      SUBROUTINE slDS2C (A, B, V)
*+
*     - - - - - -
*      D S 2 C
*     - - - - - -
*
*  Spherical coordinates to direction cosines (double precision)
*
*  Given:
*     A,B       d      spherical coordinates in radians
*                         (RA,Dec), (long,lat) etc.
*
*  Returned:
*     V         d(3)   x,y,z unit vector
*
*  The spherical coordinates are longitude (+ve anticlockwise looking
*  from the +ve latitude pole) and latitude.  The Cartesian coordinates
*  are right handed, with the x axis at zero longitude and latitude, and
*  the z axis at the +ve latitude pole.
*
*  Last revision:   26 December 2004
*
*  Copyright P.T.Wallace.  All rights reserved.
*
*  License:
*    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 2 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 (see SLA_CONDITIONS); if not, write to the
*    Free Software Foundation, Inc., 51 Franklin Street, Fifth Floor,
*    Boston, MA  02110-1301  USA
*
*  Copyright (C) 1995 Association of Universities for Research in Astronomy Inc.
*-

      IMPLICIT NONE

      DOUBLE PRECISION A,B,V(3)

      DOUBLE PRECISION COSB


      COSB = COS(B)

      V(1) = COS(A)*COSB
      V(2) = SIN(A)*COSB
      V(3) = SIN(B)

      END
