aboutsummaryrefslogtreecommitdiff
path: root/math/slalib/doc/v2tp.hlp
diff options
context:
space:
mode:
Diffstat (limited to 'math/slalib/doc/v2tp.hlp')
-rw-r--r--math/slalib/doc/v2tp.hlp42
1 files changed, 42 insertions, 0 deletions
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