MTA Monitoring Report 07/13/18 - 07/19/18

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: 1.378e-02 CTI/year (3.776e-05 CTI/day)
Detrended slope: 1.754e-02 CTI/year (4.805e-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     (178,149) (21,95)       (335,412)    
Flickering Warm Pixels (692,141) (143,700) (427,125) (910,239) (802,665) (726,537) (811,637) (680,391) (318,53) (419,163) (758,244) (247,364) (233,227) (607,281) (357,303) (369,376) (282,385) (263,317) (161,206) (745,313) (341,427) (1000,214)   (182,474) (197,241) (881,53) (40,49) (636,819) (65,23)
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, 5 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

13 TSC moves this period

Telemetry

New violations or new extrema are shown in blue cells.

MSID 07/13/18 07/14/18 07/15/18 07/16/18 07/17/18 07/18/18 07/19/18 yellow limits
(lower)
upper
red limits
(lower)
upper
Units Description
HRMACAV (284.85) (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           (253.98) (242.69) (260.2)
303.0
(250.2)
308.0
CONE # -Z SIDE OBA
MZOBACONE           304.15 303.07 (260.2)
303.0
(250.2)
308.0
CONE # -Z SIDE OBA
TFTERANGE   (0.00) (0.00) (0.00) (0.00)     (16.7)
37.5
(11.1)
45.0
K # TFTE VENT/RAD TEMP
TFTERANGE       37.99       (16.7)
37.5
(11.1)
45.0
K # TFTE VENT/RAD TEMP
IMHVLV (45.00)   (80.00) (80.00) (99.00) (99.00) (99.00) (126.0)
128.0
(125.0)
129.0
(2IMHVLV) #Imaging bot MCP HV monitor
IMHBLV     (87.00) (37.00) (105.00) (105.00) (105.00) (126.0)
128.0
(125.0)
129.0
(2IMHBLV) #Imaging bot and top MCP HV monitor
SPHBLV (38.00) (78.00)           (79.0)
128.0
(78.0)
129.0
(2SPHBLV) #Spect bot and top MCP HV monitor
S2HVLV (82.00) (83.00) (82.00) (82.00) (83.00) (83.00) (83.00) (126.0)
128.0
(125.0)
129.0
(2S2HVLV) #Shield PMT 2 HV monitor
LLDIALV (30.00)             (130.0)
132.0
(129.0)
133.0
(2LLDIALV) #Lower level disc setting
LLDIALV 133.00             (130.0)
132.0
(129.0)
133.0
(2LLDIALV) #Lower level disc setting
RSRFALV (0.00)     (16.00)       (172.0)
174.0
(171.0)
175.0
V #Range switch setting (2RSRFALV)
RSRFALV 190.00 190.00 190.00 186.00 185.00 185.00 185.00 (172.0)
174.0
(171.0)
175.0
V #Range switch setting (2RSRFALV)
PRBSCR (-8.65)             (1.24)
1.92
(0.90)
2.26
AMP #Primary bus current (2PRBSCR)
IMINATM (-57.30)             (-12.0)
35.0
(-15.0)
40.0
C #Imaging det temperature (2IMINATM)
IMINATM 84.20             (-12.0)
35.0
(-15.0)
40.0
C #Imaging det temperature (2IMINATM)
SMTRATM (-51.65)             (-17.0)
45.0
(-20.0)
50.0
C #Selected motor temperature (2SMTRATM)
3TSMXCET 278.28 283.26 280.77 283.26 283.26 283.26 280.77 (153.15)
263.15
(148.15)
353.15
K #-X TURTLE SHELL NR HRC CEA
3TSMXSPT 659.89 659.89 659.89 659.89 659.89 659.89 659.89 (203.15)
283.15
(148.15)
353.15
K #-X TURTLE SHELL NR ACIS SS
ELBI 66.35 63.20 65.82 62.68 63.73 63.99 64.25 (16.0)
50.0
(13.0)
66.0
AMP #LOAD BUS CURRENT (ELBI_LOW)
TAPE2PST       (292.71)   (291.85) (292.71) (323.15)
330.15
(318.15)
335.15
K #PEA-2 POWER SUPPLY 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
20556 ACIS-01236 NONE Abell 2146 OK OK
21123 ACIS-5678 HETG 4U 1907+09 OK OK
21124 ACIS-5678 HETG 4U 1907+09 OK OK
20710 ACIS-56789 HETG MKN421 CAL OK
20711 ACIS-56789 LETG MKN421 CAL OK
20712 HRC-S LETG MKN421 CAL OK
20713 ACIS-56789 LETG MKN421 CAL OK
20714 HRC-S LETG MKN421 CAL OK
20715 ACIS-56789 LETG MKN421 CAL OK
20717 ACIS-56789 HETG MKN421 CAL OK
21125 ACIS-5678 HETG 4U 1907+09 OK OK
19676 ACIS-01237 NONE CDWFS OK OK
19602 ACIS-7 NONE MXB 1659-298 OK OK
20379 ACIS-23678 NONE VHSJ2141-4816 OK OK
20200 ACIS-012367 NONE IGR J18017-3542 OK OK
18303 HRC-I NONE Jupiter OK OK
20749 ACIS-0123 NONE Bania Clump 2 OK OK
20569 ACIS-012367 NONE SDSSJ1138+2754 OK OK
20557 ACIS-01236 NONE Abell 2146 OK OK
21064 ACIS-012367 NONE PSZ2 G218.59+71.31 OK OK
20330 ACIS-01237 NONE PSR J1809-1917 OK OK
21130 ACIS-01236 NONE Abell 2146 OK OK
21126 ACIS-0123 NONE PSR J1809-1917 OK OK

Trending

This week's focus is EPHIN

Last reported on Apr 26.

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