MTA Monitoring Report 03/13/15 - 03/19/15

Archive of all weekly reports
Archive of monthly reports

Radiation

Observing stopped by ground activation of SCS-107 at 2015:076:04:34z ACE P3 rates are dropping and are expected to be well down by the time of the next rad-zone exit (2015:078:04:42:46z).

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: 1.552e-6 CTI/year (4.170e-9 CTI/day)
Detrended slope: 1.537e-6 CTI/year (4.211e-9 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 (153,205) (143,700) (910,239) (802,665) (726,537) (21,95)       (335,412)    
Flickering Warm Pixels (692,141) (427,125)   (703,739) (247,364) (607,281) (357,303) (369,376) (669,577) (263,317) (367,511) (161,206)     (182,474) (197,241) (881,53) (150,374)
Current Hot Pixels                    
Flickering Hot Pixels                    
Warm column candidates         884 510 512 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

6 TSC moves this period

Telemetry

New violations or new extrema are shown in blue cells.

MSID 03/13/15 03/14/15 03/15/15 03/16/15 03/17/15 03/18/15 03/19/15 yellow limits
(lower)
upper 		red limits
(lower)
upper 		Units Description
1DAHBCU 0.40             (-998)
0.20		(-999)
999		 AMP #DA HEATER CURRENT B
1DAHBVO 4.31             (-998)
1.0		(-999)
999		 V #DA HEATER VOLTAGE B
1DAHHBVO 28.08             (-998)
1.0		(-999)
999		 V #DA HOUSING HEATER INPUT VOLTAGE B
LLDIALV             (94.00) (130.0)
132.0		(129.0)
133.0		 (2LLDIALV) #Lower level disc setting
RSRFALV   (74.00)         (94.00) (172.0)
174.0		(171.0)
175.0		 V #Range switch setting (2RSRFALV)
RSRFALV 185.00 192.00 190.00 190.00 190.00 190.00 190.00 (172.0)
174.0		(171.0)
175.0		 V #Range switch setting (2RSRFALV)
OHRTHR27 297.29 297.33 297.34 297.33 297.34 297.32 297.31 (295.48)
297.15		(279.37)
307.15		 K #RT 20 : PERISCOPE
OHRTHR42 294.44 294.63 294.64 294.59 294.69 294.69 294.69 (292.15)
294.37		(279.37)
307.15		 K #RT 133: PERISCOPE
OHRTHR43 294.13 294.61 294.67 294.56 294.78 294.82 294.74 (291.59)
293.26		(279.37)
307.15		 K #RT 134: PERISCOPE


IRUs

Recent Observations

OBSID DETECTOR GRATING TARGET ANALYSIS ACA
17174 ACIS-5678 NONE ZwCl 1234.0+02916 OK OK
17062 ACIS-5678 NONE NGC 5133 OK OK
17471 ACIS-01236 NONE Centaurus A OK OK
17173 ACIS-23567 NONE Abell 1664 OK OK
17149 ACIS-0123 NONE Abell1882 - Filament #1 OK OK
17022 ACIS-678 NONE SDSS J0936+0046 OK OK
17633 ACIS-0123 NONE Chandra Deep Field-South OK OK
17205 ACIS-012367 NONE ZwCl 0008.8+5215 EAST OK OK
16344 ACIS-0123 NONE BRC2 OK OK
17634 ACIS-0123 NONE Chandra Deep Field-South OK OK
16710 ACIS-456789 HETG GRS 1915+105 CC OK

Trending

This week's focus is HRMA Thermal.

Last reported on Dec 25.

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