Tohban Report 2010-11-10
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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 |
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. We remain in normal/vigorous decimation mode, with 4 minutes of data taken on each side of the eclipse. An increase of half a degree on the cold plate 1 was reported. This increase in temperature is related to the decreasing daylight time.