Tohban Report 2018-03-07: Difference between revisions
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{{Infobox Tohban Report| | {{Infobox Tohban Report| | ||
|start_date = 28 Feb 2018 | |start_date = 28 Feb 2018 | ||
|end_date = 7 Mar 2018 | |end_date = 7 Mar 2018 | ||
|tohban_name = Juan Carlos Martinez Oliveros | |tohban_name = Juan Carlos Martinez Oliveros | ||
|tohban_email = oliveros@ssl.berkeley.edu | |tohban_email = oliveros@ssl.berkeley.edu | ||
|next_tohban = Martin Fivian | |||
|next_tohban = | |||
}} | }} | ||
== Solar Activity == | == Solar Activity == | ||
Solar activity this week was relatively low. There are not visible active regions on disk. Solar activity is expected to be very low throughout the forecast period (07-09 Mar). | |||
Solar activity this week was relatively low. There are not | |||
visible active regions on disk. | |||
Solar activity is expected to be very low throughout the forecast | |||
period (07-09 Mar). | |||
How many GOES flares occurred? | How many GOES flares occurred? | ||
Flares above B, C, M, X class were 9 1 0 0 | |||
And how many of these are listed in the RHESSI flare list? | |||
9 1 0 0 | Flares above B, C, M, X class were 1 0 0 0 | ||
And how many of these are listed in the RHESSI flare | |||
list? | |||
1 0 0 0 | |||
And how many had EXCELLENT coverage? | And how many had EXCELLENT coverage? | ||
Flares above B, C, M, X class were 1 0 0 0 | |||
1 0 0 0 | There were RHESSI flares/GOES flares 1 / 11 | ||
There were RHESSI flares/GOES flares | |||
1 / | |||
11 | |||
over the time range 28-Feb-18 07-Mar-18 | over the time range 28-Feb-18 07-Mar-18 | ||
== Memory Management == | == Memory Management == | ||
The SSR reached a maximum of ~55 percent during this week. | |||
The SSR reached a maximum of ~55 percent during this | |||
week. | |||
== Spacecraft Status == | == Spacecraft Status == | ||
Detectors 3 and 8 are active and taking data. | Detectors 3 and 8 are active and taking data. | ||
The cold plate 1 and 2 temperatures are ~156.4K and 155.3K. As last week. | |||
Currently the Cryocooler power is ~55 W and the acceleration is at ~11mg | |||
Currently the Cryocooler power is ~55 W and the acceleration is at | |||
~11mg | |||
== Data Gaps == | == Data Gaps == | ||
There are multiple VC1 data gaps during the week. | |||
There are multiple VC1 data gaps during the week. | |||
== Detector issues = | == Detector issues = | ||
== Other notes == | == Other notes == | ||
Line 88: | Line 47: | ||
== Spacecraft Management == | == Spacecraft Management == | ||
{| class="wikitable" | {| class="wikitable" | ||
|- | |- | ||
| Decimation || Active/Vigorous | | Decimation || Active/Vigorous | ||
|- | |- | ||
| HLAT Decimation || Rear decimation | | HLAT Decimation || Rear decimation | ||
|- | |- | ||
| Night time data (fronts) || plus/minus 4 minutes from daylight | |||
| Night time data (fronts) || plus/minus 4 minutes from | |||
daylight | |||
|- | |- | ||
| Night time data (rears) || plus/minus 4 minutes from daylight | |||
| Night time data (rears) || plus/minus 4 minutes from | |||
daylight | |||
|- | |- | ||
| Require extra passes? || No | | Require extra passes? || No | ||
|- | |- | ||
| Requirement for moving pointer? || No | | Requirement for moving pointer? || No | ||
|- | |- | ||
| Attenuator operation || logic enabled | | Attenuator operation || logic enabled | ||
|- | |- | ||
| Detector problems? || See notes above. | | Detector problems? || See notes above. | ||
|} | |} | ||
[[Category:Tohban Report]] | [[Category:Tohban Report]] | ||
[[Category:Tohban]] | [[Category:Tohban]] |
Latest revision as of 15:57, 14 March 2018
Tohban Reports | |
---|---|
Start Date: | 28 Feb 2018 |
End Date: | 7 Mar 2018 |
Tohban: | Juan Carlos Martinez Oliveros |
Tohban email: | oliveros@ssl.berkeley.edu |
Next Tohban: | Martin Fivian |
List all reports |
Solar Activity
Solar activity this week was relatively low. There are not visible active regions on disk. Solar activity is expected to be very low throughout the forecast period (07-09 Mar).
How many GOES flares occurred?
Flares above B, C, M, X class were 9 1 0 0
And how many of these are listed in the RHESSI flare list?
Flares above B, C, M, X class were 1 0 0 0
And how many had EXCELLENT coverage?
Flares above B, C, M, X class were 1 0 0 0
There were RHESSI flares/GOES flares 1 / 11 over the time range 28-Feb-18 07-Mar-18
Memory Management
The SSR reached a maximum of ~55 percent during this week.
Spacecraft Status
Detectors 3 and 8 are active and taking data.
The cold plate 1 and 2 temperatures are ~156.4K and 155.3K. As last week.
Currently the Cryocooler power is ~55 W and the acceleration is at ~11mg
Data Gaps
There are multiple VC1 data gaps during the week.
= Detector issues
Other notes
Spacecraft Management
Decimation | Active/Vigorous |
HLAT Decimation | Rear decimation |
Night time data (fronts) | plus/minus 4 minutes from daylight |
Night time data (rears) | plus/minus 4 minutes from daylight |
Require extra passes? | No |
Requirement for moving pointer? | No |
Attenuator operation | logic enabled |
Detector problems? | See notes above. |