Tohban Report 2009-03-04
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(New page: {{Infobox Tohban Report| |start_date = 25 Feb 2009 |end_date = 04 Mar 2009 |tohban_name = Lindsay Glesener |tohban_email = glesener@ssl.berkeley.edu |next_tohban = Pascal Saint-Hilaire }} ...) |
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A HV change was requested: another 6 steps down on detectors 6 and 8. | A HV change was requested: another 6 steps down on detectors 6 and 8. | ||
- | [[Category:Tohban Report]] | + | [[Category:Tohban Report 2009]] |
[[Category:Tohban]] | [[Category:Tohban]] |
Revision as of 02:42, 28 February 2013
Tohban Reports | |
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Start Date: | 25 Feb 2009 |
End Date: | 04 Mar 2009 |
Tohban: | Lindsay Glesener |
Tohban email: | glesener@ssl.berkeley.edu |
Next Tohban: | Pascal Saint-Hilaire |
List all reports |
Contents |
Solar Activity
Very quiet; no GOES flares and no new active regions.
Memory Management
Max SSR fill is 25-30%. The decimation is normal/active and front-segment events are being recorded during eclipse.
Data Gaps
On March 3, there is about half a day of sporadically missing data packets, likely from a bad pass. Since there was no solar activity during this time, it's probably not worth replaying the data.
Spacecraft Operations
On Feb. 26, the temperature threshold for the HV cutoff was changed from 100K to 115K, with yellow and red limits put in at 105K and 110K, respectively. This was done to ensure that we do not trip the cutoff since the temperature is now just below 100K. (CP2 is currently at 97.6K.) However, it does appear the the temperatures have recently been trending downward.
A HV change was requested: another 6 steps down on detectors 6 and 8.