Tohban Report 2017-04-19

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|tohban_name = Milo Buitrago-Casas
|tohban_name = Milo Buitrago-Casas
|tohban_email = milo@ssl.berkeley.edu
|tohban_email = milo@ssl.berkeley.edu
-
|next_tohban  = TBD
+
|next_tohban  = Jim McTiernan
}}
}}
== Solar Activity ==
== Solar Activity ==
-
The Sun was active this week, producing seven M-class flares. Currently there are five AR on disk, but four of them are expected to rotate off the disk very soon.
+
The Sun was active this week, producing a handful of B-class flares and two C-flares, one yesterday and one this morning. Currently, there is one AR peeping out on the Est limb and is expected to remain on disk this coming week with a slight chance to host  M-class flares.
How many GOES flares occurred?
How many GOES flares occurred?
-
   Flares above B, C, M, X class were    39    30     7     0
+
   Flares above B, C, M, X class were    18     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    21    17     5     0
+
   Flares above B, C, M, X class were     8     1     0     0
And how many had EXCELLENT coverage?
And how many had EXCELLENT coverage?
-
   Flares above B, C, M, X class were    12    11     2     0
+
   Flares above B, C, M, X class were     0     0     0     0
   
   
-
There were RHESSI flares/GOES flares         188 /          76
+
There were RHESSI flares/GOES flares         22 /          19
-
over the time range 28-Mar-17 04-Apr-17
+
over the time range 11-Apr-17 18-Apr-17
-
 
+
== Memory Management ==
== Memory Management ==
-
Early the week, the SSR was quiet high ~40% at due to the four detectors that were on last week. After turning off detectors 1 and 8 on April 12, the SSR was gradually emptying reaching a minimum of 9% at the end of the day on Monda April 17. In response to the rotation on the disk of a big Active Region, detectors 1 and 8 were turned on again so the SSR is expected to gradually increase this week.
+
Early this week, the SSR was quite high ~40% at due to the four detectors that were on last week. After turning off detectors 1 and 8 on April 12, the SSR was gradually emptying reaching a minimum of 9% at the end of the day on Monda April 17. In response to the rotation on the disk of a big Active Region, detectors 1 and 8 were turned on again so the SSR is expected to gradually increase this week. Currently, it is at 18.4%.
== Spacecraft Status ==
== Spacecraft Status ==
-
Detectors 3 and 6 are recording events. Due to the increased solar activities, 1, and 8 were turned on.
+
Detectors 3 and 6 are recording events. Due to a big active region on the solar disk, detectors 1 and 8 were turned on.
-
The cold tips are 129.5 and 128.0 K as of 5-Apr-2017. The cold plates, 1 and 2 are 153.3 and 151.8 K. Cryocooler power is steady at 76W.  
+
The cold tips are 127.3 and 125.1 K as of 19-Apr-2017. The cold plates, 1 and 2 are 152.5 and 151.0 K. Cryocooler power is steady at 74.9W.  
See:
See:
Line 41: Line 40:
Relatively large (>300 sec) data gaps as follows:
Relatively large (>300 sec) data gaps as follows:
-
GAPS IN APP_ID = 102 (VC3-MONITOR RATES) WITH PACKET RATE LT 30
 
  GAP START TIME              GAP END TIME                  GAP (SEC)
  GAP START TIME              GAP END TIME                  GAP (SEC)
-
2017-03-30T19:40:00.000 -- 2017-03-30T20:05:00.000      1500.0000
+
  2017-04-15T17:25:00.000 -- 2017-04-15T22:40:00.000      18900.000
-
  2017-04-02T06:00:00.000 -- 2017-04-02T06:25:00.000      1500.0000
+
  2017-04-15T17:25:00.000 -- 2017-04-15T22:35:00.000      18600.000
-
  2017-04-02T11:55:00.000 -- 2017-04-02T12:10:00.000      900.00000
+
  2017-04-13T13:50:00.000 -- 2017-04-13T14:00:00.000      600.00000
-
  2017-04-03T21:05:00.000 -- 2017-04-03T21:20:00.000      900.00000
+
-
2017-04-03T21:25:00.000 -- 2017-04-04T00:00:00.000      9300.0000
+
== Detector issues ==
== Detector issues ==
-
Detectors 1, 3, 6 and 8 are powered on, and are recording events. While the AR2644 that produced M-class flares is now at the limb, there is still another big AR on disk. So it was determined to keep the detectors 1 and 8 on unless there is an issue with the temperatures.  
+
Because the moderate solar activity early this week, and the presence of a new active region on the Est solar limb, it was decided to turn on detectors 1 and 8 the past Monday Abril 17 around 21:30UT. Temperatures on the cold plates and tips looked stable during the last couple of days after turning on those two detectors. Also the SSR filling level has been rather low (~15% at the end of the passes).
 +
 
