Building Sequence Database Files for the
Hopkins Ultraviolet Telescope
Despite the best efforts of pre-mission planners, real-time conditions
may make it necessary to change some of the observational
parameters. These changes will be accomplished by editing the SDFs
(which will be available on our ground support computers at the
POCC in Huntsville),
re-running the BUILDSEQ program, and uplinking revised sequence loads to
the MMU on the Shuttle. In general, these changes will be
made by HUT Instrument Team members specifically trained for this
activity, in consultation with the person assigned responsibility for
filling out each SDF in the first place.
This document was translated by mm2html v1.3 on 13.07.94.
Jon