Tohban Report 2009-10-28: Difference between revisions
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|tohban_name = Jim McTiernan | |tohban_name = Jim McTiernan | ||
|tohban_email = jimm@ssl.berkeley.edu | |tohban_email = jimm@ssl.berkeley.edu | ||
|next_tohban = | |next_tohban = Pascal Saint-Hilaire | ||
}} | }} | ||
== Solar Activity == | == Solar Activity == | ||
Plenty of activity. | Plenty of activity. How many GOES flares occurred? | ||
Flares above B, C, M, X class were 48 9 0 0 | |||
And how many of these are listed in the RHESSI flare list? | |||
Flares above B, C, M, X class were 31 7 0 0 | |||
And how many had EXCELLENT coverage? | |||
Flares above B, C, M, X class were 20 6 0 0 | |||
There were RHESSI flares/GOES flares 97 / 58 | |||
over the time range 21-Oct-09 28-Oct-09 | |||
Some RHESSI flares showed emission in the 12 to 25 keV band. | |||
== Memory Management == | == Memory Management == |
Revision as of 17:11, 29 October 2009
Tohban Reports | |
---|---|
Start Date: | 21 Oct 2009 |
End Date: | 28 Oct 2009 |
Tohban: | Jim McTiernan |
Tohban email: | jimm@ssl.berkeley.edu |
Next Tohban: | Pascal Saint-Hilaire |
List all reports |
Solar Activity
Plenty of activity. How many GOES flares occurred?
Flares above B, C, M, X class were 48 9 0 0
And how many of these are listed in the RHESSI flare list?
Flares above B, C, M, X class were 31 7 0 0
And how many had EXCELLENT coverage?
Flares above B, C, M, X class were 20 6 0 0
There were RHESSI flares/GOES flares 97 / 58 over the time range 21-Oct-09 28-Oct-09
Some RHESSI flares showed emission in the 12 to 25 keV band.
Memory Management
Decimation was normal/active for the week. Front segment events are not turned off during eclipses. SSR is at 2.7%
Data Gaps
None. There have been no data gaps since we lost 1 monitor rate packet on 28 September. There hasn't been a real gap (i.e., no packets for a period longer than 5 minutes) since 3 Spetember 2009.