 +
Commanding were the follow:
 +
 
 +
2017-107-21:31:18 start idib_on_g1
 +
2017-107-21:31:35 start idib_on_g8
 +
2017-107-21:32:05 start ihv_ramp_stage2_g1 ; 1000 V
 +
2017-107-21:32:20 start ihv_ramp_stage2_g8 ; 1000 V
 +
 
 +
17-107-23:09:42 start ihv_ramp_stage3_g1
 +
17-107-23:09:58 start ihv_ramp_stage3_g8
 +
 
 +
17-107-23:14:37 start sc_ssr_rtime halted
 +
 
 +
17-108-00:40:32 start idib_chg_thrshld(8, FRONT, FAST, 0x90)
 +
17-108-00:40:36 /IDPUDUMPTABL TABLE=DIBTBL8
 +
17-108-00:40:36 /IDPUTABLE8 OFFSET=FRONTFASTDAC
 +
17-108-00:41:06 /IDPULOAD VALUE=0x90
 +
 
 +
17-108-00:43:46 start idib_chg_thrshld(1, FRONT, FAST, 0x80)
 +
17-108-00:43:49 /IDPUDUMPTABL TABLE=DIBTBL1
 +
17-108-00:43:49 /IDPUTABLE1 OFFSET=FRONTFASTDAC
 +
17-108-00:43:58 /IDPULOAD VALUE=0x80
 +
 
 +
17-108-00:45:22 start idib_chg_thrshld(1, REAR, FAST, 0x60)
 +
17-108-00:45:26 /IDPUDUMPTABL TABLE=DIBTBL1
 +
17-108-00:45:27 /IDPUTABLE1 OFFSET=REARFASTDAC
 +
17-108-00:45:34 /IDPULOAD VALUE=0x60
 +
 
 +
17-108-00:49:52 start sc_ssr_rtime halted
 +
 
 +
Detectors 1, 3, 6 and 8 are on and working. There is a new active region on disk (AR2651) that produced a C-class flare this morning and will remain active for the next couple of days. So it was determined to keep the detectors 1 and 8 on unless there is an issue with the temperatures.
== Notes ==
== Notes ==
-
For the flare of April 3 14UT, pileup was relatively high (40% at 30 keV) with the attenuator state A1. It was decided to revisit the current thresholds of the thin/thick attenuator logic.
+
There was an explained attenuator change on 13 April 2017 at 13:55 UT.  Albert's best guess is that this is (at least partially) corrupted data. At first glance, there is not any other explanation for why the front-decimation level could vary so wildly on short timescales, from minimal decimation to throwing out ~255/256 of counts.  In the corresponding lightcurve plot one orbit earlier, the decimation level also appears to change during eclipse, which is weird as well. Further investigation is needed.
== Spacecraft Management ==
== Spacecraft Management ==
Line 76: Line 103:
| Attenuator operation || None
| Attenuator operation || None
|-
|-
-
| Detector problems? || None
+
| Detector problems? || See notes above.
|}
|}

Latest revision as of 18:40, 19 April 2017


Tohban Reports
Start Date: 29 March 2017
End Date: 5 April 2017
Tohban: Milo Buitrago-Casas
Tohban email: milo@ssl.berkeley.edu
Next Tohban: Jim McTiernan
List all reports



Contents

Solar Activity

The Sun was active this week, producing a handful of B-class flares and two C-flares, one yesterday and one this morning. Currently, there is one AR peeping out on the Est limb and is expected to remain on disk this coming week with a slight chance to host M-class flares.

How many GOES flares occurred?

 Flares above B, C, M, X class were     18     1     0     0

And how many of these are listed in the RHESSI flare list?

