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Diffstat (limited to 'math/slalib/doc/v2tp.hlp')
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diff --git a/math/slalib/doc/v2tp.hlp b/math/slalib/doc/v2tp.hlp new file mode 100644 index 00000000..6522e398 --- /dev/null +++ b/math/slalib/doc/v2tp.hlp @@ -0,0 +1,42 @@ +.help v2tp Jun99 "Slalib Package" +.nf + + SUBROUTINE slV2TP (V, V0, XI, ETA, J) + + - - - - - + V 2 T P + - - - - - + + Given the direction cosines of a star and of the tangent point, + determine the star's tangent-plane coordinates. + + (single precision) + + Given: + V r(3) direction cosines of star + V0 r(3) direction cosines of tangent point + + Returned: + XI,ETA r tangent plane coordinates of star + J i status: 0 = OK + 1 = error, star too far from axis + 2 = error, antistar on tangent plane + 3 = error, antistar too far from axis + + Notes: + + 1 If vector V0 is not of unit length, or if vector V is of zero + length, the results will be wrong. + + 2 If V0 points at a pole, the returned XI,ETA 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 slS2TP. + + P.T.Wallace Starlink 27 November 1996 + + Copyright (C) 1996 Rutherford Appleton Laboratory + Copyright (C) 1995 Association of Universities for Research in Astronomy Inc. + +.fi +.endhelp |