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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/gio/gflush.x | |
download | iraf-osx-40e5a5811c6ffce9b0974e93cdd927cbcf60c157.tar.gz |
Repatch (from linux) of OSX IRAF
Diffstat (limited to 'sys/gio/gflush.x')
-rw-r--r-- | sys/gio/gflush.x | 18 |
1 files changed, 18 insertions, 0 deletions
diff --git a/sys/gio/gflush.x b/sys/gio/gflush.x new file mode 100644 index 00000000..ef597da8 --- /dev/null +++ b/sys/gio/gflush.x @@ -0,0 +1,18 @@ +# Copyright(c) 1986 Association of Universities for Research in Astronomy Inc. + +include <gio.h> + +# GFLUSH -- Flush the graphics output. A simple call to the FIO flush does not +# suffice since the graphics data stream may be spread over three or more +# processes. Flush any buffered polyline output, append the GKI_FLUSH metacode +# instruction, and flush the FIO buffered metacode output. The other processes +# will take similar actions upon receipt of the GKI_FLUSH instruction. + +procedure gflush (gp) + +pointer gp # graphics descriptor + +begin + call gpl_flush() + call gki_flush (GP_FD(gp)) +end |