SXT REPORT FOR WEEKS 4 (This week number of consistent with the convention adopted in the Yohkoh database.) 17-23 January 1994 23 January 1994 Nariaki Nitta GENERAL STATUS In spite of an SEU-induced error, the SXT and the Yohkoh spacecraft are working well. PERSONNEL Hugh Hudson returned to ISAS together with other Hawaiians, Dick Canfield and Barry LaBonte. Nariaki Nitta is going back to California. Greg Slater is in charge reformatting and other software issues. Two BCS scientists from RAL, Jim Lang and Dave Pike are making short visits. SOLAR ACTIVITY Despite the strong expectations that AR 7654 would produce large flares, it apparently became weaker, and the GOES background level is around B3. SCIENCE PROGRESS There were significant activities focusing on AR 7260 (the region of interest at the Hawaii CDAW, Dec. 93). Canfield worked with Shibata (NAOJ) and his students on moving blue-shifted features seen in the MCCD dopplergrams, in connection with the emerging-flux-driven reconnection model. Shimizu (Univ of Tokyo) and Nitta had a short session on how to locate X-ray microflares on the MCCD continuum images. Lidia van Driel-Gesztelyi (Univ of Tokyo) made her monthly visit to ISAS and worked with Nitta on the draft of a paper on flares along the sheared inversion line, also examining flares in the emerging flux region in detail. Apart from AR 7260, Hudson discussed hard X-ray emission above the soft X-ray loop with its discoverer S. Masuda. The Yohkoh seminar resumed on the 20th with the speaker M. Ugai (Ehime Univ). The topic, spontaneous reconnection, interested many people who attended the seminar. On the same day, we went to a Japanese-style shouting bar to entertain R. Fielder, a secretary of LPARL, who used to work for SXT and was on her personal trip to Japan. There, half of the guests enjoyed hot debates on the importance of reconnection. SXT OPERATIONS The bright point campaign was cancelled due to the unfulfilled expectations of many flares. Hudson will take over as Chief Observer.