.help dtps2c Jun99 "Slalib Package" .nf SUBROUTINE slDPSC (XI, ETA, RA, DEC, RAZ1, DECZ1, : RAZ2, DECZ2, N) - - - - - - - D P S C - - - - - - - From the tangent plane coordinates of a star of known RA,Dec, determine the RA,Dec of the tangent point. (double precision) Given: XI,ETA d tangent plane rectangular coordinates RA,DEC d spherical coordinates Returned: RAZ1,DECZ1 d spherical coordinates of tangent point, solution 1 RAZ2,DECZ2 d 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: slDA2P 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