27 December 1999 N. V. Nitta CHIEF OBSERVER'S REPORT for Week 52 20-Dec-99 to 26-Dec-99 GENERAL Two large active regions, AR 8798 and AR 8806, continued to be present, with the latter being more flare productive. However, no flares after 22 December exceeded the GOES M1 level, and no large CMEs occurred. A region coming up from the NE limb, AR 8810, may be the target of FlareGenesis over the next week or so. SXT TECHNICAL There are no outstanding issues at the moment. Pointing has been updated on Saturday. For Web material see Current Week: http://isass1.solar.isas.ac.jp/sxt_co/991224.html Index: http://isass1.solar.isas.ac.jp/sxt_co/index.html This week's science nugget continues a discussion of the involvement of large-scale structures (filament channels?) in CMEs than a single active region, which often assumes the S-like shape. CAMPAIGNS We are still waiting for the FlareGenesis launch. We continued to send daily messages to Antarctica in support of target selection. 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 No change in the SXT ops personnel. Greg Slater has graciously extended his stay primarily to finish fixing Y2K issues. Jingxiu Wang returned to Beijing with 22 GB of data stored on hard disk. SEMINARS No seminar. SXT TABLE PLAN, WEEK 53 (26-Dec-99 to 31-Dec-99) If the launch of Flare Genesis takes place on 27 December, we still have two days this year to coordinate. After that the next opportunity will be only on 4-Jan-00. ________________________________#_______________________________ JST Day UT Start Time Pass Table ID Monday AM 26-DEC-99 18:55 1 991226 P1 ARS1 DIFF Monday AM 27-DEC-99 00:03 4 991226 P4 ARS1 DARK Tuesday AM 27-DEC-99 17:26 1 991227 P1 ARS1 FG Wednesday AM 28-DEC-99 21:02 3 991228 P3 ARS1 FG Thursday AM 29-DEC-99 19:31 3 991229 P3 ARS1 STD This plan is subject to change. Continuing requests: KSC & SSOC Tohbans: If any KSC passes are likely to be cancelled (for example due to a typhoon) 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.