CHIEF OBSERVER'S REPORT for Week 37 4-Sep-00 through 10-Sep-00 H. Hudson, A. Takeda GENERAL Activity remains low, but there were at least two M-class flares. We are still running the special flare-mode table with 2x2 FR images. It works well. SXT TECHNICAL No problems. SXT SCIENTIFIC For Web material see the science nuggets: Current Week: http://isass1.solar.isas.ac.jp/sxt_co/000908.html Index: http://isass1.solar.isas.ac.jp/sxt_co/index.html The current nugget deals with a beautiful pre-flare, flare, flare ejection, CME event of Sept. 7. Quite a nice event. CAMPAIGNS We supported the TXI rocket (SAO tunable X-ray imager). It flew on schedule, but its SPARCS system (pointing) failed - no data. This week we have also been running in support of JOP126 on coronal loop temperature structure. For this purpose we've been getting strip images 1024x256 at full resolution. JOP104 starts on September 15, to stydy the onset of flare-CME events. 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 Aki Takeda started. Nariaki Nitta arrived. SEMINARS None TELEMETRY DOWNLINKS Week Wallops Goldstone Canberra Madrid NASA ISAS 37 22 8 1 11 42 28 38 27 6 0 7 40 31 SXT TABLE PLAN, WEEK 38 (11-sep-00 to 17-sep) JOP126 observations will continue, concluding on 20-Sep; in the meanwhile JOP104 begins on Friday, Sep. 15, and will emphasize SUMER observations of the E limb. ________________________________#_______________________________ JST Day UT Start Time Pass Table ID Tuesday AM 11-SEP-00 17:04 3 000911 P3 ARS1 DIF126* Tuesday PM 12-SEP-00 13:46 1 000912 P1 ARS1 DARK Wednesday AM 12-SEP-00 18:52 4 000912 P4 ARS1 JOP126* Wednesday PM 13-SEP-00 13:52 2 000913 P2 ARS1 JOP126 Friday AM 14-SEP-00 15:42 3 000914 P3 ARS1 JOP104* Friday PM 15-SEP-00 12:24 2 000915 P2 ARS1 JOP104 Saturday PM 16-SEP-00 14:13 3 000916 P3 ARS1 JOP104 * 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.