Tohban Report 2011-01-19: Difference between revisions
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[[Category:Tohban Report 2011]] | |||
[[Category:Tohban Report | |||
Latest revision as of 01:25, 7 March 2013
| Tohban Reports | |
|---|---|
| Start Date: | 12 Jan 2011 |
| End Date: | 19 Jan 2011 |
| Tohban: | Claire Raftery |
| Tohban email: | claire@ssl.berkeley.edu |
| Next Tohban: | Hazel Bain |
| List all reports | |
Solar Activity
Nothing major. One AR produced a flurry of B class flares and a few small C class, including an LDE.
How many GOES flares occurred?
Flares above B, C, M, X class were 31 3 0 0
And how many of these are listed in the RHESSI flare list?
Flares above B, C, M, X class were 19 3 0 0
And how many had EXCELLENT coverage?
Flares above B, C, M, X class were 6 1 0 0
There were RHESSI flares/GOES flares 62 / 34
RHESSI Operations
Detector 6 is showing some unusual arcing behaviour in the front segments only. Per David Smith, the high voltage has been reduced by 16 steps: 6 steps on Jan 13 and 10 more steps on Jan 18. Tomorrow should show whether or not this is sufficient.
Data Gaps
GAPS IN APP_ID = 1 (VC1-SOH) WITH PACKET RATE LT 30 N_GAPS 1 GAP START TIME GAP END TIME GAP (SEC) 2011-01-18T02:20:00.000 -- 2011-01-18T02:25:00.000 300.00000