Tohban Report 2010-09-29

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|tohban_name = Lindsay Glesener
|tohban_name = Lindsay Glesener
|tohban_email = glesener@ssl.berkeley.edu
|tohban_email = glesener@ssl.berkeley.edu
-
|next_tohban  = TBA
+
|next_tohban  = Juan Carlos Martinez Oliveros
}}
}}
== Solar Activity ==
== Solar Activity ==
-
There are currently three active regions on the disk, though only one has been flaring.  There were about 28 B class flares in the last week, 14 of which were caught by RHESSI.  The only C-class activity consisted of two flares in the last day.
+
There are currently three active regions on the disk, though only one has been flaring.  There were about 28 B class flares in the last week, 14 of which were caught by RHESSI.  The only C-class activity consisted of three flares in the last day.  Similar flare rates will likely continue through the next week.
== Memory Management ==
== Memory Management ==
-
The SSR is emptying completely.
+
The SSR is emptying completely at the end of the daily passes, max 25%.
== Data Gaps ==
== Data Gaps ==
 +
 +
There were two large data gaps in the last two days:
<pre>
<pre>
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GAP START TIME              GAP END TIME                  GAP (SEC)
GAP START TIME              GAP END TIME                  GAP (SEC)
2010-09-28T00:00:00.000 -- 2010-09-28T01:40:00.000      6000.0000
2010-09-28T00:00:00.000 -- 2010-09-28T01:40:00.000      6000.0000
-
 
+
</pre>
 +
<pre>
GAPS IN APP_ID = 1 (VC1-SOH) WITH PACKET RATE LT 30
GAPS IN APP_ID = 1 (VC1-SOH) WITH PACKET RATE LT 30
N_GAPS          1
N_GAPS          1
Line 44: Line 47:
</pre>
</pre>
-
== Operations ==
+
Data are on the ground and will be reprocessed.  Isolated passes cannot be identified for the gaps; the reason for the gaps is currently unknown.
-
 
+
-
 
+
-
== Other notes ==
+
-
 
+
 +
== 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]]
[[category:Tohban]]
[[category:Tohban Report]]
[[category:Tohban Report]]

Revision as of 18:26, 29 September 2010


Tohban Reports
Start Date: 22 Sep 2010
End Date: 29 Sep 2010
Tohban: Lindsay Glesener
Tohban email: glesener@ssl.berkeley.edu
Next Tohban: Juan Carlos Martinez Oliveros
List all reports



Contents

Solar Activity

There are currently three active regions on the disk, though only one has been flaring. There were about 28 B class flares in the last week, 14 of which were caught by RHESSI. The only C-class activity consisted of three flares in the last day. Similar flare rates will likely continue through the next week.

Memory Management

The SSR is emptying completely at the end of the daily passes, max 25%.

Data Gaps

There were two large data gaps in the last two days: 

GAPS IN APP_ID = 1 (VC1-SOH) WITH PACKET RATE LT 30
N_GAPS           1
GAP START TIME              GAP END TIME                   GAP (SEC)
2010-09-28T00:00:00.000 -- 2010-09-28T03:15:00.000       11700.000
GAPS IN APP_ID = 154 (VC1-PMTRAS) WITH PACKET RATE LT 4
N_GAPS           1
GAP START TIME              GAP END TIME                   GAP (SEC)
2010-09-28T00:00:00.000 -- 2010-09-28T03:15:00.000       11700.000
GAPS IN APP_ID = 102 (VC3-MONITOR RATES) WITH PACKET RATE LT 30
N_GAPS           1
GAP START TIME              GAP END TIME                   GAP (SEC)
2010-09-28T00:00:00.000 -- 2010-09-28T01:40:00.000       6000.0000

GAPS IN APP_ID = 1 (VC1-SOH) WITH PACKET RATE LT 30
N_GAPS           1
GAP START TIME              GAP END TIME                   GAP (SEC)
2010-09-27T20:45:00.000 -- 2010-09-28T00:00:00.000       11700.000
GAPS IN APP_ID = 154 (VC1-PMTRAS) WITH PACKET RATE LT 4
N_GAPS           1
GAP START TIME              GAP END TIME                   GAP (SEC)
2010-09-27T20:50:00.000 -- 2010-09-28T00:00:00.000       11400.000
GAPS IN APP_ID = 102 (VC3-MONITOR RATES) WITH PACKET RATE LT 30
N_GAPS           1
GAP START TIME              GAP END TIME                   GAP (SEC)
2010-09-27T22:25:00.000 -- 2010-09-27T23:40:00.000       4500.0000

Data are on the ground and will be reprocessed. Isolated passes cannot be identified for the gaps; the reason for the gaps is currently unknown.

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.

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