Tohban Report 2010-06-02: Difference between revisions
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imported>Pshilaire (New page: {{Infobox Tohban Report| |start_date = 26 May 2010 |end_date = 02 June 2010 |tohban_name = Pascal Saint-Hilaire |tohban_email = shilaire@ssl.berkeley.edu |next_tohban = TBD }} == Solar ...) |
imported>Pshilaire No edit summary |
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== Data Gaps == | == Data Gaps == | ||
We have a lot of large data gaps. Have to look into this! | |||
[[category:Tohban]] | [[category:Tohban]] | ||
[[category:Tohban Report]] | [[category:Tohban Report]] | ||
Revision as of 17:53, 2 June 2010
| Tohban Reports | |
|---|---|
| Start Date: | 26 May 2010 |
| End Date: | 02 June 2010 |
| Tohban: | Pascal Saint-Hilaire |
| Tohban email: | shilaire@ssl.berkeley.edu |
| Next Tohban: | TBD |
| List all reports | |
Solar Activity
GOES baseline level steadily increased A5 level. We have three AR, which have been otherwise discreet.
How many GOES flares occurred?
Flares above B, C, M, X class were 2 0 0 0
And how many of these are listed in the RHESSI flare list?
Flares above B, C, M, X class were 1 0 0 0
And how many had EXCELLENT coverage?
Flares above B, C, M, X class were 1 0 0 0
There were RHESSI flares/GOES flares 2 / 2 over the time range 25-May-10 01-Jun-10
Memory Management
Memory seems now under control. We are now at 21.56% at the end of the pass set. We should be near to breaking even without the Waldheim passes.
We are now at Normal/Vigorous, we decimate both NMZ and SMZ, and both fronts and rears are off at night.
There was a shutter change...
Data Gaps
We have a lot of large data gaps. Have to look into this!