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[vsnet-history 1964] HST Progress Report (Starrfield, nova net)




From: starrfie@hydro.la.asu.edu (Sumner Starrfield)
Subject: HST Progress Report (fwd)
Date: Thu, 16 Dec 93 22:23:47 MST

Forwarded message:
>From wms@stsci.edu Wed Dec 15 10:19:58 1993
Date: Wed, 15 Dec 93 12:26:43 EST
From: Robert Williams <wms@stsci.edu>
Message-ID: <vsnet-history1964@hoge.baba.hajime.jp>
To: starrfie@hydro.la.asu.edu
Subject: HST Progress Report

>From DOXSEY@avion.stsci.edu Wed Dec 15 12:18:18 1993
Subject: SMOV report Dec. 15, 1993
To: wms@stsci.edu, elt@astrovax.princeton.edu, grepass@gsfcmail.nasa.gov,
        jnb@sns.ias.edu, GILLIL@stsci.edu, sparks@stsci.edu, weaver@stsci.edu,
        mcgrath@stsci.edu, storrs@stsci.edu, ~saha@avion.stsci.edu,
        mackenty@stsci.edu, ~library@avion.stsci.edu, rjallen@stsci.edu,
        LONG@stsci.edu, sbaum@stsci.edu, ford@stsci.edu, SESD@avion.stsci.edu,
        ~hasan@avion.stsci.edu, hack@stsci.edu, cox@stsci.edu, drs@stsci.edu,
        ~KEYES@avion.stsci.edu, ~KINNEY@avion.stsci.edu, jtroeltzsch@ball.com,
        HULBERT@stsci.edu, jcampbell@gsfcmail.nasa.gov
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			SM Report #13

	11:00 AM December 15	349:16:00

	
	Summary of recent activities:

	The alignment of the new gyros relative to the FHSTs has
	been accomplished.  A total of 6 large angle slews were
	used in the calibration.  The new alignment matrices will
	be uplinked this afternoon.  A second set of 6 large angle
	slews this evening will confirm the calibration.

	There have been only a few SI activities in the last two
	days.  A GHRS aliveness test successfully checked out
	GHRS side 2.  In addition, the GHRS aperture and vent doors,
	which had been closed for the servicing mission, were
	opened.

	Problems/Issues/Changes under consideration:

	None

	Near-term plans:

	The second SMS, 93350, has been sent to PASS and starts 
	executing this evening.  This SMS covers 4 days and will
	continue basic spacecraft and SI checkout.  We will verify
	that guide star acquisitions work and run internal tests on
	the GHRS, FOS, and FOC.  Initial WFPC-II operations will
	take place during this period.  Tests will be run to check
	out the AFM and internal calibration systems.  The CCDs will
	be cooled to about -20 degrees C and internal flats will be
	taken.  The first UV contamination monitor observations and
	the first data on POM alignments will also be taken.


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