Tohban report, 3-May-2006 to 10-May-2006
Hugh Hudson, hhudson@ssl.berkeley.edu

1. Solar Activity

One C-class flare, but too high a background level to think about
quiet-Sun observations.

How many GOES flares occurred?
  Flares above B, C, M, X class were     14     1     0     0
And how many of these are listed in the RHESSI flare list?
  Flares above B, C, M, X class were      3     1     0     0
And how many had EXCELLENT coverage?
  Flares above B, C, M, X class were      2     1     0     0
 
There were RHESSI flares/GOES flares          17 /           15
over the time range 02-May-06 09-May-06

The "farside" activity monitor, found at
http://soi.stanford.edu/data/full_farside/latest.syn.gif
or via the Tohban Live link, has substantially improved. It seems now
to show several active regions, so we might see something next week.
Or, maybe not.

2. Memory Managment

Memory fill level oscillated between 30-50% all week. This is too high
because of decimation losses, we should do something about it.

3. Data Gaps

GAP START TIME              GAP END TIME                   GAP (SEC)

2006-05-07T07:55:00.000 -- 2006-05-07T08:35:00.000       2400.0000
2006-05-08T14:15:00.000 -- 2006-05-08T14:25:00.000       600.00000
2006-05-08T05:20:00.000 -- 2006-05-08T05:40:00.000       1200.0000

4. Spacecraft Operations

All quiet... 

5. Science presentation: Sigrid Stoiser on the Neupert effect

6. Next Week's Tohban: Sigrid Stoiser