RHESSI Tohban report, February 7, 2005 to February 14, 2005
Amir Caspi (cepheid@ssl.berkeley.edu)

[1] Solar Activity
	Activity during the past week was very weak, with only 9 C-class
flares in total.  5 of the flares were at least partially observed by
RHESSI, with excellent coverage of 3 of those.


[2] Memory Management
	With the low activity, memory has not been a significant issue.
The SSR has remained between ~5% and ~40% the entire week, and is
currently at ~10% as of pass on 14-Feb-2005 @ 10:51 UT.


[3] Data Gaps
	There is a 5-minute gap in the VC3 data on 8 Feb 2005.  There are
also numerous gaps in the QuickLook plots, but these are not listed on the
Daily Data Gaps page - this is presumably a software bug.


[4] Special Operations
	The high voltages for detectors 5 and 6 were lowered by 4 steps on
8 Feb 2005.  Due to the low activity and therefore the low SSR level, the
front segments have been operating at night since 8 Feb 2005.  This will
likely continue as long as solar and particle activity remain low.


[5] Other Notes
	The 2005 transit of the Crab will occur only a few days after the
RHESSI workshop in Switzerland.  Careful planning will be required.


Next week's tohban: Amir Caspi (again)