Tohban Report 2010-06-02: Difference between revisions

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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.
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]]
[[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.