Tohban Report 2010-10-20: Difference between revisions
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imported>Hazelbain (New page: {{Infobox Tohban Report| |start_date = 13 Oct 2010 |end_date = 20 Oct 2010 |tohban_name = Hazel Bain |tohban_email = hbain@ssl.berkeley.edu |next_tohban = Lindsay Glesener }} == Solar Ac...) |
imported>Lglesener No edit summary |
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No commanding changes this week. Spin rate is 14.65 and we remain in normal/vigorous decimation mode, with 4 minutes of data taken on each side of the eclipse. | No commanding changes this week. Spin rate is 14.65 and we remain in normal/vigorous decimation mode, with 4 minutes of data taken on each side of the eclipse. | ||
[[category:Tohban Report 2010]] | |||
[[category:Tohban Report]] | |||
Latest revision as of 01:21, 7 March 2013
| Tohban Reports | |
|---|---|
| Start Date: | 13 Oct 2010 |
| End Date: | 20 Oct 2010 |
| Tohban: | Hazel Bain |
| Tohban email: | hbain@ssl.berkeley.edu |
| Next Tohban: | Lindsay Glesener |
| List all reports | |
Solar Activity
This week NOAA AR 11112 further evolved and produced a number of C class flares and an M class flare. AR 11112 will rotate off the disk in the next 2 days. There are currently 6 active regions on disk.
How many GOES flares occurred? Flares above B, C, M, X class were 29 7 1 0 And how many of these are listed in the RHESSI flare list? Flares above B, C, M, X class were 15 4 1 0 And how many had EXCELLENT coverage? Flares above B, C, M, X class were 10 1 1 0
Memory Management
The minimum SSR level is around ~16% with a maximum of ~36%. Some extra weilheim passes have been scheduled to account for this.
Data Gaps
N_GAPS 1 GAP START TIME GAP END TIME GAP (SEC) 2010-10-17T09:20:00.000 -- 2010-10-17T17:35:00.000 29700.000
Spacecraft Status
No commanding changes this week. Spin rate is 14.65 and we remain in normal/vigorous decimation mode, with 4 minutes of data taken on each side of the eclipse.