March 5, 2000 H. Hudson CHIEF OBSERVER'S REPORT for Week 10 27-Feb-00 through 05-Mar-00 GENERAL Solar activity hinted at an increase this week, and there was a (minimal) X-class flare. SXT TECHNICAL SXT functioned properly, no new problems to report. We carried out two redefinitions of Yohkoh normal pointing, one inadvertently putting us back at the old standard location for two days. There were several Y2K bugs associated with this, and we hope we've seen the last of them. For Web material see Current Week: http://isass1.solar.isas.ac.jp/sxt_co/000303.html Index: http://isass1.solar.isas.ac.jp/sxt_co/index.html The science nugget this week summarizes the X-flare observations. It is quite amazingly impulsive and Neupert-like. The decay is exceptionally fast, in spite of strong ejectivity, and the post-flare loops really shrunk to a one-pixel unresolved point at GOES maximum. CAMPAIGNS No coordinated campaigns have been scheduled for this week. For SXT plans, see: http://isass1.solar.isas.ac.jp/sxt_co/sxt_future.html For SXT completed campaigns, see: http://isass1.solar.isas.ac.jp/sxt_co/sxt_catalog.html PERSONNEL Hudson left to attend the ISTP workshop at GSFC. SEMINARS There was no seminar this week. SXT TABLE PLAN, WEEK 11 (06-Mar-00 - 11-Mar-00) This week's operations are standard, with no coordinated campaigns planned as of the time of this writing. ________________________________#_______________________________ JST Day UT Start Time Pass Table ID Monday PM 06-MAR-00 14:09 4 000306 P4 ARS1 DARKCAL Tuesday PM 07-MAR-00 09:13 2 000307 P2 ARS1 DIFF Tuesday PM 07-MAR-00 12:38 4 000307 P4 ARS1 STD Wednesday PM 08-MAR-00 12:49 4 000308 P4 ARS1 STD Thursday PM 09-MAR-00 13:00 4 000309 P4 ARS1 STD Friday PM 10-MAR-00 09:45 3 000310 P3 ARS1 STD Saturday PM 11-MAR-00 11:39 4 000311 P4 ARS1 STD Continuing requests: KSC & SSOC Tohbans: If any KSC passes are likely to be cancelled (for example due to heavy snowfall) or an SXT table cannot be uploaded for some reason, please telephone and e-mail the Chief Observer immediately. (sxt_co@isass0.solar.isas.ac.jp, copy to sxt_st@flare2.solar.isas.ac.jp). KSC Tohbans: In general flare mode supersedes table upload, i.e. if a flare is in progress please do not upload a new table, and contact the chief observer. Normally it is OK to go ahead with the planned table without change on the next pass, if it is available. Chief observers should keep an eye on this.