31 December 1999 H.S. Hudson CHIEF OBSERVER'S REPORT for Week 53 27-Dec-99 to 31-Dec-99 GENERAL Three M-class flares at the beginning of the week, but then little else. Potentially interesting E-limb activity did not seem to pan out, at least judging by the NOAA reports. The balloon bearing the Flare Genesis telescope is still in its box, so far as we know, so we hope that activity resumes in good time. SXT TECHNICAL There are no outstanding issues at the moment. Minor Y2K bugs here and there, nothing urgent (but it is not midnight yet). For Web material see Current Week: http://isass1.solar.isas.ac.jp/sxt_co/991231.html Index: http://isass1.solar.isas.ac.jp/sxt_co/index.html Inspired by an AGU press release and a visit to one of the world's electron headquarters sites, this week's nugget deals with how in the world the Sun could manage to turn the solar wind off for three days. We all believe that it comes from the network, which looks tiresomely the same day in and day out... CAMPAIGNS We are still waiting for the FlareGenesis launch. Our support messages will resume Jan. 4, assuming that all goes well. 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 N. V. Nitta and G. Slater returned for a happy holiday in the U.S. SEMINARS No seminar. 31 December 1999 H. S. Hudson DRAFT SXT TABLE PLAN, WEEK 02 (3-Jan-00 to 9-Jan-00) DRAFT We are likely to have the Flare Genesis telescope in polar orbit this week, and this reflects that. We are a bit confused about week numbers (Jan. 2 is a Sunday and Wallops .w01 ends on this day). ________________________________#_______________________________ JST Day UT Start Time Pass Table ID Tuesday AM 4-Jan-00 15:36 2 000104 P2 ARS2 DIFF Wednesday AM 5-Jan-00 17:30 3 000105 P3 ARS2 DKCAL Thursday AM 6-Jan-00 17:43 3 000106 P3 ARS2 FG Friday AM 7-Jan-00 12:47 1 000107 P1 ARS2 FG Saturday AM 8-Jan-00 14:41 2 000106 P2 ARS2 FG This 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.