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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 /sys/imio/tf/impnlr.x | |
download | iraf-osx-40e5a5811c6ffce9b0974e93cdd927cbcf60c157.tar.gz |
Repatch (from linux) of OSX IRAF
Diffstat (limited to 'sys/imio/tf/impnlr.x')
-rw-r--r-- | sys/imio/tf/impnlr.x | 31 |
1 files changed, 31 insertions, 0 deletions
diff --git a/sys/imio/tf/impnlr.x b/sys/imio/tf/impnlr.x new file mode 100644 index 00000000..c60c8631 --- /dev/null +++ b/sys/imio/tf/impnlr.x @@ -0,0 +1,31 @@ +# Copyright(c) 1986 Association of Universities for Research in Astronomy Inc. + +include <imhdr.h> +include <imio.h> + +# IMPNL -- Put the next line to an image of any dimension or datatype. +# This is a sequential operator. The index vector V should be initialized +# before the first call to the first line to be written. Each call increments +# the leftmost subscript by one, until V equals IM_LEN, at which time EOF +# is returned. Subsequent writes are ignored. + +int procedure impnlr (imdes, lineptr, v) + +pointer imdes +pointer lineptr # on output, points to the pixels +long v[IM_MAXDIM] # loop counter +int npix +int impnln() +extern imflsr() +errchk impnln + +begin + if (IM_FLUSH(imdes) == YES) + call zcall1 (IM_FLUSHEPA(imdes), imdes) + + npix = impnln (imdes, lineptr, v, TY_REAL) + if (IM_FLUSH(imdes) == YES) + call zlocpr (imflsr, IM_FLUSHEPA(imdes)) + + return (npix) +end |