REAL FUNCTION slPAV ( V1, V2 ) *+ * - - - - * P A V * - - - - * * Position angle of one celestial direction with respect to another. * * (single precision) * * Given: * V1 r(3) direction cosines of one point * V2 r(3) direction cosines of the other point * * (The coordinate frames correspond to RA,Dec, Long,Lat etc.) * * The result is the bearing (position angle), in radians, of point * V2 with respect to point V1. It is in the range +/- pi. The * sense is such that if V2 is a small distance east of V1, the * bearing is about +pi/2. Zero is returned if the two points * are coincident. * * V1 and V2 do not have to be unit vectors. * * The routine slBEAR performs an equivalent function except * that the points are specified in the form of spherical * coordinates. * * Called: slDPAV * * Last revision: 11 September 2005 * * 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 REAL V1(3), V2(3) INTEGER I DOUBLE PRECISION D1(3), D2(3) DOUBLE PRECISION slDPAV * Call the double precision version. DO I=1,3 D1(I) = V1(I) D2(I) = V2(I) END DO slPAV = REAL(slDPAV(D1,D2)) END