Tohban Report 2010-11-03: Difference between revisions
imported>ClaireRaftery (New page: {{Infobox Tohban Report| |start_date = 27 Oct 2010 |end_date = 03 Nov 2010 |tohban_name = Claire Raftery |tohban_email = claire@ssl.berkeley.edu |next_tohban = Hazel Bain }} == Solar Act...) |
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Revision as of 17:22, 3 November 2010
| Tohban Reports | |
|---|---|
| Start Date: | 27 Oct 2010 |
| End Date: | 03 Nov 2010 |
| Tohban: | Claire Raftery |
| Tohban email: | claire@ssl.berkeley.edu |
| Next Tohban: | |
| List all reports | |
Solar Activity
There have been four ARs on disk throughout the week. However, NOAA 11120 and NOAA 11117 have been the most active, producing the vast majority of events. The former NOAA 11112 is approaching the east limb. Having produced an M2.9 flare, along with 7 C class flares during its last passage, B and C class events are probable from this region in the coming week, along with continued C class activity from NOAA 11120.
How many GOES flares occurred? Flares above B, C, M, X class were 83 4 0 0 And how many of these are listed in the RHESSI flare list? Flares above B, C, M, X class were 71 3 0 0 And how many had EXCELLENT coverage? Flares above B, C, M, X class were 71 2 0 0
Memory Management
The SSR is emptying out at ~10% and is reaching a maximum at ~35%. This is due to some missed contacts this week. It should be rectified next week.
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) 2010-10-28T18:25:00.000 -- 2010-10-28T18:30:00.000 300.00000 GAPS IN APP_ID = 102 (VC3-MONITOR RATES) WITH PACKET RATE LT 30 N_GAPS 1 GAP START TIME GAP END TIME GAP (SEC) 2010-10-29T02:35:00.000 -- 2010-10-29T02:40:00.000 300.00000 GAPS IN APP_ID = 102 (VC3-MONITOR RATES) WITH PACKET RATE LT 30 N_GAPS 1 GAP START TIME GAP END TIME GAP (SEC) 2010-11-02T23:55:00.000 -- 2010-11-03T00:00:00.000 300.00000
Spacecraft Status
No commanding changes this week. Spin rate is 14.7 and we remain in normal/vigorous decimation mode, with 4 minutes of data taken on each side of the eclipse.