Tohban Report 2011-04-27: Difference between revisions
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[[Category:Tohban Report | [[Category:Tohban Report 2011]] | ||
Latest revision as of 17:17, 17 March 2013
| Tohban Reports | |
|---|---|
| Start Date: | 20 Apr 2011 |
| End Date: | 27 Apr 2011 |
| Tohban: | Lindsay Glesener |
| Tohban email: | glesener@ssl.berkeley.edu |
| Next Tohban: | Hazel Bain |
| List all reports | |
Solar Activity
The Sun is quiet, though not inactive. The cluster of active regions (11195,6,7) are still making their way across the disk, but are not producing large flares. Altogether there are 5 named ARs on the disk. STEREO-B indicates that this level of activity will probably continue.
How many GOES flares occurred?
Flares above B, C, M, X class were 14 29 2 0
And how many of these are listed in the RHESSI flare list?
Flares above B, C, M, X class were 9 20 1 0
And how many had EXCELLENT coverage?
Flares above B, C, M, X class were 7 8 0 0
There were RHESSI flares/GOES flares 271 / 28 over the time range 20-Apr-11 27-Apr-11
Memory Management
The SSR is emptying at the end of each pass. We remain in normal/active decimation mode.
Data Gaps
No significant data gaps.
Spacecraft Status
No special commanding; all spacecraft parameters are nominal.
Science Presentation
There was a stupendous, mind-blowing science presentation by Lindsay Glesener.