, phi, theta) - -const double lat, lng, eul[5]; -double *phi, *theta; - -{ - double coslat, coslng, dlng, dphi, sinlat, sinlng, x, y, z; - - coslat = cosdeg (lat); - sinlat = sindeg (lat); - - dlng = lng - eul[0]; - coslng = cosdeg (dlng); - sinlng = sindeg (dlng); - - /* Compute the native longitude. */ - x = sinlat*eul[4] - coslat*eul[3]*coslng; - if (fabs(x) < tol) { - /* Rearrange formula to reduce roundoff errors. */ - x = -cosdeg (lat+eul[1]) + coslat*eul[3]*(1.0 - coslng); - } - y = -coslat*sinlng; - if (x != 0.0 || y != 0.0) { - dphi = atan2deg (y, x); - } else { - /* Change of origin of longitude. */ - dphi = dlng - 180.0; - } - *phi = eul[2] + dphi; - - /* Normalize the native longitude. */ - if (*phi > 180.0) { - *phi -= 360.0; - } else if (*phi < -180.0) { - *phi += 360.0; - } - - /* Compute the native latitude. */ - if (fmod(dlng,180.0) == 0.0) { - *theta = lat + coslng*eul[1]; - if (*theta > 90.0) *theta = 180.0 - *theta; - if (*theta < -90.0) *theta = -180.0 - *theta; - } else { - z = sinlat*eul[3] + coslat*eul[4]*coslng; - /* Use an alternative formula for greater numerical accuracy. */ - if (fabs(z) > 0.99) { - if (z < 0) - *theta = -acosdeg (sqrt(x*x+y*y)); - else - *theta = acosdeg (sqrt(x*x+y*y)); - } else { - *theta = asindeg (z); - } - } - - return 0; -} - -/*-----------------------------------------------------------------------*/ - -int sphrev (phi, theta, eul, lng, lat) - -const double phi, theta, eul[5]; -double *lng, *lat; - -{ - double cosphi, costhe, dlng, dphi, sinphi, sinthe, x, y, z; - - costhe = cosdeg (theta); - sinthe = sindeg (theta); - - dphi = phi - eul[2]; - cosphi = cosdeg (dphi); - sinphi = sindeg (dphi); - - /* Compute the celestial longitude. */ - x = sinthe*eul[4] - costhe*eul[3]*cosphi; - if (fabs(x) < tol) { - /* Rearrange formula to reduce roundoff errors. */ - x = -cosdeg (theta+eul[1]) + costhe*eul[3]*(1.0 - cosphi); - } - y = -costhe*sinphi; - if (x != 0.0 || y != 0.0) { - dlng = atan2deg (y, x); - } else { - /* Change of origin of longitude. */ - dlng = dphi + 180.0; - } - *lng = eul[0] + dlng; - - /* Normalize the celestial longitude. */ - if (eul[0] >= 0.0) { - if (*lng < 0.0) *lng += 360.0; - } else { - if (*lng > 0.0) *lng -= 360.0; - } - - if (*lng > 360.0) { - *lng -= 360.0; - } else if (*lng < -360.0) { - *lng += 360.0; - } - - /* Compute the celestial latitude. */ - if (fmod(dphi,180.0) == 0.0) { - *lat = theta + cosphi*eul[1]; - if (*lat > 90.0) *lat = 180.0 - *lat; - if (*lat < -90.0) *lat = -180.0 - *lat; - } else { - z = sinthe*eul[3] + costhe*eul[4]*cosphi; - - /* Use an alternative formula for greater numerical accuracy. */ - if (fabs(z) > 0.99) { - if (z < 0) - *lat = -acosdeg (sqrt(x*x+y*y)); - else - *lat = acosdeg (sqrt(x*x+y*y)); - } else { - *lat = asindeg (z); - } - } - - return 0; -} -/* Dec 20 1999 Doug Mink - Change cosd() and sind() to cosdeg() and sindeg() - * Dec 20 1999 Doug Mink - Include wcslib.h, which includes wcstrig.h, sph.h - * Dec 20 1999 Doug Mink - Define copysign only if it is not already defined - * - * Jan 5 2000 Doug Mink - Drop copysign - * - * Sep 19 2001 Doug Mink - No change for WCSLIB 2.7 - */ |