MTA Monitoring Report 10/29/21 - 11/04/21

Archive of all weekly reports
Archive of monthly reports


Radiation

Several shocks related to C-class flares passed over the weekend including one on Saturday Oct 30 and a bigger one on Sunday Oct 31. An M1.7 class flare on Tue, Nov 2, also produced an Earth directed CME. This resulted in a sharp increase in the ACE P3 rates which reached ~10,000, putting ACIS on track to exceed the attenuated orbital fluence limit of 2e9 by >~50%. ACIS requested a radiation shutdown meeting on Wed, Nov 3, at 5:30PM EST. At 6:40PM EST, comm was established, autonomous safing had not occurred. FD and ACIS continued to monitor the situation but no action was required, the ACE P3 rates stayed at ~80,000. ACIS would have received about 1/2 its threshold orbital dose over the next 4 hours before radzone SIM translation if the rates did not go down. Geomagnetic field stayed unsettled until the end of the week, and the ACE P3 rates stayed elevated with a decreasing trend.

Detrended CTI

Although we prefer to quote CTI values of the cleanest data (FT <= -119.7 C, int time > 7000sec), the data that fulfills these conditions are getting rare. We now quote CTI based on temperature corrected data for Focal plane temperature <= -118.5 C).

The unit is now CTI/year not CTI/day.

Average of ACIS-I CCDs (MnKa) slope: 5.518e-02 CTI/year (1.512e-04 CTI/day)
Detrended slope: 6.019e-02 CTI/year (1.649e-04 CTI/day)

ACIS Warm Pixels

We display all bad pixels that have showed up in past, and, if any, previously unknown bad pixels appeared in the last 14 days. We also list hot pixels (defined as 1000 above the average of bias background). Warm columns 509-514 are probably due to boundaries.

New definitions of warm pixels and flickering pixels (May 15, 2014). If a pixel displays the level beyond a threshold for more than 70% of the time in the past two weeks, the pixel is categorized as a "warm" pixel. If a pixel is above the threshold more than 30% of time but less than 70% of the time in the past two weeks, the pixel is categorized as a "flickering" pixel.

 CCD0CCD1CCD2CCD3CCD4CCD5CCD6CCD7CCD8CCD9
Previously Unknown Bad Pixels         (52,386)          
Current Warm Pixels (143,700) (154,9) (802,665) (910,239) (178,149) (526,66) (726,537) (21,95)       (335,412)    
Flickering Warm Pixels   (427,125) (665,25)       (670,387) (1000,214) (884,31)   (275,393)  
Current Hot Pixels                    
Flickering Hot Pixels                    
Warm column candidates           512 1022 510   512 1022    
Flickering Warm column candidates                    

ACIS Focal Plane Temperature

For this period, 10 peaks are observed.

Weekly focal plane temperature with sun angle, earth angle, and altitude overplotted. Sun angle is the solar array angle, that is the angle between the sun and the optical axis (+X axis). The earth angle is the angle between earth and the ACIS radiator (+Z axis). Altitude varies from 34 kkm to 128 kkm.



SIM Movements

8 TSC moves this period

Telemetry

New violations or new extrema are shown in blue cells.

