Tohban Report 2010-11-10
From RHESSI Wiki
| Tohban Reports | |
|---|---|
| Start Date: | 03 Nov 2010 |
| End Date: | 10 Nov 2010 |
| Tohban: | Juan Carlos Martinez Oliveros |
| Tohban email: | oliveros@ssl.berkeley.edu |
| Next Tohban: | Jim McTiernan |
| List all reports | |
Contents |
Solar Activity
During the week there have been a total of three active regions on disk. The active region NOAA 11121 has been the most active producing a variety of flares including an M5.4 flare.
How many GOES flares occurred? Flares above B, C, M, X class were 27 10 3 0 And how many of these are listed in the RHESSI flare list? Flares above B, C, M, X class were 13 10 3 0 And how many had EXCELLENT coverage? Flares above B, C, M, X class were 3 2 0 0
Memory Management
The SSR is emptying out at about 0% and was reaching a maximum at ~35%.
Data Gaps
No major data gaps were reported. However, there were three VC3 data gaps:
GAPS IN APP_ID = 102 (VC3-MONITOR RATES) WITH PACKET RATE LT 30 N_GAPS 1 GAP START TIME GAP END TIME GAP (SEC) 2010-11-03T20:50:00.000 -- 2010-11-03T20:55:00.000 300.00000 GAPS IN APP_ID = 102 (VC3-MONITOR RATES) WITH PACKET RATE LT 30 N_GAPS 1 GAP START TIME GAP END TIME GAP (SEC) 2010-11-05T18:00:00.000 -- 2010-11-05T18:05:00.000 300.00000 GAPS IN APP_ID = 102 (VC3-MONITOR RATES) WITH PACKET RATE LT 30 N_GAPS 1 GAP START TIME GAP END TIME GAP (SEC) 2010-11-09T08:35:00.000 -- 2010-11-09T08:40:00.000 300.00000
Spacecraft Status
No commanding changes this week. Spin rate is 14.9 and we remain in normal/vigorous decimation mode, with 4 minutes of data taken on each side of the eclipse. The PTP (programmable Telemetry Processor) has been replaced as it was causing problems. This is the original that has been used since launch. The replacement now takes two copies of both the high time res and SMEX headers - the primary copy and the backup.
