Tohban Report 2015-03-04
| Tohban Reports | |
|---|---|
| Start Date: | 25 Feb 2015 |
| End Date: | 4 Mar 2015 |
| Tohban: | Milo Buitrago-Casas & Lindsay Glesener |
| Tohban email: | milo@ssl.berkeley.edu |
| Next Tohban: | ? |
| List all reports | |
Solar Activity
Overall, solar activity this week was a bit higher than last. There are 2 active regions on the disk, both at the west limb producing many C and M class flares. This is a fairly recent burst of activity that started early Tuesday; before that time solar activity was quiet-to-moderate. These two AR will rotate off any second, and there isn't a lot else active, so solar activity is expected to drop soon. There should be a day or two of good opportunity for occulted flares.
How many GOES flares occurred?
Flares above B, C, M, X class were 6 26 4 0
And how many of these are listed in the RHESSI flare list?
Flares above B, C, M, X class were 4 17 4 0
And how many had EXCELLENT coverage?
Flares above B, C, M, X class were 0 0 0 0
There were RHESSI flares/GOES flares 208 / 36 over the time range 24-Feb-15 03-Mar-15
Memory Management
Spacecraft Status
Data Gaps
Temperatures
Cold Plate Temperatures 1 and 2 showed to be stable during the whole week. Cold Tip Temperatures 1 and 2 had values in accordance with the Cryocooler Power. However, because the cooler is now running at 97.6% of maximum allowed power, next Tohban should keep an eye on the Cryocooler parameters.
Detector issues
Other notes
Spacecraft Management
| Decimation | Normal/Vigorous |
| Night time data (fronts) | full nighttime events |
| Night time data (rears) | full nighttime events |
| Require extra passes? | Yes |
| Requirement for moving pointer? | No |
| Attenuator operation | Normal |