Tohban Report 2011-10-26: Difference between revisions
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{{Infobox Tohban Report| | {{Infobox Tohban Report| | ||
|start_date = | |start_date = 19 Oct 2011 | ||
|end_date = | |end_date = 26 Oct 2011 | ||
|tohban_name = Jim McTiernan | |tohban_name = Jim McTiernan | ||
|tohban_email = jimm@ssl.berkeley.edu | |tohban_email = jimm@ssl.berkeley.edu | ||
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[[Category:Tohban Report | [[Category:Tohban Report 2011]] | ||
Latest revision as of 17:26, 17 March 2013
| Tohban Reports | |
|---|---|
| Start Date: | 19 Oct 2011 |
| End Date: | 26 Oct 2011 |
| Tohban: | Jim McTiernan |
| Tohban email: | jimm@ssl.berkeley.edu |
| Next Tohban: | Jim McTiernan |
| List all reports | |
Solar Activity
Small stuff. but 1 M class:
How many GOES flares occurred?
Flares above B, C, M, X class were 0 9 1 0
And how many of these are listed in the RHESSI flare list?
Flares above B, C, M, X class were 0 6 1 0
And how many had EXCELLENT coverage?
Flares above B, C, M, X class were 0 6 0 0
There were RHESSI flares/GOES flares 227 / 10 over the time range 18-Oct-11 25-Oct-11
RHESSI Operations
Decimation was normal/vigorous for the full week.
Noise
No obvious noise spikes in any detectors
Data Gaps
None