Tohban Report 2010-03-10: Difference between revisions
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imported>Hhudson (new tohban named!) |
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|start_date = 3 Mar 2010 | |start_date = 3 Mar 2010 | ||
|end_date = 10 Mar 2010 | |end_date = 10 Mar 2010 | ||
|tohban_name = | |tohban_name = Pascal St.-Hilaire | ||
|tohban_email = | |tohban_email = shilaire@ssl.berkeley.edu | ||
|next_tohban = TBD | |next_tohban = TBD | ||
}} | }} | ||
Latest revision as of 19:09, 10 March 2010
| Tohban Reports | |
|---|---|
| Start Date: | 3 Mar 2010 |
| End Date: | 10 Mar 2010 |
| Tohban: | Pascal St.-Hilaire |
| Tohban email: | shilaire@ssl.berkeley.edu |
| Next Tohban: | TBD |
| List all reports | |
Solar Activity
The Sun started the week with weak activity, but then that has disappeared and spotless days have returned. All the indices agree that we're finished with solar minimum; now, how soon will we see really strong active regions?
How many GOES flares occurred?
Flares above B, C, M, X class numbered 20 1 0 0
And how many of these are listed in the RHESSI flare list?
Flares above B, C, M, X class numbered 9 1 0 0
And how many had EXCELLENT coverage?
Flares above B, C, M, X class numbered 8 0 0 0
over the time range 02-Mar-10 09-Mar-10
RHESSI observed the only C-class event well, but with nothing above 12-25 keV.
GOES is going through its eclipse season.
Data survey
Nothing unusual spotted, no gaps. A couple of spikes in the data: one spike; another spike (the latter at the terminator)
Operations
Spin-up.