Tohban Report 2011-06-29: Difference between revisions
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The SSR is emptying at the end of each pass. We remain in normal/active decimation mode. | The SSR is emptying at the end of each pass. We remain in normal/active decimation mode. | ||
Both front and rear data will now be taken during eclipse. This will likely have an effect on the SSR fill level. In addition, the shuttle is due for launch next week which will have a detrimental affect on our passes, and therefore will make it more difficult to empty the SSR. Also, if the disk-center EFR continues to grow, it may produce some interesting flares which we will want to catch so the SSR fill level should be monitored closely this week. | |||
== Data Gaps == | == Data Gaps == | ||
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http://sprg.ssl.berkeley.edu/~tohban/browser/?show=grth+monfr+monff&date=20110625&time=025555 | http://sprg.ssl.berkeley.edu/~tohban/browser/?show=grth+monfr+monff&date=20110625&time=025555 | ||
The high voltage for G6 will be dropped 4 steps per David Smith to try to alleviate the arcs. | |||
A spinup will be preformed later this week, depending on activity. | |||
[[Category:Tohban Report | [[Category:Tohban Report 2011]] | ||
Latest revision as of 17:20, 17 March 2013
| Tohban Reports | |
|---|---|
| Start Date: | 22 June 2011 |
| End Date: | 29 June 2011 |
| Tohban: | Claire Raftery |
| Tohban email: | claire@ssl.berkeley.edu |
| Next Tohban: | Nicole Duncan |
| List all reports | |
Solar Activity
There was no significant activity this week with only B class flares occurring. It looks like it will continue this way for the time being unless an EFR appears.
How many GOES flares occurred?
Flares above B, C, M, X class were 7 0 0 0
And how many of these are listed in the RHESSI flare list?
Flares above B, C, M, X class were 6 0 0 0
And how many had EXCELLENT coverage?
Flares above B, C, M, X class were 4 0 0 0
There were RHESSI flares/GOES flares 54 / 7 over the time range 22-Jun-11 29-Jun-1
Memory Management
The SSR is emptying at the end of each pass. We remain in normal/active decimation mode.
Both front and rear data will now be taken during eclipse. This will likely have an effect on the SSR fill level. In addition, the shuttle is due for launch next week which will have a detrimental affect on our passes, and therefore will make it more difficult to empty the SSR. Also, if the disk-center EFR continues to grow, it may produce some interesting flares which we will want to catch so the SSR fill level should be monitored closely this week.
Data Gaps
No data gaps.
Spacecraft Status
No special commanding; all spacecraft parameters are nominal, although Detector 6 continues to arc occasionally, the worst of which was seen here: http://sprg.ssl.berkeley.edu/~tohban/browser/?show=grth+monfr+monff&date=20110625&time=025555
The high voltage for G6 will be dropped 4 steps per David Smith to try to alleviate the arcs.
A spinup will be preformed later this week, depending on activity.