Repatch (from linux) of OSX IRAF

1 files changed, 101 insertions, 0 deletions

diff --git a/math/slalib/tpv2c.f b/math/slalib/tpv2c.f
new file mode 100644
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+      SUBROUTINE slTPVC (XI, ETA, V, V01, V02, N)
+*+
+*     - - - - - -
+*      T P V C
+*     - - - - - -
+*
+*  Given the tangent-plane coordinates of a star and its direction
+*  cosines, determine the direction cosines of the tangent-point.
+*
+*  (single precision)
+*
+*  Given:
+*     XI,ETA    r       tangent plane coordinates of star
+*     V         r(3)    direction cosines of star
+*
+*  Returned:
+*     V01       r(3)    direction cosines of tangent point, solution 1
+*     V02       r(3)    direction cosines of tangent point, solution 2
+*     N         i       number of solutions:
+*                         0 = no solutions returned (note 2)
+*                         1 = only the first solution is useful (note 3)
+*                         2 = both solutions are useful (note 3)
+*
+*  Notes:
+*
+*  1  The vector V must be of unit length or the result will be wrong.
+*
+*  2  Cases where there is no solution can only arise near the poles.
+*     For example, it is clearly impossible for a star at the pole
+*     itself to have a non-zero XI value, and hence it is meaningless
+*     to ask where the tangent point would have to be.
+*
+*  3  Also near the poles, cases can arise where there are two useful
+*     solutions.  The argument N indicates whether the second of the
+*     two solutions returned is useful.  N=1 indicates only one useful
+*     solution, the usual case;  under these circumstances, the second
+*     solution can be regarded as valid if the vector V02 is interpreted
+*     as the "over-the-pole" case.
+*
+*  4  This routine is the Cartesian equivalent of the routine slTPSC.
+*
+*  P.T.Wallace   Starlink   5 June 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,V(3),V01(3),V02(3)
+      INTEGER N
+
+      REAL X,Y,Z,RXY2,XI2,ETA2P1,SDF,R2,R,C
+
+
+      X=V(1)
+      Y=V(2)
+      Z=V(3)
+      RXY2=X*X+Y*Y
+      XI2=XI*XI
+      ETA2P1=ETA*ETA+1.0
+      SDF=Z*SQRT(XI2+ETA2P1)
+      R2=RXY2*ETA2P1-Z*Z*XI2
+      IF (R2.GT.0.0) THEN
+         R=SQRT(R2)
+         C=(SDF*ETA+R)/(ETA2P1*SQRT(RXY2*(R2+XI2)))
+         V01(1)=C*(X*R+Y*XI)
+         V01(2)=C*(Y*R-X*XI)
+         V01(3)=(SDF-ETA*R)/ETA2P1
+         R=-R
+         C=(SDF*ETA+R)/(ETA2P1*SQRT(RXY2*(R2+XI2)))
+         V02(1)=C*(X*R+Y*XI)
+         V02(2)=C*(Y*R-X*XI)
+         V02(3)=(SDF-ETA*R)/ETA2P1
+         IF (ABS(SDF).LT.1.0) THEN
+            N=1
+         ELSE
+            N=2
+         END IF
+      ELSE
+         N=0
+      END IF
+
+      END