RHESSI Tohban report, 29-sep-2003 to 5-oct-2003
J.McTiernan, jimm@ssl.berkeley.edu

1. Solar Activity:

Plenty of activity. The GOES background level started the week in the
high B range and is now donw to the B2-B3 level.  This explains the
lack of B flares; when the background is in the high B's it's hard to
get a B flare.

How many GOES flares occurred?
 
Flares above B, C, M, X class were           13          40           2           0
 
And how many had good RHESSI coverage?
 
Flares above B, C, M, X class were            6          29           0           0
 
And how many are listed in the RHESSI flare_list?
 
Flares above B, C, M, X class were            7          29           0           0
 
How many RHESSI flares:         118

2. Memory Managment:

Decimation was front-active, rear-active, due to the high activity level.
The average SSR fill level from 28-sep-2003 to 10-oct-2003 is:
2003/09/28      24.4051
2003/09/29      38.7545
2003/09/30      50.0540
2003/10/01      48.9090
2003/10/02      46.0723
2003/10/03      42.2222


3. Data Gaps:

None.