Tohban Report 2010-07-27
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Flares above B, C, M, X class were 39 1 0 0 | Flares above B, C, M, X class were 39 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 | + | Flares above B, C, M, X class were 18 0 0 0 |
And how many had EXCELLENT coverage? | And how many had EXCELLENT coverage? | ||
Flares above B, C, M, X class were 17 0 0 0 | Flares above B, C, M, X class were 17 0 0 0 | ||
- | There were RHESSI flares/GOES flares | + | There were RHESSI flares/GOES flares 18 / 40 |
over the time range 21-Jul-10 27-Jul-10 | over the time range 21-Jul-10 27-Jul-10 | ||
Line 79: | Line 79: | ||
A Gamma Ray Burst was observed by RHESSI on July 24th around 00:40:00 UT, lasting 2-3 min. Excellent RHESSI coverage. Also observed by Swift, Konus, INTEGRAL, and Suzaku. | A Gamma Ray Burst was observed by RHESSI on July 24th around 00:40:00 UT, lasting 2-3 min. Excellent RHESSI coverage. Also observed by Swift, Konus, INTEGRAL, and Suzaku. | ||
- | + | [[category:Tohban Report 2010]] | |
- | [[category:Tohban Report]] | + |
Latest revision as of 01:16, 7 March 2013
Tohban Reports | |
---|---|
Start Date: | 21 Jul 2010 |
End Date: | 27 Jul 2010 |
Tohban: | Neus Agueda |
Tohban email: | nagueda@ssl.berkeley.edu |
Next Tohban: | Meriem Alaoui |
List all reports |
Contents |
Solar Activity
Solar activity is at low levels. There were 39 flares this week, all of them B-class flares except for a C2.2 flare. Unfortunately the C-class flare was not caught by RHESSI. The active region that produced this flare (NOAA AR 11089) is now at S24W45. There are two other ARs on the disk, one close to the central meridian and the other one close to the west limb (W90).
How many GOES flares occurred?
Flares above B, C, M, X class were 39 1 0 0
And how many of these are listed in the RHESSI flare list?
Flares above B, C, M, X class were 18 0 0 0
And how many had EXCELLENT coverage?
Flares above B, C, M, X class were 17 0 0 0
There were RHESSI flares/GOES flares 18 / 40 over the time range 21-Jul-10 27-Jul-10
Memory Management
The SSR reached a max of 20% during the day. Santiago passes have been added.
Data Gaps
Some data gaps on Jul 22th, Jul 25th and Jul 26th, due to trouble processing the Wallops passage.
DATA GAPS FOR 2010/07/22 TIME RANGE: 2010-07-22T00:00:00.000 -- 2010-07-23T00:00:00.000 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) 2010-07-22T07:30:00.000 -- 2010-07-22T07:35:00.000 300.00000 DATA GAPS FOR 2010/07/25 TIME RANGE: 2010-07-25T00:00:00.000 -- 2010-07-26T00:00:00.000 GAPS IN APP_ID = 1 (VC1-SOH) WITH PACKET RATE LT 30 N_GAPS 1 GAP START TIME GAP END TIME GAP (SEC) 2010-07-25T14:35:00.000 -- 2010-07-26T00:00:00.000 33900.000 GAPS IN APP_ID = 154 (VC1-PMTRAS) WITH PACKET RATE LT 4 N_GAPS 1 GAP START TIME GAP END TIME GAP (SEC) 2010-07-25T14:40:00.000 -- 2010-07-26T00:00:00.000 33600.000 GAPS IN APP_ID = 102 (VC3-MONITOR RATES) WITH PACKET RATE LT 30 N_GAPS 1 GAP START TIME GAP END TIME GAP (SEC) 2010-07-25T14:35:00.000 -- 2010-07-25T17:55:00.000 12000.000 DATA GAPS FOR 2010/07/26 TIME RANGE: 2010-07-26T00:00:00.000 -- 2010-07-27T00:00:00.000 GAPS IN APP_ID = 1 (VC1-SOH) WITH PACKET RATE LT 30 N_GAPS 2 GAP START TIME GAP END TIME GAP (SEC) 2010-07-26T00:00:00.000 -- 2010-07-26T09:50:00.000 35400.000 2010-07-26T14:35:00.000 -- 2010-07-26T14:40:00.000 300.00000 GAPS IN APP_ID = 154 (VC1-PMTRAS) WITH PACKET RATE LT 4 N_GAPS 1 GAP START TIME GAP END TIME GAP (SEC) 2010-07-26T00:00:00.000 -- 2010-07-26T09:50:00.000 35400.000 GAPS IN APP_ID = 102 (VC3-MONITOR RATES) WITH PACKET RATE LT 30 N_GAPS 3 GAP START TIME GAP END TIME GAP (SEC) 2010-07-26T10:00:00.000 -- 2010-07-26T10:05:00.000 300.00000 2010-07-26T11:20:00.000 -- 2010-07-26T12:10:00.000 3000.0000 2010-07-26T23:55:00.000 -- 2010-07-27T00:00:00.000 300.00000
Others
A Gamma Ray Burst was observed by RHESSI on July 24th around 00:40:00 UT, lasting 2-3 min. Excellent RHESSI coverage. Also observed by Swift, Konus, INTEGRAL, and Suzaku.