Tohban Report 2009-10-28

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Revision as of 17:26, 28 October 2009 (view source) Jmctiernan (Talk | contribs) (Tohban report) ← Older edit		Revision as of 17:11, 29 October 2009 (view source) Jmctiernan (Talk | contribs) m Newer edit →
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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  = TBD	+	|next_tohban  = Pascal Saint-Hilaire
	}}		}}
	== Solar Activity ==		== Solar Activity ==
-	Plenty of activity. Hmmm, it seems that we don't have GOES event list data for the last few weeks. There have been numerous B and a few C class flares There were 103 RHESSI Flares for the time period: 21-Oct-2009 10:05:11 to 28-Oct-2009 10:05:11. Activity will persist while the active regions 11028 and 11029 are on the disk.	+	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 ==

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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.