MTA Monitoring Report 06/16/17 - 06/22/17

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: 1.332e-02 CTI/year (3.650e-05 CTI/day)
Detrended slope: 1.619e-02 CTI/year (4.436e-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     (726,537) (21,95)   (357,303) (369,376) (161,206) (1000,214) (335,412)    
Flickering Warm Pixels (692,141) (667,782) (153,205) (143,700) (910,239) (802,665)   (680,391) (847,364) (419,163) (885,460) (758,244) (247,364) (669,577) (607,281) (263,317) (280,313) (367,511) (258,797) (341,427)     (182,474) (197,241) (881,53) (139,109) (150,374) (636,819)
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, 4 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

16 TSC moves this period

Telemetry

New violations or new extrema are shown in blue cells.

MSID 06/16/17 06/17/17 06/18/17 06/19/17 06/20/17 06/21/17 06/22/17 yellow limits
(lower)
upper
red limits
(lower)
upper
Units Description
1PIN1AT 344.99 344.99 344.99 344.99 344.99 344.99 344.99 (-20.0)
30.0
(-36.5)
36.5
C # PSMC TEMP 1A
HRMACAV (284.85) (284.85)   (287.95) (284.85)     (293.4)
294.8
(292.8)
295.5
TEMP # HRMA CAVITY AVG
MZOBACONE         (221.33)     (260.2)
303.0
(250.2)
308.0
CONE # -Z SIDE OBA
MZOBACONE         303.03     (260.2)
303.0
(250.2)
308.0
CONE # -Z SIDE OBA
TFTERANGE   (0.00) (0.00)   (0.00) (0.00) (0.00) (16.7)
34.5
(11.1)
42.0
K # TFTE VENT/RAD TEMP
TFTERANGE   34.52 35.51 35.80 35.81 36.74 34.56 (16.7)
34.5
(11.1)
42.0
K # TFTE VENT/RAD TEMP
5EPHINT   341.22 341.76 344.96 341.22 345.63 334.66 (261.15)
300.15
(258.15)
303.15
K #EPHIN TEMP
HKP5V     (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   346.29 347.63 350.47 347.63 351.98 341.39 (268.15)
336.15
(253.15)
346.15
K #EPHIN HOUSEKEEPING EBOX: TEMPERATURE (5EHSE300)
IMHBLV (105.00) (105.00) (87.00) (32.00) (87.00) (105.00) (33.00) (126.0)
128.0
(125.0)
129.0
(2IMHBLV) #Imaging bot and top MCP HV monitor
IMHBLV       192.00       (126.0)
128.0
(125.0)
129.0
(2IMHBLV) #Imaging bot and top MCP HV monitor
SPHBLV       (15.00)     (32.00) (79.0)
128.0
(78.0)
129.0
(2SPHBLV) #Spect bot and top MCP HV monitor
S2HVLV (83.00) (83.00) (82.00) (64.00) (83.00) (83.00) (83.00) (126.0)
128.0
(125.0)
129.0
(2S2HVLV) #Shield PMT 2 HV monitor
RSRFALV 185.00 185.00 186.00 190.00 185.00 185.00 190.00 (172.0)
174.0
(171.0)
175.0
V #Range switch setting (2RSRFALV)
3TSMXCET 278.28 278.28 280.77 275.78 280.77 278.28 273.29 (153.15)
263.15
(148.15)
353.15
K #-X TURTLE SHELL NR HRC CEA
3TSMXSPT 313.19 315.69 318.18 313.19 313.19 315.69 313.19 (203.15)
283.15
(148.15)
353.15
K #-X TURTLE SHELL NR ACIS SS
TAPE2PST         (293.57) (293.57)   (323.15)
330.15
(318.15)
335.15
K #PEA-2 POWER SUPPLY TEMP
4PRT3AT (258.46) (258.46) (259.14) (258.46) (259.14) (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
20096 ACIS-456789 HETG IC4329a OK OK
18106 ACIS-56789 NONE 4C63.20 OK OK
19136 ACIS-7 NONE CXO J164710.2-455216 OK OK
20099 ACIS-67 HETG GX340+0 OK OK
19572 ACIS-01236 NONE PKS 0745-191 North OK OK
19573 ACIS-01236 NONE PKS 0745-191 West OK OK
19574 ACIS-01236 NONE PKS 0745-191 South OK OK
19575 ACIS-01236 NONE PKS 0745-191 East OK OK
18990 ACIS-5678 HETG Cr X-1 OK OK
20097 ACIS-456789 HETG IC4329a OK OK
20093 ACIS-5678 HETG Cr X-1 OK OK
18953 ACIS-235678 NONE IGR J16479-4514 OK OK
19843 HRC-S NONE Vega CAL OK
18921 ACIS-0123 NONE IRDC G35.4-0.33 OK OK
19841 HRC-I NONE Vega CAL OK
19952 ACIS-456789 HETG Vela X-1 OK OK
18982 ACIS-012367 NONE IGR J16482-2959 OK OK
20104 ACIS-35678 NONE NGC 6338 OK OK
19526 ACIS-7 NONE Mrk 504 OK OK
20100 ACIS-0123 NONE IRDC G35.4-0.33 OK OK
19559 ACIS-23678 NONE SDSSJ234145.51-004640.5 OK OK
19853 ACIS-456789 HETG MKN421 CAL OK
19854 ACIS-56789 LETG MKN421 CAL OK
19855 HRC-S LETG MKN421 CAL OK
19856 ACIS-56789 LETG MKN421 CAL OK
19857 HRC-S LETG MKN421 CAL OK
19858 ACIS-56789 LETG MKN421 CAL OK

Trending

This week's focus is Spacecraft Bus and Subsystem Trends

Last reported on Mar 30.

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