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+.help tps2c Jun99 "Slalib Package"
+.nf
+
+ SUBROUTINE slTPSC (XI, ETA, RA, DEC, RAZ1, DECZ1,
+ : RAZ2, DECZ2, N)
+
+ - - - - - -
+ T P S C
+ - - - - - -
+
+ From the tangent plane coordinates of a star of known RA,Dec,
+ determine the RA,Dec of the tangent point.
+
+ (single precision)
+
+ Given:
+ XI,ETA r tangent plane rectangular coordinates
+ RA,DEC r spherical coordinates
+
+ Returned:
+ RAZ1,DECZ1 r spherical coordinates of tangent point, solution 1
+ RAZ2,DECZ2 r spherical coordinates 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 RAZ1 and RAZ2 values are returned in the range 0-2pi.
+
+ 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
+ to bring about this combination of XI and DEC.
+
+ 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 corresponds to the "over-the-pole" case, and this is
+ reflected in the values of RAZ2 and DECZ2 which are returned.
+
+ 4 The DECZ1 and DECZ2 values are returned in the range +/-pi, but
+ in the usual, non-pole-crossing, case, the range is +/-pi/2.
+
+ 5 This routine is the spherical equivalent of the routine slDPVC.
+
+ Called: slRA2P
+
+ P.T.Wallace Starlink 5 June 1995
+
+ Copyright (C) 1995 Rutherford Appleton Laboratory
+ Copyright (C) 1995 Association of Universities for Research in Astronomy Inc.
+
+.fi
+.endhelp