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author | Joseph Hunkeler <jhunkeler@gmail.com> | 2015-07-08 20:46:52 -0400 |
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committer | Joseph Hunkeler <jhunkeler@gmail.com> | 2015-07-08 20:46:52 -0400 |
commit | fa080de7afc95aa1c19a6e6fc0e0708ced2eadc4 (patch) | |
tree | bdda434976bc09c864f2e4fa6f16ba1952b1e555 /math/slalib/pav.f | |
download | iraf-linux-fa080de7afc95aa1c19a6e6fc0e0708ced2eadc4.tar.gz |
Initial commit
Diffstat (limited to 'math/slalib/pav.f')
-rw-r--r-- | math/slalib/pav.f | 71 |
1 files changed, 71 insertions, 0 deletions
diff --git a/math/slalib/pav.f b/math/slalib/pav.f new file mode 100644 index 00000000..6e6af8a3 --- /dev/null +++ b/math/slalib/pav.f @@ -0,0 +1,71 @@ + 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 |