Tohban Report 2010-08-18: Difference between revisions
imported>Lglesener (New page: {{Infobox Tohban Report| |start_date = 11 Aug 2010 |end_date = 18 Aug 2010 |tohban_name = Lindsay Glesener |tohban_email = glesener@ssl.berkeley.edu |next_tohban = tba }} == Solar Activi...) |
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|tohban_name = Lindsay Glesener | |tohban_name = Lindsay Glesener | ||
|tohban_email = glesener@ssl.berkeley.edu | |tohban_email = glesener@ssl.berkeley.edu | ||
|next_tohban = | |next_tohban = Claire Raftery | ||
}} | }} | ||
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== Memory Management == | == Memory Management == | ||
The SSR is | The SSR is emptying each day. | ||
== Data Gaps == | == Data Gaps == | ||
| Line 31: | Line 32: | ||
2010-08-12T11:10:00.000 -- 2010-08-12T14:00:00.000 10200.000 | 2010-08-12T11:10:00.000 -- 2010-08-12T14:00:00.000 10200.000 | ||
</pre> | </pre> | ||
These data were later located and are being reprocessed now. | |||
== Operations == | == Operations == | ||
A spin up was performed Aug 16. Current spin rate is 14.94 rpm. | A spin up was performed Aug 16. Current spin rate is 14.94 rpm. Normal/vigorous decimation. No events during eclipse or north/south magnetic zones. We agreed to temporarily take events during eclipse for at least a few days to see if we can still empty the SSR. It will be at the Operator / Tohban's discretion whether to turn off these events. | ||
A livetime issue was discussed. Since about 1 month after the anneal, the livetime averages (fronts and rears) have dropped to about 60%. The most likely reason for this is that livetime drops to 0 during nights since we are no longer taking events. Jim will try to adjust the livetime calculation so that it does not include zeros. | |||
== Other notes == | |||
The AGU abstract deadline is Sept 2. | |||
[[category:Tohban Report 2010]] | |||
[[category:Tohban Report]] | |||
Latest revision as of 01:16, 7 March 2013
| Tohban Reports | |
|---|---|
| Start Date: | 11 Aug 2010 |
| End Date: | 18 Aug 2010 |
| Tohban: | Lindsay Glesener |
| Tohban email: | glesener@ssl.berkeley.edu |
| Next Tohban: | Claire Raftery |
| List all reports | |
Solar Activity
Currently there are four active regions on the Sun.
How many GOES flares occurred? Flares above B, C, M, X class were 36 5 0 0 And how many of these are listed in the RHESSI flare list? Flares above B, C, M, X class were 22 4 0 0 And how many had EXCELLENT coverage? Flares above B, C, M, X class were 11 1 0 0
Memory Management
The SSR is emptying each day.
Data Gaps
GAPS IN APP_ID = 102 (VC3-MONITOR RATES) WITH PACKET RATE LT 30 N_GAPS 1 GAP START TIME GAP END TIME GAP (SEC) 2010-08-12T11:10:00.000 -- 2010-08-12T14:00:00.000 10200.000
These data were later located and are being reprocessed now.
Operations
A spin up was performed Aug 16. Current spin rate is 14.94 rpm. Normal/vigorous decimation. No events during eclipse or north/south magnetic zones. We agreed to temporarily take events during eclipse for at least a few days to see if we can still empty the SSR. It will be at the Operator / Tohban's discretion whether to turn off these events.
A livetime issue was discussed. Since about 1 month after the anneal, the livetime averages (fronts and rears) have dropped to about 60%. The most likely reason for this is that livetime drops to 0 during nights since we are no longer taking events. Jim will try to adjust the livetime calculation so that it does not include zeros.
Other notes
The AGU abstract deadline is Sept 2.