Tohban Report 2011-11-30: Difference between revisions
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|tohban_name = Claire Raftery | |tohban_name = Claire Raftery | ||
|tohban_email = claire@ssl.berkeley.edu | |tohban_email = claire@ssl.berkeley.edu | ||
|next_tohban = | |next_tohban = Hugh | ||
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Tohban should monitor G6 for this effect to ensure it doesn't get worse. | Tohban should monitor G6 for this effect to ensure it doesn't get worse. | ||
[[Category:Tohban Report | |||
[[Category:Tohban Report 2011]] | |||
Latest revision as of 01:16, 19 March 2013
| Tohban Reports | |
|---|---|
| Start Date: | 23 Nov 2011 |
| End Date: | 30 Nov 2011 |
| Tohban: | Claire Raftery |
| Tohban email: | claire@ssl.berkeley.edu |
| Next Tohban: | Hugh |
| List all reports | |
Solar Activity
Solar activity was extremely quiet with nothing more than some small C class flares despite numerous active regions. Stereo B doesn't show anything too large coming up.
How many GOES flares occurred?
Flares above B, C, M, X class were 9 24 0 0
And how many of these are listed in the RHESSI flare list?
Flares above B, C, M, X class were 6 15 0 0
And how many had EXCELLENT coverage?
Flares above B, C, M, X class were 5 5 0 0
There were RHESSI flares/GOES flares 164 / 33 over the time range 23-Nov-11 30-Nov-11
Memory Management
SSR is emptying.
Data Gaps
No data gaps.
Spacecraft Status
Detector noise and spikes are still a problem:
G3: http://sprg.ssl.berkeley.edu/~tohban/browser/?show=grth+qlpcr+qlpfr+qlprr+monfs+monfr+monff&date=20111126&time=103509 http://sprg.ssl.berkeley.edu/~tohban/browser/?show=grth+qlpcr+qlpfr+qlprr+monfs+monfr+monff&date=20111125&time=034015
G6: http://sprg.ssl.berkeley.edu/~tohban/browser/?show=grth+qlpcr+qlpfr+qlprr+monfs+monfr+monff&date=20111128&time=071949 http://sprg.ssl.berkeley.edu/~tohban/browser/?show=grth+qlpcr+qlpfr+qlprr+monfs+monfr+monff&date=20111126&time=103846 http://sprg.ssl.berkeley.edu/~tohban/browser/?show=grth+qlpcr+qlpfr+qlprr+monfs+monfr+monff&date=20111126&time=183141 http://sprg.ssl.berkeley.edu/~tohban/browser/?show=grth+qlpcr+qlpfr+qlprr+monfs+monfr+monff&date=20111126&time=045831
G8: http://sprg.ssl.berkeley.edu/~tohban/browser/?show=grth+qlpcr+qlpfr+qlprr+monfs+monfr+monff&date=20111129&time=174107 http://sprg.ssl.berkeley.edu/~tohban/browser/?show=grth+qlpcr+qlpfr+qlprr+monfs+monfr+monff&date=20111129&time=033647 http://sprg.ssl.berkeley.edu/~tohban/browser/?show=grth+qlpcr+qlpfr+qlprr+monfs+monfr+monff&date=20111128&time=133800 http://sprg.ssl.berkeley.edu/~tohban/browser/?show=grth+qlpcr+qlpfr+qlprr+monfs+monfr+monff&date=20111123&time=183755
G9: http://sprg.ssl.berkeley.edu/~tohban/browser/?show=grth+qlpcr+qlpfr+qlprr+monfs+monfr+monff&date=20111127&time=052123 http://sprg.ssl.berkeley.edu/~tohban/browser/?show=grth+qlpcr+qlpfr+qlprr+monfs+monfr+monff&date=20111126&time=083805 http://sprg.ssl.berkeley.edu/~tohban/browser/?show=grth+qlpcr+qlpfr+qlprr+monfs+monfr+monff&date=20111124&time=183427
G6 appears to have a burst of noise coming out of SAA passes e.g. http://sprg.ssl.berkeley.edu/~tohban/browser/?show=grth+qlpcr+qlpfr+qlprr+monfs+monfr+monff&date=20111123&time=164747
Tohban should monitor G6 for this effect to ensure it doesn't get worse.