Tohban Report 2011-02-02: Difference between revisions
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imported>Lglesener (Created page with "{{Infobox Tohban Report| |start_date = 26 Jan 2011 |end_date = 02 Feb 2011 |tohban_name = Lindsay Glesener |tohban_email = glesener@ssl.berkeley.edu |next_tohban = TBA }} == So...") |
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|tohban_name = Lindsay Glesener | |tohban_name = Lindsay Glesener | ||
|tohban_email = glesener@ssl.berkeley.edu | |tohban_email = glesener@ssl.berkeley.edu | ||
|next_tohban = | |next_tohban = Jim McTiernan | ||
}} | }} | ||
== Solar Activity == | == Solar Activity == | ||
Solar activity is currently low, but we did have an M class flare last week. This event may have been slightly occulted, making it an even larger-than-M absolute size | Solar activity is currently low, but we did have an M class flare last week. This event may have been slightly occulted, making it an even larger-than-M absolute size. | ||
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== Spacecraft Commanding == | == Spacecraft Commanding == | ||
A spinup was performed on Feb. 1. The spin rate is now | A spinup was performed on Feb. 1. The spin rate is now 15.0 rpm. | ||
== Memory Management == | == Memory Management == | ||
The SSR had a max of 60% and a min of 25%. The large memory fill was likely due to fewer passes this week due to Themis maneuvering. For this week there are several added Weilheim passes. No data is taken during eclipse. | |||
[[Category:Tohban Report 2011]] | |||
[[Category:Tohban Report | |||
Latest revision as of 01:26, 7 March 2013
| Tohban Reports | |
|---|---|
| Start Date: | 26 Jan 2011 |
| End Date: | 02 Feb 2011 |
| Tohban: | Lindsay Glesener |
| Tohban email: | glesener@ssl.berkeley.edu |
| Next Tohban: | Jim McTiernan |
| List all reports | |
Solar Activity
Solar activity is currently low, but we did have an M class flare last week. This event may have been slightly occulted, making it an even larger-than-M absolute size.
How many GOES flares occurred? Flares above B, C, M, X class were 32 4 1 0 And how many of these are listed in the RHESSI flare list? Flares above B, C, M, X class were 12 4 1 0 And how many had EXCELLENT coverage? Flares above B, C, M, X class were 5 2 1 0
Spacecraft Commanding
A spinup was performed on Feb. 1. The spin rate is now 15.0 rpm.
Memory Management
The SSR had a max of 60% and a min of 25%. The large memory fill was likely due to fewer passes this week due to Themis maneuvering. For this week there are several added Weilheim passes. No data is taken during eclipse.