Tohban report, 2-may-2005 to 9-may-2005
J.McTiernan, jimm@ssl.berkeley.edu

1. Solar Activity: Pretty active, the background GOES level was in the low
to mid B's, but with many flares.

How many GOES flares occurred?
  Flares above B, C, M, X class were     37    16     2     0
And how many of these are listed in the RHESSI flare list?
  Flares above B, C, M, X class were     12    14     2     0
And how many had EXCELLENT coverage?
  Flares above B, C, M, X class were     10     6     0     0
 
There were RHESSI flares/GOES flares          53 /           55
over the time range 01-May-05 08-May-05
 

2. Memory Managment:

Front events were turned off at night on 2-may, also decimation
was increased on 4-may from normal/active to active/active.
The SSR fill level is at 36% now. There were no pointer motions.

3. Data Gaps: 

In vc3 data
2005-05-02T08:55:00.000 -- 2005-05-02T10:55:00.000       7200.0000
2005-05-03T16:40:00.000 -- 2005-05-03T18:10:00.000       5400.0000
2005-05-04T05:20:00.000 -- 2005-05-04T05:25:00.000       300.00000
2005-05-04T05:45:00.000 -- 2005-05-04T05:50:00.000       300.00000
2005-05-04T18:00:00.000 -- 2005-05-04T18:10:00.000       600.00000
2005-05-06T08:20:00.000 -- 2005-05-06T08:40:00.000       1200.0000
2005-05-07T12:10:00.000 -- 2005-05-07T12:20:00.000       600.00000
2005-05-07T12:25:00.000 -- 2005-05-07T12:35:00.000       600.00000

The second gap should be filled soon. The first may have been 
overwritten. The shorter gaps are due to bad monitor rate packets in WPS
files.