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author | Joe Hunkeler <jhunkeler@gmail.com> | 2015-08-11 16:51:37 -0400 |
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committer | Joe Hunkeler <jhunkeler@gmail.com> | 2015-08-11 16:51:37 -0400 |
commit | 40e5a5811c6ffce9b0974e93cdd927cbcf60c157 (patch) | |
tree | 4464880c571602d54f6ae114729bf62a89518057 /math/slalib/tp2v.f | |
download | iraf-osx-40e5a5811c6ffce9b0974e93cdd927cbcf60c157.tar.gz |
Repatch (from linux) of OSX IRAF
Diffstat (limited to 'math/slalib/tp2v.f')
-rw-r--r-- | math/slalib/tp2v.f | 74 |
1 files changed, 74 insertions, 0 deletions
diff --git a/math/slalib/tp2v.f b/math/slalib/tp2v.f new file mode 100644 index 00000000..ba2ff7dd --- /dev/null +++ b/math/slalib/tp2v.f @@ -0,0 +1,74 @@ + SUBROUTINE slTP2V (XI, ETA, V0, V) +*+ +* - - - - - +* T P 2 V +* - - - - - +* +* Given the tangent-plane coordinates of a star and the direction +* cosines of the tangent point, determine the direction cosines +* of the star. +* +* (single precision) +* +* Given: +* XI,ETA r tangent plane coordinates of star +* V0 r(3) direction cosines of tangent point +* +* Returned: +* V r(3) direction cosines of star +* +* Notes: +* +* 1 If vector V0 is not of unit length, the returned vector V will +* be wrong. +* +* 2 If vector V0 points at a pole, the returned vector V will be +* based on the arbitrary assumption that the RA of the tangent +* point is zero. +* +* 3 This routine is the Cartesian equivalent of the routine slTP2S. +* +* P.T.Wallace Starlink 11 February 1995 +* +* Copyright (C) 1995 Rutherford Appleton Laboratory +* +* 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 XI,ETA,V0(3),V(3) + + REAL X,Y,Z,F,R + + + X=V0(1) + Y=V0(2) + Z=V0(3) + F=SQRT(1.0+XI*XI+ETA*ETA) + R=SQRT(X*X+Y*Y) + IF (R.EQ.0.0) THEN + R=1E-20 + X=R + END IF + V(1)=(X-(XI*Y+ETA*X*Z)/R)/F + V(2)=(Y+(XI*X-ETA*Y*Z)/R)/F + V(3)=(Z+ETA*R)/F + + END |