MSID 10/29/21 10/30/21 10/31/21 11/01/21 11/02/21 11/03/21 11/04/21 yellow limits
(lower)
upper
red limits
(lower)
upper
Units Description
ELBI       66.09       (20.0)
60.0
(13.0)
66.0
AMPLOAD BUS CURRENT (HIGH RANGE)
ESAMYI (0.06)     (0.06)     (0.06) (6.0)
27.0
(5.62)
33.0
AMPS/A -Y CURRENT
OBADIAGRAD 4.16 4.07 4.33 4.34 4.30 4.28 4.14 (-1.11)
3.5
(-2.78)
3.9
KOBA DIAM GRAD
OBACONEAVG   305.45 302.42 301.39 306.48 305.82 304.00 (282.5)
300.0
(281.8)
301.0
KOBA CONE AVG TEMP
TSCTSF3 (267.70) (268.06)     (268.06) (267.70)   (278.15)
359.15
(269.15)
483.15
KSC-TS FITTING -3 TEMP
OBAAVG 303.60 301.89     302.53 302.01   (282.5)
300.0
(281.4)
301.0
KOBA/TFTE TEMP
MZOBACONE 309.89       308.93 308.38   (260.2)
303.0
(250.2)
308.0
CONE-Z SIDE OBA CONE
CTXBPWR     (0.00) (0.00)       (36.12)
37.0
(36.0)
38.0
DBMTRANSMITTER B OUTPUT POWER
TCM_TX1 (268.79)   (268.43)     (268.79) (267.70) (283.15)
348.15
(269.15)
404.15
KTRANSPONDER-1 EXT BPL TEMP
HRMAAVG 309.26 309.28 309.03         (306.0)
308.0
(305.0)
309.0
KAVG OF HRMA METRICS


IRUs

Gyro Bias Drift Gyro Bias Drift Histogram

Recent Observations

OBSID DETECTOR GRATING TARGET ANALYSIS ACA
26166 ACIS-0123 NONE RMJ022905.6+043003.1 OK OK
23579 ACIS-7 NONE GRB211023B OK OK
26183 ACIS-7 NONE IGR J02341+0228 OK OK
26169 ACIS-7 NONE MAXI J1848-015 OK OK
26187 ACIS-7 NONE MAXI J1848-015 OK OK
26186 ACIS-0123 NONE RMJ010721.8+141623.6 OK OK
25295 ACIS-23567 NONE ESO 528-G 036 OK OK
23856 ACIS-01236 NONE SPT-CLJ2355-6002 OK OK
25444 ACIS-23678 NONE NGC 1090 OK OK
25459 ACIS-23678 NONE NVSS J003659+183203 OK OK
23458 ACIS-7 NONE MAXI J1848-015 OK OK
26067 ACIS-0123 NONE PSZ2G176.25-52.57 OK OK
25460 ACIS-678 NONE B2 0135+29 OK OK
25061 ACIS-3678 NONE SNR 0519-69.0 OK OK
25464 ACIS-678 NONE B3 1520+437 OK OK
24481 ACIS-5678 HETG 4U0114+65 OK/NA OK
25179 ACIS-7 NONE SN1986J OK OK
26174 ACIS-678 NONE B2.1 0241+30 Missing Missing
26116 ACIS-0123 NONE eMACSJ1508.1+5755 OK OK
26180 ACIS-456789 HETG 4U0114+65 OK/NA OK

Trending

This week's focus is Gratings

Last reported on Aug 19.

Only the most interesting or representative msids are shown below. For a full listing choose the bulletted link.


MSIDMeanRMSDelta/YrDelta/Yr/YrUnitDescription
4hposaro -0.0100.03368.52 +/- 19.851.17 +/- 0.94naNA
4hposbro -0.0050.03369.11 +/- 20.071.18 +/- 0.95naNA
4lposaro 0.0130.02173.81 +/- 12.860.39 +/- 0.56naNA
4lposbro 0.0220.02272.88 +/- 13.230.30 +/- 0.57naNA
4mp28av 0.0100.0010.38 +/- 0.720.00 +/- 0.03VMCE A: +28 VOLT MONITOR
4mp28bv 0.0640.0051.88 +/- 3.060.01 +/- 0.13VMCE B: +28 VOLT MONITOR
4mp5av 0.0160.0010.45 +/- 0.740.01 +/- 0.03VMCE A: +5 VOLT MONITOR
4mp5bv 0.0119.126e-040.34 +/- 0.560.00 +/- 0.02VMCE B: +5 VOLT MONITOR


If you have any questions, please contact: swolk@head.cfa.harvard.edu