Tohban Report 2012-04-04

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Tohban Reports
Start Date: 29 Mar 2012
End Date: 4 Apr 2012
Tohban: Lindsay Glesener
Tohban email: glesener@ssl.berkeley.edu
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Solar Activity

This was a very quiet week, with no flares above C level. The past few days have been especially quiet, with no flares above B level.

How many GOES flares occurred?

Flares above B, C, M, X class were     16    7     0     0

And how many of these are listed in the RHESSI flare list?

Flares above B, C, M, X class were     12     5     0     0

And how many had EXCELLENT coverage?

Flares above B, C, M, X class were      8     4     0     0


Memory Management

At one point the SSR filled. See below.

RHESSI Operations

April 3, 22:26:42 UT: The SAS data rate was increased for coordinated limb observations with an SDO roll maneuver. Although this commanding was expected to only cause a small increase in the SSR fill, it instead caused the SSR to fill completely.

March 30, 17:53:27 UT: The front fast event threshold for detector 2 was raised by 0x10, from 0x60 to 0x70. This was done in order to save livetime that was being eaten up by excess fast rates in G2 due to light leak.

Data Gaps