Tohban Report 2010-03-10: Difference between revisions
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== Solar Activity == | == Solar Activity == | ||
The Sun started the week with weak activity, but then that has disappeared and spotless days have returned. | |||
All the [http://www.leif.org/research/TSI-SORCE-2008-now.png indices] agree that we're finished with solar minimum; now, how soon will we see really strong active regions? | |||
Flares above B, C, M, X class | 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 [http://sprg.ssl.berkeley.edu/~tohban/browser/?show=grth+qlpcr+qli03&date=20100304&time=161754 only C-class event] well, but with nothing above 12-25 keV. | |||
GOES is going through its eclipse season. | |||
== Data survey == | == Data survey == | ||
Nothing unusual spotted, no gaps | Nothing unusual spotted, no gaps. A couple of spikes in the data: | ||
[http://sprg.ssl.berkeley.edu/~tohban/browser/?show=grth+qlpcr+monfs+monrs&date=20100307&time=042024 one spike]; | |||
[http://sprg.ssl.berkeley.edu/~tohban/browser/?show=grth+qlpcr+monfs+monrs&date=20100305&time=170248 another spike] (the latter at the terminator) | |||
== Operations == | |||
Spin-up | |||
Revision as of 18:35, 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