Tohban Report 2010-03-10: Difference between revisions
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How many GOES flares occurred? | How many GOES flares occurred? | ||
Flares above B, C, M, X class numbered 20 1 0 0 | Flares above B, C, M, X class numbered 20 1 0 0 | ||
And how many of these are listed in the RHESSI flare list? | And how many of these are listed in the RHESSI flare list? | ||
Flares above B, C, M, X class numbered 9 1 0 0 | Flares above B, C, M, X class numbered 9 1 0 0 | ||
And how many had EXCELLENT coverage? | And how many had EXCELLENT coverage? | ||
Flares above B, C, M, X class numbered 8 0 0 0 | Flares above B, C, M, X class numbered 8 0 0 0 | ||
over the time range 02-Mar-10 09-Mar-10 | over the time range 02-Mar-10 09-Mar-10 | ||
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== Operations == | == Operations == | ||
Spin-up | Spin-up. |
Revision as of 18:36, 10 March 2010
Tohban Reports | |
---|---|
Start Date: | 3 Mar 2010 |
End Date: | 10 Mar 2010 |
Tohban: | Hugh Hudson |
Tohban email: | hhudson@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.