April 17, 2000 H. S. Hudson CHIEF OBSERVER'S REPORT for Week 16 10-April-00 through 16-April-00 GENERAL Yohkoh supported JOP083. Activity was not high, only four M flares (same as last week). SXT TECHNICAL SXT functioned properly, no new problems to report but one SEU. We carried out a routine repointing. SXT experimented with multiple H res long exposures, as opposed to long/short movie pairs. For Web material see Current Week: http://isass1.solar.isas.ac.jp/sxt_co/000414.html Index: http://isass1.solar.isas.ac.jp/sxt_co/index.html This week's nugget describes the impulsive excitation of an active-region sigmoid by a flare in the JOP083 target region. CAMPAIGNS In the middle of JOP083. 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 Acton departed, and Handy arrived: conservation of Bozon number established. SEMINARS S. Akiyama: "High-temperature regions above flare loop tops" S. Watari: "he interplanetary disturbance during 1999 Feb. 18-19 associated with an interconnecting loop structure" This week: Grechnev and Uchida. SXT TABLE PLAN, WEEK 17 (17-Apr-00 - 22-Apr-00) JOP 83 continues. We have generally been doing high-cadence observations with a single filter, looking at microflares. The contact has been Jack Ireland at SOHO. ________________________________#_______________________________ JST Day UT Start Time Pass Table ID Tuesday AM 17-APR-00 18:16 3 000417 P3 ARS1 DKCAL* Tuesday PM 18-APR-00 11:36 1 000418 P1 ARS2 JOP83+DF Wednesday AM 18-APR-00 16:43 4 000418 P4 ARS2 JOP83* Wednesday PM 19-APR-00 13:27 3 000419 P3 ARS2 JOP83 Friday AM 20-APR-00 15:19 4 000420 P4 ARS2 JOP83* Friday PM 21-APR-00 13:46 3 000421 P3 ARS2 JOP83 Saturday PM 22-APR-00 13:56 3 000422 P3 ARS1 STD * The ID reflects the UT date of the first pass. 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.