 Flares above B, C, M, X class were      8     1     0     0

And how many had EXCELLENT coverage?

 Flares above B, C, M, X class were      0     0     0     0

There were RHESSI flares/GOES flares 22 / 19 over the time range 11-Apr-17 18-Apr-17

Memory Management

Early this week, the SSR was quite high ~40% at due to the four detectors that were on last week. After turning off detectors 1 and 8 on April 12, the SSR was gradually emptying reaching a minimum of 9% at the end of the day on Monda April 17. In response to the rotation on the disk of a big Active Region, detectors 1 and 8 were turned on again so the SSR is expected to gradually increase this week. Currently, it is at 18.4%.

Spacecraft Status

Detectors 3 and 6 are recording events. Due to a big active region on the solar disk, detectors 1 and 8 were turned on.

The cold tips are 127.3 and 125.1 K as of 19-Apr-2017. The cold plates, 1 and 2 are 152.5 and 151.0 K. Cryocooler power is steady at 74.9W. See:

http://sprg.ssl.berkeley.edu/~ayshih/soh/latest_temperatures.pdf

for a summary plot of recent temperatures, efficiencies and accelerometer values.

Data Gaps

Relatively large (>300 sec) data gaps as follows:

GAP START TIME              GAP END TIME                   GAP (SEC)
2017-04-15T17:25:00.000 -- 2017-04-15T22:40:00.000       18900.000
2017-04-15T17:25:00.000 -- 2017-04-15T22:35:00.000       18600.000
2017-04-13T13:50:00.000 -- 2017-04-13T14:00:00.000       600.00000

Detector issues

Because the moderate solar activity early this week, and the presence of a new active region on the Est solar limb, it was decided to turn on detectors 1 and 8 the past Monday Abril 17 around 21:30UT. Temperatures on the cold plates and tips looked stable during the last couple of days after turning on those two detectors. Also the SSR filling level has been rather low (~15% at the end of the passes).

Commanding were the follow:

2017-107-21:31:18 start idib_on_g1
2017-107-21:31:35 start idib_on_g8
2017-107-21:32:05 start ihv_ramp_stage2_g1 ; 1000 V
2017-107-21:32:20 start ihv_ramp_stage2_g8 ; 1000 V
17-107-23:09:42 start ihv_ramp_stage3_g1
17-107-23:09:58 start ihv_ramp_stage3_g8
17-107-23:14:37 start sc_ssr_rtime halted
17-108-00:40:32 start idib_chg_thrshld(8, FRONT, FAST, 0x90)
17-108-00:40:36 /IDPUDUMPTABL TABLE=DIBTBL8
17-108-00:40:36 /IDPUTABLE8 OFFSET=FRONTFASTDAC
17-108-00:41:06 /IDPULOAD VALUE=0x90
17-108-00:43:46 start idib_chg_thrshld(1, FRONT, FAST, 0x80)
17-108-00:43:49 /IDPUDUMPTABL TABLE=DIBTBL1
17-108-00:43:49 /IDPUTABLE1 OFFSET=FRONTFASTDAC
17-108-00:43:58 /IDPULOAD VALUE=0x80
17-108-00:45:22 start idib_chg_thrshld(1, REAR, FAST, 0x60)
17-108-00:45:26 /IDPUDUMPTABL TABLE=DIBTBL1
17-108-00:45:27 /IDPUTABLE1 OFFSET=REARFASTDAC
17-108-00:45:34 /IDPULOAD VALUE=0x60
17-108-00:49:52 start sc_ssr_rtime halted


Detectors 1, 3, 6 and 8 are on and working. There is a new active region on disk (AR2651) that produced a C-class flare this morning and will remain active for the next couple of days. So it was determined to keep the detectors 1 and 8 on unless there is an issue with the temperatures.

Notes

There was an explained attenuator change on 13 April 2017 at 13:55 UT. Albert's best guess is that this is (at least partially) corrupted data. At first glance, there is not any other explanation for why the front-decimation level could vary so wildly on short timescales, from minimal decimation to throwing out ~255/256 of counts. In the corresponding lightcurve plot one orbit earlier, the decimation level also appears to change during eclipse, which is weird as well. Further investigation is needed.

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 None
Detector problems? See notes above.
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