Tohban Report 2010-10-13: Difference between revisions
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Revision as of 17:46, 13 October 2010
Tohban Reports | |
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Start Date: | 06 Oct 2010 |
End Date: | 12 Oct 2010 |
Tohban: | Claire Raftery |
Tohban email: | claire@ssl.berkeley.edu |
Next Tohban: | |
List all reports |
Solar Activity
There is once active region on disk - NOAA AR 11112. The region has produced a number of B class flares but is in its decay phase and consists of a single alpha spot surrounded by bipolar plage. Former NOAA AR 11109/11110 will rotate on disk in the next 2 days. This region produced a number of C class flares during its last disk passage and may increase activity in the coming week.
How many GOES flares occurred? Flares above B, C, M, X class were 18 0 0 0 And how many of these are listed in the RHESSI flare list? Flares above B, C, M, X class were 9 0 0 0 And how many had EXCELLENT coverage? Flares above B, C, M, X class were 4 0 0 0
Memory Management
The SSR is
Data Gaps
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) 2010-10-07T16:15:00.000 -- 2010-10-07T16:20:00.000 300.00000 GAPS IN APP_ID = 102 (VC3-MONITOR RATES) WITH PACKET RATE LT 30 N_GAPS 2 GAP START TIME GAP END TIME GAP (SEC) 2010-10-12T21:55:00.000 -- 2010-10-12T22:05:00.000 600.00000 2010-10-12T23:35:00.000 -- 2010-10-13T00:00:00.000 1500.0000
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.