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 X-Vms-To: @SMSTAFF.DIS Mime-Version: 1.0 Content-Type: TEXT/PLAIN Content-Transfer-Encoding: 7BIT 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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