Tohban Report 2010-06-02: Difference between revisions
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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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We are now at Normal/Vigorous, we decimate both NMZ and SMZ, and both fronts and rears are off at night. | We are now at Normal/Vigorous, we decimate both NMZ and SMZ, and both fronts and rears are off at night. | ||
== Data Gaps == | == Data Gaps == | ||
We have a lot of large data gaps. | We have a lot of large data gaps. Looks like Wallops files being misplaced/misnamed. But we seem to have all of them, and the data gaps should disappear in due time. | ||
[[category:Tohban Report 2010]] | |||
[[category:Tohban Report]] | |||
Latest revision as of 08:06, 4 March 2013
| Tohban Reports | |
|---|---|
| Start Date: | 26 May 2010 |
| End Date: | 02 June 2010 |
| Tohban: | Pascal Saint-Hilaire |
| Tohban email: | shilaire@ssl.berkeley.edu |
| Next Tohban: | Lindsay Glesener |
| 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.
Data Gaps
We have a lot of large data gaps. Looks like Wallops files being misplaced/misnamed. But we seem to have all of them, and the data gaps should disappear in due time.