RHESSI Tohban report, 17-Sept-2004 to 23-Sept-2004 
Hugh Hudson (hhudson@ssl.berkeley.edu)

1. Solar Activity:

Activity was quite low, ending the week with only a single numbered
active region, and a rather boring one at that. However there was a
nice M-class flare and particle event on September 19. RHESSI 
observed about ten minutes' worth of the impulsive phase, but not
above 100 keV; according to Sa"m we then missed some more of the
hard X-ray event because of night.

How many GOES flares occurred?
  Flares above B, C, M, X class were     32     8     1     0
And how many of these are listed in the RHESSI flare list?
  Flares above B, C, M, X class were      9     5     1     0
And how many had EXCELLENT coverage?
  Flares above B, C, M, X class were      5     3     0     0

There were RHESSI flares/GOES flares          43 /           41
over the time range 17-Sep-04 25-Sep-04

2. Memory Management:

Back under control, dropping to below 30% at the conclusion of
the Berkeley passes.

3. Operations:

Spin rate approacheth 14.4 rpm. Ought we not increase it?

4. Other

A. Steven's new tool, tohban info at a glance, is now linked on

http://sprg.ssl.berkeley.edu:80/~tohban/

I've been using it but not to the exclusion of other things. Please
have a try and provide feedback to him. It has many clickable links
but has suffered this week because of a long EIT bakeout sequence.

B. I have colored my GOES_RHESSI plots somewhat and when I can figure out
how IDL colors work properly, I will fill them neatly in and otherwise
tidy up. I have now included both GOES spacecraft for the low channel,
so that eclipse gaps (currently happening for GOES 12) are filled in.

5. Next week's tohban: Paula Balciunaite