aboutsummaryrefslogtreecommitdiff
path: root/math/slalib/doc/cc2s.hlp
diff options
context:
space:
mode:
authorJoe Hunkeler <jhunkeler@gmail.com>2015-08-11 16:51:37 -0400
committerJoe Hunkeler <jhunkeler@gmail.com>2015-08-11 16:51:37 -0400
commit40e5a5811c6ffce9b0974e93cdd927cbcf60c157 (patch)
tree4464880c571602d54f6ae114729bf62a89518057 /math/slalib/doc/cc2s.hlp
downloadiraf-osx-40e5a5811c6ffce9b0974e93cdd927cbcf60c157.tar.gz
Repatch (from linux) of OSX IRAF
Diffstat (limited to 'math/slalib/doc/cc2s.hlp')
-rw-r--r--math/slalib/doc/cc2s.hlp33
1 files changed, 33 insertions, 0 deletions
diff --git a/math/slalib/doc/cc2s.hlp b/math/slalib/doc/cc2s.hlp
new file mode 100644
index 00000000..8a16e76e
--- /dev/null
+++ b/math/slalib/doc/cc2s.hlp
@@ -0,0 +1,33 @@
+.help cc2s Jun99 "Slalib Package"
+.nf
+
+ SUBROUTINE slCC2S (V, A, B)
+
+ - - - - -
+ C C 2 S
+ - - - - -
+
+ Direction cosines to spherical coordinates (single precision)
+
+ Given:
+ V r(3) x,y,z vector
+
+ Returned:
+ A,B r spherical coordinates in radians
+
+ The spherical coordinates are longitude (+ve anticlockwise
+ looking from the +ve latitude pole) and latitude. The
+ Cartesian coordinates are right handed, with the x axis
+ at zero longitude and latitude, and the z axis at the
+ +ve latitude pole.
+
+ If V is null, zero A and B are returned.
+ At either pole, zero A is returned.
+
+ P.T.Wallace Starlink July 1989
+
+ Copyright (C) 1995 Rutherford Appleton Laboratory
+ Copyright (C) 1995 Association of Universities for Research in Astronomy Inc.
+
+.fi
+.endhelp