SXT Status report Mon, 20 January 1992 Fm: James Lemen The past week of operations was remarkably calm compared to the previous week (which had SEU-related troubles on 5 days in a row). There were no reported SXT problems and also no operational errors. The solar activity was also quite low for the most part, with only a few small flares observed. For this reason, on Tuesday we changed the Quiet High full frame table and inserted long (15s) exposures in the thin Al and Dagwood sandwich filters. One change from earlier operations is that we have decided to decrease the cadence of the 15s exposure images compared to the 75 ms and 2.667s images. There were many interesting images, one set showing large expanding loops on the N-W limb - perhaps associated with a CME. Greg Slater and Keith Strong spend much of week working on a new SXT movie covering about one solar rotation during the month of November. The movie was made using a professional M II tape recorder that S. Tsuneta had managed to borrow. The quality is much better than what we have made with existing equipment. Looking at the movie is certainly instructive, although it is clear that the ability to alter the rate of the playback would be highly desirable. The movie was made by combining the short (75 ms) and medium (2.667s) exposures from the standard Quiet High table. This increased the dynamic range and very adequately removed the saturated portions of the images. I have enjoyed viewing the approximately 1 minute movie about a dozen times. Each time I watch it I see something new. Sam Freeland arrived at the end of last week for a one week visit. One of his major activities will be to install a patch in the SXTE-U on-board software will perform checksums during each CCD exposure. This should make it easier to track and to understand future occurrences of SEU's. At the Yohkoh weekly operations meeting T. Kosugi announced that a necktie pin featuring an SXT image had been made by NEC. These pins may be purchased for 600 Yen (about $5). It is not exactly specified how these might be ordered, but if anyone reading this message would like to purchase one or more of these tie pins, you can respond to me (J. Lemen) and I will try to forward the list to the appropriate person. --- End of Report --- From sag::ISASS0::lemen Tue Jan 21 05:48:51 1992 Date: Tue, 21 Jan 92 05:48:22 -0800 From: sag::ISASS0::lemen (James R. Lemen) To: acton, freeland, hudson, morrison, nitta, sag::linford, slater, strong Cc: lemen, sag::friedlaender Subject: Short Status Report Status: RO Hello Everyone, This is an abreviated status report. 1. We have decided to remove the long (15s) exposures from the FFI sequence tables since the activity has been increasing somewhat recently. 2. Hara san ran a sequence (involving 3 table loads) today to try to get better data to compare the various filter ratios. He in particular would like to gain confidence in the calibration of the 3 micron Mg filter. 3. Sam is planning to do a patch on Thursday to provide a checksum function during each SXT exposure. The instrument has continued to operate without incident for the past 11 days. Regards, Jim From sag::ISASS0::lemen Thu Jan 23 02:21:08 1992 Date: Thu, 23 Jan 92 02:20:59 -0800 From: sag::ISASS0::lemen (James R. Lemen) To: acton, freeland, hudson, morrison, nitta, sag::linford, slater, strong Cc: lemen, sag::friedlaender Subject: Short Status Report - SEU on 23-Jan-92 Status: RO Hello Everyone, This is a short status report for Fri, 23-Jan-92. 1. Today the SXT experienced another SEU between the 3rd and 4th KSC contact. During the 4th pass we discovered that a filter hard error had caused the DP-J to turn off the power to the peripherals. This causes an "open-shutter" indication, and so Yohkoh was pointed to the east by 21 arc-min as a precaution. During the 5th pass a checksum was performed (with Sam Freeland in attendance) which verified that a code corruption had occurred, indicating that the primary cause was probably an SEU. Next, the recovering sequence was initiated, but because of a typing error, it was not possible to complete the sequence before the end of the pass. The SXT is currently in a same configuration (shutter is closed), but is not taking data. We will attempt to complete the