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author | Joe Hunkeler <jhunkeler@gmail.com> | 2015-08-11 16:51:37 -0400 |
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committer | Joe Hunkeler <jhunkeler@gmail.com> | 2015-08-11 16:51:37 -0400 |
commit | 40e5a5811c6ffce9b0974e93cdd927cbcf60c157 (patch) | |
tree | 4464880c571602d54f6ae114729bf62a89518057 /math/slalib/doc/pcd.hlp | |
download | iraf-osx-40e5a5811c6ffce9b0974e93cdd927cbcf60c157.tar.gz |
Repatch (from linux) of OSX IRAF
Diffstat (limited to 'math/slalib/doc/pcd.hlp')
-rw-r--r-- | math/slalib/doc/pcd.hlp | 51 |
1 files changed, 51 insertions, 0 deletions
diff --git a/math/slalib/doc/pcd.hlp b/math/slalib/doc/pcd.hlp new file mode 100644 index 00000000..dd6263a4 --- /dev/null +++ b/math/slalib/doc/pcd.hlp @@ -0,0 +1,51 @@ +.help pcd Jun99 "Slalib Package" +.nf + + SUBROUTINE slPCD (DISCO,X,Y) + + - - - - + P C D + - - - - + + Apply pincushion/barrel distortion to a tangent-plane [x,y]. + + Given: + DISCO d pincushion/barrel distortion coefficient + X,Y d tangent-plane coordinates + + Returned: + X,Y d distorted coordinates + + Notes: + + 1) The distortion is of the form RP = R*(1 + C*R**2), where R is + the radial distance from the tangent point, C is the DISCO + argument, and RP is the radial distance in the presence of + the distortion. + + 2) For pincushion distortion, C is +ve; for barrel distortion, + C is -ve. + + 3) For X,Y in units of one projection radius (in the case of + a photographic plate, the focal length), the following + DISCO values apply: + + Geometry DISCO + + astrograph 0.0 + Schmidt -0.3333 + AAT PF doublet +147.069 + AAT PF triplet +178.585 + AAT f/8 +21.20 + JKT f/8 +13.32 + + 4) There is a companion routine, slUPCD, which performs + an approximately inverse operation. + + P.T.Wallace Starlink 31 December 1992 + + Copyright (C) 1995 Rutherford Appleton Laboratory + Copyright (C) 1995 Association of Universities for Research in Astronomy Inc. + +.fi +.endhelp |