Tohban Report 2009-05-20: Difference between revisions
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imported>Ayshih (New page: {{Infobox Tohban Report| |start_date = 14 May 2009 |end_date = 20 May 2009 |tohban_name = Albert Shih |tohban_email = ayshih@ssl.berkeley.edu |next_tohban = }} == Solar Activity == The ...) |
imported>Ayshih No edit summary |
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|tohban_name = Albert Shih | |tohban_name = Albert Shih | ||
|tohban_email = ayshih@ssl.berkeley.edu | |tohban_email = ayshih@ssl.berkeley.edu | ||
|next_tohban = | |next_tohban = Lindsay Glesener | ||
}} | }} | ||
== Solar Activity == | == Solar Activity == | ||
The Sun has been fairly quiet: only one numbered active region (AR 11017), which will move over the west limb in a couple of days. | The Sun has been fairly quiet: only one numbered active region (AR 11017), which will move over the west limb in a couple of days. The region produced an A-class flare on May 14 that RHESSI caught most of. STEREO shows no sign of notable activity in the near future. | ||
== Memory Management == | == Memory Management == | ||
The SSR has not been emptying after each set of passes, presumably due to a reduced number of passes as a consequence of the ongoing Shuttle mission and THEMIS operations. | |||
== Data Gaps == | == Data Gaps == | ||
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== Spacecraft Operations == | == Spacecraft Operations == | ||
The HV on detector 1 was lowered by 4 steps on May 14 (DoY 134). | |||
[[Category:Tohban Report]] | [[Category:Tohban Report]] | ||
[[Category:Tohban]] | [[Category:Tohban]] | ||
Revision as of 22:46, 20 May 2009
| Tohban Reports | |
|---|---|
| Start Date: | 14 May 2009 |
| End Date: | 20 May 2009 |
| Tohban: | Albert Shih |
| Tohban email: | ayshih@ssl.berkeley.edu |
| Next Tohban: | Lindsay Glesener |
| List all reports | |
Solar Activity
The Sun has been fairly quiet: only one numbered active region (AR 11017), which will move over the west limb in a couple of days. The region produced an A-class flare on May 14 that RHESSI caught most of. STEREO shows no sign of notable activity in the near future.
Memory Management
The SSR has not been emptying after each set of passes, presumably due to a reduced number of passes as a consequence of the ongoing Shuttle mission and THEMIS operations.
Data Gaps
No known VC3 gaps.
Spacecraft Operations
The HV on detector 1 was lowered by 4 steps on May 14 (DoY 134).