CHIEF OBSERVER'S REPORT for Week 35 27-Aug-01 through 2-Sep-01 A. Takeda GENERAL Solar activity remained high, although the GOES background has been gradually declining since the middle of the week. NOAA 9591 and the 9600/9601 complex were the major sources of the flare activity. SXT TECHNICAL No new problems to report. The operation supporting system at Kagoshima station was fully restored and has resumed normal operations. SXT SCIENTIFIC For Web material see the science nuggets: Current Week: http://isass1.solar.isas.ac.jp/sxt_co/010831.html Index: http://isass1.solar.isas.ac.jp/sxt_co/index.html This week's nugget, "Millimeter waves, white light, and gamma rays" presents the images and/or light curves during the X5.3 event on 25th August obtained in different wavelength ranges, including Yohkoh/GRS1, HXT, and SXT. CAMPAIGNS We made support observation for the balloon experiment (flying HX spectrometor, lead by a NAOJ and ISAS team) during the period between 23UT on the 28th and 2UT on the 29th. Although no major flares occurred during the flight, their instruments worked perfectly to get valuable data. 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 came back on 1st Sep., thus he will become the SXT_CO this coming week. SEMINARS No seminar this week. SXT TABLE PLAN, WEEK 36 (3-Sep-01 through 9-Sep-01) No official campaigns for this week. There will be two table uploads on Tuesday and Wednesday. _______________________________________________________________ JST Day UT Start Time Pass Table ID Monday PM 3-Sep-01 10:47 2 010903 P2 ARS1 STD Tuesday PM 4-Sep-01 07:23 1 010904 P1 ARS1 DIFF Tuesday PM 4-Sep-01 12:27 4 010904 P4 ARS1 STD Wednesday PM 5-Sep-01 07:22 1 010905 P1 ARS1 DARK Wednesday PM 5-Sep-01 12:26 4 010905 P4 ARS1 STD Thursday PM 6-Sep-01 09:01 2 010906 P2 ARS1 STD Friday PM 7-Sep-01 09:00 2 010907 P2 ARS1 STD Saturday PM 8-Sep-01 08:58 3 010908 P3 ARS1 STD The date part of a table ID reflects the UT date of pass 1. This table plan is likely to change. Prepare for last minute changes. Continuing requests: KSC & SSOC Tohbans: If any KSC passes are likely to be cancelled (for example due to typhoons) or an SXT table cannot be uploaded for any 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.