Tohban Report 2010-12-08

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== Solar Activity ==
== Solar Activity ==
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No much activity during the week. In the last couple of days the activity increased, but mainly small stuff.
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A large prominence (~ 1 Rs in length!). Look at EUV images! Only 1 C-flare during this week, though.
<pre>
<pre>
How many GOES flares occurred?
How many GOES flares occurred?
-
   Flares above B, C, M, X class were     7     0     0    0
+
   Flares above B, C, M, X class were    35    1     0    0
And how many of these are listed in the RHESSI flare list?
And how many of these are listed in the RHESSI flare list?
-
   Flares above B, C, M, X class were     4     0    0    0
+
   Flares above B, C, M, X class were     15     0    0    0
And how many had EXCELLENT coverage?
And how many had EXCELLENT coverage?
-
   Flares above B, C, M, X class were     2     0    0    0
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   Flares above B, C, M, X class were     11     0    0    0
   
   
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There were RHESSI flares/GOES flares          17 /           7
+
There were RHESSI flares/GOES flares          33 /           36
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over the time range 24-Nov-10 01-Dec-10
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over the time range 30-Nov-10 07-Dec-10
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</pre>
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</pre>
 +
 
 +
Today, two ~10-hr long GOES flux increase (from ~B1 baseline to ~B2). CMEs??
== Memory Management ==
== 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.
+
Because we are loosing 1-2 BGS passes a day to THEMIS/ARTEMIS operations, we are using 2 Waldheim passes/day. This should last until ~Sunday.
-
 
+
There is a little bit of concern we might have some troubles when the Sun becomes more active (we are getting more data than before the last anneal), but we should be able to handle it.
== Data Gaps ==
== Data Gaps ==
-
No major data gaps were reported. However, there were two VC3 data gaps:
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No data gaps of importance were reported.
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-
<pre>
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DATA GAPS FOR 2010/11/25
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TIME RANGE: 2010-11-25T00:00:00.000 -- 2010-11-26T00:00:00.000
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NO GAPS IN APP_ID = 1 (VC1-SOH)
+
-
NO GAPS IN APP_ID = 154 (VC1-PMTRAS)
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-
GAPS IN APP_ID = 102 (VC3-MONITOR RATES) WITH PACKET RATE LT 30
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N_GAPS          1
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GAP START TIME              GAP END TIME                  GAP (SEC)
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2010-11-25T00:10:00.000 -- 2010-11-25T00:15:00.000      300.00000
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-
</pre>
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-
 
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<pre>
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-
DATA GAPS FOR 2010/11/29
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TIME RANGE: 2010-11-29T00:00:00.000 -- 2010-11-30T00:00:00.000
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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)
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-
2010-11-29T11:30:00.000 -- 2010-11-29T11:35:00.000      300.00000
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</pre>
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-
 
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== Spacecraft Status ==
== 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.  
+
No commanding changes this week, except for a spin up last Wednesday. We remain in normal/vigorous decimation mode, with 4 minutes of data taken on each side of the eclipse.  
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[[Category:Tohban Report]]
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[[Category:Tohban Report 2010]]
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[[Category:Tohban]]
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Latest revision as of 01:23, 7 March 2013


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



Contents

Solar Activity

A large prominence (~ 1 Rs in length!). Look at EUV images! 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

Because we are loosing 1-2 BGS passes a day to THEMIS/ARTEMIS operations, we are using 2 Waldheim passes/day. This should last until ~Sunday. There is a little bit of concern we might have some troubles when the Sun becomes more active (we are getting more data than before the last anneal), but we should be able to handle it.

Data Gaps

No data gaps of importance were reported.

Spacecraft Status

No commanding changes this week, except for a spin up last Wednesday. We remain in normal/vigorous decimation mode, with 4 minutes of data taken on each side of the eclipse.

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