Tohban Report 2009-09-30

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(New page: {{Infobox Tohban Report| |start_date = 23 September 2009 |end_date = 30 September 2009 |tohban_name = Lindsay Glesener |tohban_email = glesener@ssl.berkeley.edu |next_tohban = Neus Agueda...)
 
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Pascal Saint-Hilaire gave a presentation explaining his "deep integration" technique for imaging moving sources, as used in the most recent RHESSI science nugget (#111).
Pascal Saint-Hilaire gave a presentation explaining his "deep integration" technique for imaging moving sources, as used in the most recent RHESSI science nugget (#111).
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[[Category:Tohban Report]]
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[[Category:Tohban Report 2009]]
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Latest revision as of 03:19, 1 March 2013


Tohban Reports
Start Date: 23 September 2009
End Date: 30 September 2009
Tohban: Lindsay Glesener
Tohban email: glesener@ssl.berkeley.edu
Next Tohban: Neus Agueda
List all reports



Contents

Solar Activity

There are two new-cycle active regions on the Sun: 11026 and 11027. Region 11026 produced a few A- and B-class flares, and one C1 flare on Sept. 25 at ~0100 that was observed by RHESSI up to 20 keV. At least three of the smaller flares were also caught by RHESSI.

Memory Management

The SSR reached a max of 25% and is emptying after each pass.

Data Gaps

Problematic Santiago pass yesterday (9/29). Data has been replayed and should be available.

Spacecraft Operations

A spin-up was performed Monday, from ~14.5 rpm to 14.9 rpm. Cold Plate 2 is down slightly due to increased daytime. RHESSI is in normal/active decimation mode.

Other Notes

Pascal Saint-Hilaire gave a presentation explaining his "deep integration" technique for imaging moving sources, as used in the most recent RHESSI science nugget (#111).

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