Tohban Report 2013-04-03
From RHESSI Wiki
|Start Date:||27 Mar 2013|
|End Date:||04 Apr 2013|
|Next Tohban:||Juan Carlos Martinez Oliveros|
|List all reports|
Solar activity remained low with only 2 C-class flares. These C-class flares occurred on the last day of the week (Apr-03) and solar activity may become moderate over the next few days. On the other hand, STEREO B shows no active region which will rotate onto the disk over the next few days.
How many GOES flares occurred?
Flares above B, C, M, X class were 11 0 0 0
And how many of these are listed in the RHESSI flare list?
Flares above B, C, M, X class were 7 0 0 0
And how many had EXCELLENT coverage?
Flares above B, C, M, X class were 3 0 0 0
There were RHESSI flares/GOES flares 124 / 11 over the time range 26-Mar-13 02-Apr-13
The SSR emptied after most pass set.
A spin-up from 14.6 to 15.0 RPM was performed on 2013-086 between 18:23 and 19:30 UT.
There is one small (300 sec) data gap in VC3 data. GAP START TIME GAP END TIME GAP (SEC) 2013-04-02T23:55:00.000 -- 2013-04-03T00:00:00.000 300.00000
Detector 5 HV was lowered by 10 counts, bringing the voltage to 3800 V. The detector 5 monitor rate remains elevated (as high as that of detector 2).
The problem of quicklook generation processing has been fixed.
|HLAT Decimation||Rear decimation weight 6, no front decimation|
|Night time data (fronts)||+/- 4 minutes|
|Night time data (rears)||Taking data at nights|
|Require extra passes?||No|
|Requirement for moving pointer?||No|
|Detector problems?||Detector 5 arc + extended noise period.|