Tohban Report 2010-12-08: Difference between revisions

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{{Infobox Tohban Report|
{{Infobox Tohban Report|
|start_date = 1 Dec 2010
|start_date = 1 Dec 2010
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Today, two ~10-hr long GOES flux increase (from ~B1 baseline to ~B2). CMEs??
Today, two ~10-hr long GOES flux increase (from ~B1 baseline to ~B2). CMEs??
== Memory Management ==
The SSR is increasing the fill level due to loss passes, reaching a maximum at ~47%. In average the were 10 passes per day. It is expected that this regime will last another week.
== Data Gaps ==
No major data gaps were reported. However, there were two VC3 data gaps:
<pre>
DATA GAPS FOR 2010/11/25
TIME RANGE: 2010-11-25T00:00:00.000 -- 2010-11-26T00:00:00.000
NO GAPS IN APP_ID = 1 (VC1-SOH)
NO GAPS IN APP_ID = 154 (VC1-PMTRAS)
GAPS IN APP_ID = 102 (VC3-MONITOR RATES) WITH PACKET RATE LT 30
N_GAPS          1
GAP START TIME              GAP END TIME                  GAP (SEC)
2010-11-25T00:10:00.000 -- 2010-11-25T00:15:00.000      300.00000
</pre>
<pre>
DATA GAPS FOR 2010/11/29
TIME RANGE: 2010-11-29T00:00:00.000 -- 2010-11-30T00:00:00.000
NO GAPS IN APP_ID = 1 (VC1-SOH)
NO GAPS IN APP_ID = 154 (VC1-PMTRAS)
GAPS IN APP_ID = 102 (VC3-MONITOR RATES) WITH PACKET RATE LT 30
N_GAPS          1
GAP START TIME              GAP END TIME                  GAP (SEC)
2010-11-29T11:30:00.000 -- 2010-11-29T11:35:00.000      300.00000
</pre>
== Spacecraft Status ==
No commanding changes this week. We remain in normal/vigorous decimation mode, with 4 minutes of data taken on each side of the eclipse.
[[Category:Tohban Report]]
[[Category:Tohban]]

Revision as of 18:45, 8 December 2010


Tohban Reports
Start Date: 1 Dec 2010
End Date: 8 Dec 2010
Tohban: Pascal Saint-Hilaire
Tohban email: shilaire@ssl.berkeley.edu
Next Tohban: TBD
List all reports



Solar Activity

A large prominence (~ 1 Rs in length!). Look at EIT image! Only 1 C-flare during this week, though.

How many GOES flares occurred?
  Flares above B, C, M, X class were     35     1     0     0
And how many of these are listed in the RHESSI flare list?
  Flares above B, C, M, X class were     15     0     0     0
And how many had EXCELLENT coverage?
  Flares above B, C, M, X class were     11     0     0     0
 
There were RHESSI flares/GOES flares          33 /           36
over the time range 30-Nov-10 07-Dec-10
 

Today, two ~10-hr long GOES flux increase (from ~B1 baseline to ~B2). CMEs??

Memory Management

The SSR is increasing the fill level due to loss passes, reaching a maximum at ~47%. In average the were 10 passes per day. It is expected that this regime will last another week.


Data Gaps

No major data gaps were reported. However, there were two VC3 data gaps:

DATA GAPS FOR 2010/11/25
TIME RANGE: 2010-11-25T00:00:00.000 -- 2010-11-26T00:00:00.000
NO GAPS IN APP_ID = 1 (VC1-SOH)
NO GAPS IN APP_ID = 154 (VC1-PMTRAS)
GAPS IN APP_ID = 102 (VC3-MONITOR RATES) WITH PACKET RATE LT 30
N_GAPS           1
GAP START TIME              GAP END TIME                   GAP (SEC)
2010-11-25T00:10:00.000 -- 2010-11-25T00:15:00.000       300.00000
DATA GAPS FOR 2010/11/29
TIME RANGE: 2010-11-29T00:00:00.000 -- 2010-11-30T00:00:00.000
NO GAPS IN APP_ID = 1 (VC1-SOH)
NO GAPS IN APP_ID = 154 (VC1-PMTRAS)
GAPS IN APP_ID = 102 (VC3-MONITOR RATES) WITH PACKET RATE LT 30
N_GAPS           1
GAP START TIME              GAP END TIME                   GAP (SEC)
2010-11-29T11:30:00.000 -- 2010-11-29T11:35:00.000       300.00000

Spacecraft Status

No commanding changes this week. We remain in normal/vigorous decimation mode, with 4 minutes of data taken on each side of the eclipse.