Tohban Report 2011-09-28
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These have been traced to WHM contacts that have not yet been processed. These will be filled in shortly. | These have been traced to WHM contacts that have not yet been processed. These will be filled in shortly. | ||
| - | + | [[Category:Tohban Report 2011]] | |
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Latest revision as of 17:26, 17 March 2013
| Tohban Reports | |
|---|---|
| Start Date: | 21 Sep 2011 |
| End Date: | 28 Sep 2011 |
| Tohban: | Jim McTiernan |
| Tohban email: | jimm@ssl.berkeley.edu |
| Next Tohban: | Juan Carlos Martinez-Oliveros |
| List all reports | |
Contents |
Solar Activity
Lots of activity, 2 X flares. more than 20 M flares,
How many GOES flares occurred?
Flares above B, C, M, X class were 0 51 21 2
And how many of these are listed in the RHESSI flare list?
Flares above B, C, M, X class were 0 35 17 2
And how many had EXCELLENT coverage?
Flares above B, C, M, X class were 0 20 9 1
There were RHESSI flares/GOES flares 415 / 74 over the time range 20-Sep-11 27-Sep-11
Plenty of small stuff.
RHESSI Operations
Decimation was normal/vigorous until 26-Sep, when it was changed to Active/Vigorous. Both Front and Rear detector events are turned off during eclipses, except for 4 minutes before and after daytime. SSR fill is at 0.0% at the end of the most recent set of passes. Decimation will be reset to Normal/Vigorous now.
Noise in Detector 8
Much noise in D8 from 3 to 16UT on 22-sep-2011, and at about 5UT on the 27th.
Data Gaps
VC3 Gaps:
2011-09-27T09:25:00.000 -- 2011-09-27T15:35:00.000 2011-09-25T23:30:00.000 -- 2011-09-26T02:40:00.000
These have been traced to WHM contacts that have not yet been processed. These will be filled in shortly.
