Tohban Report 2009-07-22: Difference between revisions
imported>Pshilaire (New page: {{Infobox Tohban Report| |start_date = 15 July 2009 |end_date = 22 July 2009 |tohban_name = Pascal Saint-Hilaire |tohban_email = shilaire@ssl.berkeley.edu |next_tohban = TBD }} == Solar ...) |
imported>Lglesener No edit summary |
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|tohban_name = Pascal Saint-Hilaire | |tohban_name = Pascal Saint-Hilaire | ||
|tohban_email = shilaire@ssl.berkeley.edu | |tohban_email = shilaire@ssl.berkeley.edu | ||
|next_tohban = | |next_tohban = Lindsay Glesener | ||
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== Memory Management == | == Memory Management == | ||
Down to 0% at end of daily pass set. | Down to 0% at end of daily pass set, 22% at maximum. | ||
No front data taken during S/C night. | |||
NMZ nit decimated, SMZ decimated. | |||
Amir suggested to take front data at night, to complement the coverage of background data for Jim's background software. | |||
== Data Gaps == | == Data Gaps == | ||
Lots of VC1 data gaps this week. No | Lots of VC1 data gaps this week, courtesy of Wallops. No VC3 gaps, though. | ||
<pre> | <pre> | ||
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remained segmented through the pass. | remained segmented through the pass. | ||
[[Category:Tohban Report | Moreover, D. Smith mentionned we could turn off detector 2 if it doesn't register any useful counts during flares (it generates a lot of noise). Probably TBD with the next flare with emission above 20 keV... | ||
== Annealing issues == | |||
D. Smith would like to schedule a discussion on this topic. Tentatively, Wed, Aug 12th. | |||
[[Category:Tohban Report 2009]] | |||
Latest revision as of 03:16, 1 March 2013
| Tohban Reports | |
|---|---|
| Start Date: | 15 July 2009 |
| End Date: | 22 July 2009 |
| Tohban: | Pascal Saint-Hilaire |
| Tohban email: | shilaire@ssl.berkeley.edu |
| Next Tohban: | Lindsay Glesener |
| List all reports | |
Solar Activity
After squirting a few small flares last week, the Sun got back to being boring. There was a single A2 event. Otherwise, the GOES LO channel was flat the whole week.
Memory Management
Down to 0% at end of daily pass set, 22% at maximum. No front data taken during S/C night. NMZ nit decimated, SMZ decimated.
Amir suggested to take front data at night, to complement the coverage of background data for Jim's background software.
Data Gaps
Lots of VC1 data gaps this week, courtesy of Wallops. No VC3 gaps, though.
DATA GAPS FOR 2009/07/17 TIME RANGE: 2009-07-17T00:00:00.000 -- 2009-07-18T00:00:00.000 GAPS IN APP_ID = 1 (VC1-SOH) WITH PACKET RATE LT 30 N_GAPS 7 GAP START TIME GAP END TIME GAP (SEC) 2009-07-17T00:20:00.000 -- 2009-07-17T01:10:00.000 3000.0000 2009-07-17T01:35:00.000 -- 2009-07-17T02:15:00.000 2400.0000 2009-07-17T02:20:00.000 -- 2009-07-17T02:45:00.000 1500.0000 2009-07-17T03:20:00.000 -- 2009-07-17T04:05:00.000 2700.0000 2009-07-17T04:30:00.000 -- 2009-07-17T05:10:00.000 2400.0000 2009-07-17T05:15:00.000 -- 2009-07-17T05:35:00.000 1200.0000 2009-07-17T06:00:00.000 -- 2009-07-17T08:20:00.000 8400.0000 GAPS IN APP_ID = 154 (VC1-PMTRAS) WITH PACKET RATE LT 4 N_GAPS 5 GAP START TIME GAP END TIME GAP (SEC) 2009-07-17T00:00:00.000 -- 2009-07-17T00:50:00.000 3000.0000 2009-07-17T00:55:00.000 -- 2009-07-17T02:10:00.000 4500.0000 2009-07-17T04:20:00.000 -- 2009-07-17T06:45:00.000 8700.0000 2009-07-17T08:20:00.000 -- 2009-07-17T08:50:00.000 1800.0000 2009-07-17T09:05:00.000 -- 2009-07-17T09:20:00.000 900.00000 NO GAPS IN APP_ID = 102 (VC3-MONITOR RATES) DATA GAPS FOR 2009/07/16 TIME RANGE: 2009-07-16T00:00:00.000 -- 2009-07-17T00:00:00.000 GAPS IN APP_ID = 1 (VC1-SOH) WITH PACKET RATE LT 30 N_GAPS 4 GAP START TIME GAP END TIME GAP (SEC) 2009-07-16T21:00:00.000 -- 2009-07-16T21:10:00.000 600.00000 2009-07-16T21:20:00.000 -- 2009-07-16T21:55:00.000 2100.0000 2009-07-16T22:10:00.000 -- 2009-07-16T22:40:00.000 1800.0000 2009-07-16T22:50:00.000 -- 2009-07-16T23:50:00.000 3600.0000 GAPS IN APP_ID = 154 (VC1-PMTRAS) WITH PACKET RATE LT 4 N_GAPS 3 GAP START TIME GAP END TIME GAP (SEC) 2009-07-16T21:05:00.000 -- 2009-07-16T21:15:00.000 600.00000 2009-07-16T22:45:00.000 -- 2009-07-16T23:20:00.000 2100.0000 2009-07-16T23:30:00.000 -- 2009-07-17T00:00:00.000 1800.0000 NO GAPS IN APP_ID = 102 (VC3-MONITOR RATES)
Special Operations
As per D. Smith's request, G1 was lowered by 4 steps. The commanding was done ar 203-17:24:23 UT. The voltage now stands at 3210.8 V. The detector remained segmented through the pass.
Moreover, D. Smith mentionned we could turn off detector 2 if it doesn't register any useful counts during flares (it generates a lot of noise). Probably TBD with the next flare with emission above 20 keV...
Annealing issues
D. Smith would like to schedule a discussion on this topic. Tentatively, Wed, Aug 12th.