Report from ISAS 15 - 21 August 1994 Nariaki Nitta SUMMARY A flare-productive region AR 7765 was observed all through the week. OPERATIONS Both the satellite and SXT operations went smoothly, thanks largely to the skillful tohban Kyo Akita (Osaka Gakuin University), who reportedly has already signed return engagements. SOLAR ACTIVITY One active region (AR 7765) dominated the solar X-ray flux. It produced 6 M-class flares. Only one of them is known to have taken place during Yohkoh night. Only two of them belonged to the visible orbits and their data have been reformatted. Hugh Hudson looked at the SXT images of the M3.9 flare (14 August 1994 17:35 UT) in detail and Nariaki Nitta synthesized HXT images of the flare in all the channels. This region apparently became stabilized as it approached the western limb. PERSONNEL No change in the US SXT operations team. Bob Bentley arrived from MSSL for a four-week stay. SCIENCE Hudson and Nitta continued to work with Mukul Kundu, visiting professor at ISAS, on the relationship between X-ray jets/flares and meter-wave bursts. Kundu and Nitta managed to coalign SXT/HXT images with the Nobeyama Radio Heliograph images for two flares. The latter data show wobble of non-disk features with respect to the disk, reflecting the way calibrations are done. Fortunately, there were several active regions distibuted over the Sun, providing common features in free-free emission. Hudson worked with Akita to look into the 5 October 1992 behind-the-limb flare. The hard X-ray loop-top source is enhanced because the footpoints are probably occulted. This flare quite clearly shows an outward motion of plasmoid in the impulsive phase, as is common in this type of flares. ISAS WORKSTATIONS No more report, except that some disks (magnetic and magneto-optical) of the flareN workstations were accidentally unmounted from time to time and that we did not know who to ask for re-mounting. SEMINAR More than a dozen people have given us the titles for the extended Yohkoh seminar (= the first neighborhood meeting) that is planned on 24 August.