30 June, 2000 B. Handy, H. Hudson CHIEF OBSERVER'S REPORT for Week 27 26-Jun-00 through 2-Jul-00 GENERAL Activity tapered slightly this week, with the GOES plot nearly flatline at sub-C level for a couple of 12-hour stretches. At the last gasp, an M flare happened on July 1. This week, of course, we expect fireworks on Tuesday. SXT TECHNICAL SXT worked fine without apparent problems this week. Some experimenting took place in preparation for JOP 123 in pursuit of DEM measurements. SXT SCIENTIFIC For Web material see Current Week: http://isass1.solar.isas.ac.jp/sxt_co/000630.html Index: http://isass1.solar.isas.ac.jp/sxt_co/index.html This week's nugget was inspired by N. V. Nitta's public release of his flare catalog cross-correlating TRACE data with Yohkoh/SXT and HXT. CAMPAIGNS JOP 123 (DEM Analysis) started on July 1. 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 H. Hudson returned. SEMINARS None. TELEMETRY DOWNLINKS Week Wallops Santiago Goldstone Canberra Madrid Japan 25 31 0 5 0 4 30 26 29 0 3 7 3 26 27 28 0 1 3 1 27 SXT TABLE PLAN, WEEK 28 (02-Jul-00 - 08-Jul-00) The VLA/SOHO/SXT Campaign (JOP 128, DEM studies) runs this week. ________________________________#_______________________________ JST Day UT Start Time Pass Table ID Monday PM 03-JUL-00 01:00 2 000702 P2 ARS1 VLA* Tuesday PM 04-JUL-00 01:08 2 000703 P2 ARS1 DARK* Wednesday PM 05-JUL-00 01:16 3 000704 P3 ARS1 VLA* Thursday PM 06-JUL-00 01:24 3 000705 P3 ARS1 DIFF* Friday PM 06-JUL-00 23:49 2 000706 P2 ARS1 STD* Saturday PM 07-JUL-00 23:57 3 000707 P3 ARS1 VLA* * The ID reflects the UT date of the first pass. This table plan is subject to change. 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.