Tohban report, 2005/10/31 to 2005/11/07 Pascal Saint-Hilaire, shilaire@ssl.berkeley.edu 1. Solar Activity After the B9 flare on Halloween, solar activity has been low throughout the week (GOES baseline level: ~A3). Since Saturday, AR 10819/10820 are producing a string of B-flares (raising the baseline level to near B1). They should go over the limb later this week. How many GOES flares occurred? Flares above B, C, M, X class were 11 0 0 0 And how many of these are listed in the RHESSI flare list? Flares above B, C, M, X class were 2 0 0 0 And how many had EXCELLENT coverage? Flares above B, C, M, X class were 2 0 0 0 There were RHESSI flares/GOES flares 8 / 11 over the time range 30-Oct-05 06-Nov-05 2. Memory Management Memory is down to ~20%. Front segment data are not being taken during S/C night. Decimation scheme is Normal/Vigorous. SAS data collection rate is at 32Hz. 3. Data Gaps None, apparently. 4. Misc. Science Brian Dennis has reported a possible problem with G6 spectra, where a hump could appear around 20-50 keV. Pulse pile-up is not the cause. Maybe a noise issue? 5. Misc. GOES data (from the SSWDB) for the past few weeks is still unavailable. Next Tohban: Martin Fivian