SXT Status Report 1 - 15 September 1997 (Weeks 36 - 37) H. Hudson, S. Savy, J.-P. Wuelser SUMMARY The new solar cycle has started in earnest, with lots of active regions and flares. SXT worked fine throughout the interval and we conducted several collaborative observations. SOLAR ACTIVITY The GOES level did not drop below B during the entire interval, with a steady progression of high-latitude regions showing relatively good staying power. There were 24 flares classed at C level and above. Yohkoh has made it successfully into its second solar maximum, apparently. SXT INSTRUMENT STATUS AND CALIBRATION ACTIVITIES SXT continues to operate well. The higher activity has ended the inclusion of long exposures in the standard observing tables. We have frequently readjusted the starting levels of the partial-frame images to give the exposure control a head start. We have also begun to include the Al.1 filter routinely in the PFI's, and find that these new regions are bright enough to force exposure levels shorter than the usual limit (15 sec). There has been no further progress on the terminator (stray light correction) program. But all the pieces are in place to make the final improvements. There was a missed communication between SXT_CO and the tohbans. This has inspired us to create a new fax form that will be used in similar cases (second table transfer to be done from KSC, rather than Sagamihara) to prevent this from happening again. See below regarding a possibly interesting use of the accidental data. Data archiving is complete through Week 35, 1997. PASS CONFLICTS AT KSC Week 36: One pass cancelled on behalf of HALCA. Week 37: Three passes cancelled on behalf of HALCA. CAMPAIGNS During Sep. 8-12 we participated in an X-ray bright point observation scheduled also by SOHO and ground-based observatories (L. McDonald, A. Fludra). This was a little bit unfortunate because of the moderate activity, which kept us from doing detailed coverage during the invisible orbits. Nevertheless SXT got excellent data on each of the XBP's selected by SOHO. We also did some dedicated observation oriented towards jets. Active-region jet activity in the past cycle was most frequently found in the leading parts of active regions, but the jet-active region we tried to observe in Week 37 was the opposite. A pattern? For Yohkoh target planning, the SXT weekly observing plan is available on the Web at http://www.space.lockheed.com/SXT/html2/First_Light.html or with "finger campaign@isass0.solar.isas.ac.jp | more" . See http://sohowww.nascom.nasa.gov/operations/targets/today for SoHO target planning. VISITORS AND PERSONNEL B. Schmieder and J.-C. Pecker stopped by on the way back from the I.A.U. meeting in Kyoto, and normal research activity more or less resumed after this grand affair. Jean-Pierre Wuelser arrived from Palo Alto. Nariaki Nitta returned to Palo Alto. SEMINARS September 5: B. Schmieder (DASOP, Obs. de Paris): "CMEs and Prominences with SOHO and Yohkoh" J.-C. Pecker (College de France): "Solar Radius Variations" The latter talk was unfortunately not announceable prior to the seminar, but was quite interesting. September 11: J.-P. Wuelser (Palo Alto): "Vector Magnetic Field Observations of the Footpoints of Solar Plumes Te. Watanabe (Mitaka): "Radiative vs Conductive Energy Loss in Active Regions" OTHER SCIENCE TOPICS An operations error gave us an unusual sequence of large field-of-view observations incorporating several full-fledged active regions as well as the MDI high-resolution field. If anybody is interested, the following question might be answered: What is the correlation, if any, on time scales of minutes to hours, among distinct active regions? This question could of course also be asked on longer time scales by reference to the full-frame image data. TOHBANS Tohbans for Week 36: SSOC : T. Yoshida, T. Kosugi KSC : J. Ogura, S. Yasuno SXT_CO: H. Hudson SXT_SW: - Tohbans for Week 37: SSOC: H. Miyazaki, T. Shimizu KSC. S. Yasuno, M. Noguchi SXT_CO: H. Hudson, J.-P. Wuelser SXT_SW: -