MTA Monitoring Report 03/24/17 - 03/30/17

Archive of all weekly reports
Archive of monthly reports


Radiation

Quiet

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: 1.317e-02 CTI/year (3.609e-05 CTI/day)
Detrended slope: 1.552e-02 CTI/year (4.251e-05 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                    
Current Warm Pixels (692,141) (153,205) (143,700) (910,239) (802,665) (726,537) (680,391) (847,364) (21,95)   (357,303) (369,376) (161,206) (1000,214) (335,412)    
Flickering Warm Pixels   (427,125) (526,66) (318,53)   (607,281) (669,577) (263,317) (280,313) (367,511) (341,427) (884,31)   (182,474) (197,241) (356,902) (881,53) (139,109)  
Current Hot Pixels                    
Flickering Hot Pixels                    
Warm column candidates           510 512 1022   512 1022    
Flickering Warm Column Candidates                    

ACIS Focal Plane Temperature

For this period, 7 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

14 TSC moves this period

Telemetry

New violations or new extrema are shown in blue cells.

MSID 03/24/17 03/25/17 03/26/17 03/27/17 03/28/17 03/29/17 03/30/17 yellow limits
(lower)
upper
red limits
(lower)
upper
Units Description
HRMACAV (284.85) (284.85) (284.85)   (284.85) (284.85) (284.85) (293.4)
294.8
(292.8)
295.5
TEMP # HRMA CAVITY AVG
MZOBACONE   (221.33)   (221.33)       (260.2)
303.0
(250.2)
308.0
CONE # -Z SIDE OBA
MZOBACONE       303.31       (260.2)
303.0
(250.2)
308.0
CONE # -Z SIDE OBA
PZOBACONE   (198.92)           (260.2)
303.0
(250.2)
308.0
CONE # +Z SIDE OBA
TFTERANGE (0.00) (0.00) (0.00) (0.00)   (0.00) (0.00) (16.7)
34.5
(11.1)
42.0
K # TFTE VENT/RAD TEMP
TFTERANGE 35.76 35.10 34.61 36.57 36.80 36.12 35.85 (16.7)
34.5
(11.1)
42.0
K # TFTE VENT/RAD TEMP
SCSTRUTRNGE         22.58     (-0.5)
22.2
(-1.0)
38.8
K # SC STRUT TEMP
5EPHINT 344.30 342.31 337.94 346.96 346.96 344.30 339.58 (261.15)
300.15
(258.15)
303.15
K #EPHIN TEMP
HKP5V (5.06) (5.06) (5.06) (5.06) (5.06) (5.06)   (5.08)
5.15
(5.06)
5.17
V #HK 5 Volts Rail - Voltage
HKEBOXTEMP 350.47 349.02 345.00 351.98 353.56 349.02 345.00 (268.15)
336.15
(253.15)
346.15
K #EPHIN HOUSEKEEPING EBOX: TEMPERATURE (5EHSE300)
IMHVLV (80.00) (80.00) (99.00) (80.00) (80.00) (99.00) (99.00) (126.0)
128.0
(125.0)
129.0
(2IMHVLV) #Imaging bot MCP HV monitor
IMHBLV (87.00) (87.00) (105.00) (87.00) (87.00) (105.00) (105.00) (126.0)
128.0
(125.0)
129.0
(2IMHBLV) #Imaging bot and top MCP HV monitor
S2HVLV (83.00) (83.00) (83.00) (64.00) (83.00) (83.00) (83.00) (126.0)
128.0
(125.0)
129.0
(2S2HVLV) #Shield PMT 2 HV monitor
LLDIALV (129.00)             (130.0)
132.0
(129.0)
133.0
(2LLDIALV) #Lower level disc setting
RSRFALV 185.00 185.00 185.00 185.00 185.00 185.00 185.00 (172.0)
174.0
(171.0)
175.0
V #Range switch setting (2RSRFALV)
3FLCABPT 294.46   293.45         (253.15)
293.15
(235.65)
310.65
K #FLCA BASEPLATE (+X)
3TSMXCET 278.28 285.76 278.28 283.26 280.77 275.78 283.26 (153.15)
263.15
(148.15)
353.15
K #-X TURTLE SHELL NR HRC CEA
3TSMXSPT 318.18 318.18 315.69 315.69 315.69 315.69 313.19 (203.15)
283.15
(148.15)
353.15
K #-X TURTLE SHELL NR ACIS SS
3TSMYDPT 265.81             (203.15)
263.15
(148.15)
353.15
K #-Y TURTLE SHELL NR ACIS DPA
3TSPZSPT 293.24             (233.15)
293.15
(148.15)
353.15
K #+Z TURTLE SHELL NR ACIS SS
ESAPYI         (0.14)     (7.5)
27.5
(6.5)
33.0
AMP #S/A +Y CURRENT
ESAPYI         28.72     (7.5)
27.5
(6.5)
33.0
AMP #S/A +Y CURRENT
TAPE2PST (293.57)     (293.57) (294.00) (293.57) (293.57) (323.15)
330.15
(318.15)
335.15
K #PEA-2 POWER SUPPLY TEMP
TSAMYT         (304.78)     (369.35)
440.15
(366.15)
473.15
K #-Y WING SOLAR ARRAY TEMP
TSAPYT         (304.78)     (369.35)
440.15
(366.15)
473.15
K #+Y WING SOLAR ARRAY TEMP
4PRT3AT (258.46) (258.46) (258.46) (258.46) (258.46) (258.46) (258.46) (273.15)
283.15
(53.15)
368.15
K #IP A: PRE-COLLIMATOR PRT 3 TEMPERATURE


IRUs

Recent Observations

OBSID DETECTOR GRATING TARGET ANALYSIS ACA
19851 ACIS-7 NONE E0102-72 CAL OK
19732 ACIS-678 NONE W0533-3401 OK OK
18948 ACIS-235678 NONE 2MASS J03103891+2540535 OK OK
20045 ACIS-0123 NONE SDSSJ1030+0524 OK OK
20042 ACIS-2367 NONE SNR 0509-68.7 OK OK
20043 ACIS-01236 NONE Cygnus A - W Hotspot OK OK
20046 ACIS-0123 NONE SDSSJ1030+0524 OK OK
19525 ACIS-7 NONE 2MASS J041146+132416 OK OK
19852 ACIS-7 NONE E0102-72 CAL OK
20044 ACIS-01236 NONE Cygnus A - W Hotspot OK OK
19718 ACIS-56789 HETG GRS 1915+105 CC OK
18676 HRC-I NONE Jupiter OK OK
20055 ACIS-35678 NONE SN2017cbv OK OK
20022 ACIS-456789 HETG Mkn 876 OK OK
18234 ACIS-23678 NONE NGC 4848 OK OK
20047 ACIS-456789 HETG Mkn 876 OK OK
20049 ACIS-23678 NONE NGC 4848 OK OK
17137 ACIS-01236 NONE Cygnus A - W Hotspot OK OK
20050 ACIS-23678 NONE NGC 4848 OK OK
19479 ACIS-35678 NONE spog2178 OK OK
19627 ACIS-23678 NONE QJ0158-4325 OK OK

Trending

This week's focus is Spacecraft Bus and Subsystem Trends

Last reported on Jan 05.

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

Min/max envelopes in dark blue appear on the trending plots. The envelopes are 4th degree fits to the monthly minimum and maximum values for each MSID. The final polynomial form and binning are still being experimented with. We will soon add to the trending pages a report of the fits and predictions they give on future limit violations. The light blue curve is our original smoothing of all the data over 30 day moving boxcars. The green/yellow line is a linear fit to all the data; the break occurs at a limit change.









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