MTA Monitoring Report 08/31/18 - 09/06/18

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: 1.370e-02 CTI/year (3.753e-05 CTI/day)
Detrended slope: 1.774e-02 CTI/year (4.861e-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) (143,700) (910,239) (802,665) (726,537) (178,149) (811,637) (680,391) (21,95)       (335,412) (197,241) (881,53)  
Flickering Warm Pixels   (427,125) (643,351) (526,66) (318,53)   (607,281) (357,303) (282,385) (369,376) (669,577) (263,317) (367,511) (161,206) (258,797) (341,427) (884,31) (1000,214)   (182,474) (597,187) (139,109) (150,374) (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, 8 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 08/31/18 09/01/18 09/02/18 09/03/18 09/04/18 09/05/18 09/06/18 yellow limits
(lower)
upper
red limits
(lower)
upper
Units Description
HRMACAV   (284.85) (284.85) (286.82) (284.85)     (293.4)
294.8
(292.8)
295.5
TEMP # HRMA CAVITY AVG
HRMACAV     294.82 294.81       (293.4)
294.8
(292.8)
295.5
TEMP # HRMA CAVITY AVG
MZOBACONE   (221.33) (221.33)       (221.33) (260.2)
303.0
(250.2)
308.0
CONE # -Z SIDE OBA
MZOBACONE   303.82 303.13       303.27 (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)
37.5
(11.1)
45.0
K # TFTE VENT/RAD TEMP
TFTERANGE   37.64           (16.7)
37.5
(11.1)
45.0
K # TFTE VENT/RAD TEMP
IMHVLV   (80.00) (80.00) (99.00) (99.00)   (80.00) (126.0)
128.0
(125.0)
129.0
(2IMHVLV) #Imaging bot MCP HV monitor
IMHBLV   (87.00) (87.00) (105.00) (105.00)   (87.00) (126.0)
128.0
(125.0)
129.0
(2IMHBLV) #Imaging bot and top MCP HV monitor
SPHBLV         (78.00) (78.00)   (79.0)
128.0
(78.0)
129.0
(2SPHBLV) #Spect bot and top MCP HV monitor
S2HVLV (83.00) (82.00) (83.00) (83.00) (82.00) (83.00) (82.00) (126.0)
128.0
(125.0)
129.0
(2S2HVLV) #Shield PMT 2 HV monitor
LLDIALV 138.00 138.00           (130.0)
132.0
(129.0)
133.0
(2LLDIALV) #Lower level disc setting
RSRFALV     (20.00)     (24.00)   (172.0)
174.0
(171.0)
175.0
V #Range switch setting (2RSRFALV)
RSRFALV 190.00 190.00 185.00 185.00 191.00 190.00 190.00 (172.0)
174.0
(171.0)
175.0
V #Range switch setting (2RSRFALV)
3FLCABPT       294.96 293.95     (253.15)
293.15
(235.65)
310.65
K #FLCA BASEPLATE (+X)
3TSMXCET 283.26 280.77 283.26 280.77 280.77 288.25 285.76 (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 66.89 65.56 63.20 63.73 62.68 65.56 66.89 (16.0)
50.0
(13.0)
66.0
AMP #LOAD BUS CURRENT (ELBI_LOW)
TAPE2PST (291.85) (291.85) (293.14) (292.71) (292.71) (292.28) (291.85) (323.15)
330.15
(318.15)
335.15
K #PEA-2 POWER SUPPLY TEMP
4PRT3AT (258.46) (258.46) (258.46) (258.46) (257.79) (258.46) (258.46) (273.15)
283.15
(53.15)
368.15
K #IP A: PRE-COLLIMATOR PRT 3 TEMPERATURE


IRUs

Gyro Bias Drift Gyro Bias Drift Histogram

Recent Observations

OBSID DETECTOR GRATING TARGET ANALYSIS ACA
20331 ACIS-01237 NONE PSR J1809-1917 OK OK
21726 ACIS-3678 NONE P308-21 OK OK
20998 ACIS-7 NONE SN2011dh OK OK
20753 ACIS-01236 NONE Centaurus A OK OK
21724 ACIS-01237 NONE PSR J1809-1917 OK OK
20550 ACIS-0123 NONE 1RXSJ174537.3+395128 OK OK
20501 ACIS-01236 NONE ClG J223533+183352 OK OK
20606 ACIS-235678 NONE Q 0000-263 OK OK
20459 ACIS-23678 NONE SDSS J000904.54-103428.6 OK OK
21021 ACIS-56789 NONE LSBC F743-01 OK OK
20578 ACIS-012367 NONE SDSSJ1522+2535 OK OK
20504 ACIS-0123 NONE ClG J002855+174412 OK OK
21401 ACIS-2367 NONE 3CR 418.0 OK OK
20377 ACIS-23678 NONE VHSJ2115-5913 OK OK
20384 ACIS-23678 NONE VHSJ2332-5240 OK OK
20414 ACIS-3678 NONE J2348-3054 OK OK
20686 HRC-S NONE ArLac CAL OK
20687 HRC-S NONE ArLac CAL OK
20688 HRC-S NONE ArLac CAL OK
20689 HRC-S NONE ArLac CAL OK
20690 HRC-S NONE ArLac CAL OK
20691 HRC-S NONE ArLac CAL OK
20692 HRC-S NONE ArLac CAL OK
20693 HRC-S NONE ArLac CAL OK
20694 HRC-S NONE ArLac CAL OK
20695 HRC-S NONE ArLac CAL OK
20696 HRC-S NONE ArLac CAL OK
20697 HRC-S NONE ArLac CAL OK
20698 HRC-S NONE ArLac CAL OK
20699 HRC-S NONE ArLac CAL OK
20700 HRC-S NONE ArLac CAL OK
20701 HRC-S NONE ArLac CAL OK
20702 HRC-S NONE ArLac CAL OK
20703 HRC-S NONE ArLac CAL OK
20704 HRC-S NONE ArLac CAL OK
20779 ACIS-012367 NONE Abell 1925 OK OK
20151 ACIS-0123 NONE beta Dor OK OK
21368 ACIS-23678 NONE GRB 180720B OK OK

Trending

This week's focus is Sun Angle Correlations

Last reported on Jun 14.

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