MTA Monitoring Report 04/09/10 - 04/15/10

Archive of all weekly reports
Archive of monthly reports


Radiation

Quiet.

Detrended CTI

Although we have quoted CTI values of the cleanest data (FT <= -119.7 C, int time > 7000sec), the data fills these conditions are getting rare. We quote CTI temperature factor corrected ones. The values in the parentheses are CTI based on the cleanest data.

Average of ACIS-I CCDs (MnKa) slope: 1.401e-9 CTI/day (1.290e-9 CTI/day)
Detrended slope: 7.544e-9 CTI/day (7.274e-9 CTI/day)

ACIS Warm Pixels

We display all bad pixels 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 a computational artificial effect due to boundaries.

 CCD0CCD1CCD2CCD3CCD4CCD5CCD6CCD7CCD8CCD9
Previously Unknown Bad Pixels                    
Current Warm Pixels (153,205) (802,665) (910,239) (526,66) (726,537)     (233,321) (233,322) (233,323) (233,324) (233,325) (233,326) (258,797) (263,317) (352,544) (367,511) (369,376) (669,577) (884,31) (199,678) (335,412) (662,995)    
Flickering Warm Pixels     (206,757) (931,553) (703,739) (247,364) (227,467) (283,224) (1023,166) (280,313) (109,1) (641,669) (792,313) (233,315) (233,327) (233,328) (745,313) (843,420) (662,995) (1024,455) (1024,456) (881,53) (913,165) (833,325) (1024,431) (1024,432) (1024,454) (1024,457) (197,241) (1024,453) (829,997) (356,902) (587,544) (1024,433) (562,499) (40,49) (636,819)
Current Hot Pixels                    
Flickering Hot Pixels                    
Warm column candidates                    
Flickering Warm Column Candidates 518 509 514 1021         509 509 509 509 514 1021 509

ACIS Focal Plane Temperature

For this period, 3 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

9 TSC moves this period

Telemetry

New violations or new extrema are shown in blue cells.

MSID 04/09/10 04/10/10 04/11/10 04/12/10 04/13/10 04/14/10 04/15/10 yellow limits
(lower)
upper
red limits
(lower)
upper
Units Description
1CBAT       (200.95)       (210.0)
301.0
(205.0)
306.06
K CAMERA BODY TEMP.
1DPPWRB (7.42)   (7.39)   (7.49)   (7.39) (9.0)
43.0
(8.0)
44.0
W DPA P WER B
5EPHINT 324.91 323.50 323.03 322.10 323.97 322.10 322.10 (261.0)
300.0
(258.0)
303.0
K EPHIN
HKEBOXTEMP 328.96 328.16 327.38 327.38 328.16 326.61 326.61 (268.0)
308.0
(253.0)
343.0
K EPHIN HOUSEKEEPING EBOX: TEMPERATURE (5EHSE300)
HKFBIASLEAKI 4.88 4.88 4.88 4.88 4.88 4.84 4.88 (-100.0)
2.0
(-200.0)
3.0
uA EPHIN HOUSEKEEPING F-BIAS: LEAKAGE CURRENT (5EHSE900)
TEIO 337.13 341.84 335.56 341.84 338.70 337.13 340.27 (253.0)
320.2
(250.2)
323.0
K EPHIN ELECTRONICS HOUSING TEMP
TEPHIN 324.48 324.48 322.36 323.42 324.48 322.36 323.42 (260.8)
300.2
(258.0)
303.0
K EPHIN SENSOR HOUSING
3RCTUBPT 301.77             (234.1)
276.3
(231.6)
278.8
K RCTU BASEPLATE
ESAMYI (7.74)             (8.5)
27
(6.5)
33.0
AMP S/A -Y CURRENT
TFSSBKT1 351.03 351.03 346.67 351.03 348.63 346.67 351.03 (233.0)
345.2
(223.0)
348.0
K FSS BRACKET-1 TEMP
TFSSBKT2 348.63 351.03 348.63 351.03 348.63 348.63 351.03 (233.0)
345.2
(223.0)
348.0
K FSS BRACKET-2 TEMP
TSCIUSF8 363.84             (230.2)
346.9
(227.4)
349.7
K SC-IUS FITTING-8
TSCTSF6 302.09 300.55           (255.8)
300.2
(253.0)
303.0
K SC-TS FITTING -6
4RT584T 290.77 290.77 290.52 290.27 290.27 290.27 290.27 (281.9)
290.0
(250.2)
308.0
K RT 584 - STRUT TEMP
4RT591T 293.60 293.60           (281.9)
292.0
(250.2)
308.0
K RT 591 - STRUT TEMP
OOBTHR04 290.59 290.68 290.38 290.20 290.16 290.07 290.03 (281.9)
290.0
(250.2)
308.0
K RT 27: HRMA STRUT
OOBTHR05 290.80 290.88 290.58 290.36 290.36 290.36 290.23 (281.9)
290.0
(250.2)
308.0
K RT 28: HRMA STRUT
OOBTHR45 292.38 292.46 292.29 292.33 292.55 292.29 292.24 (281.9)
292.0
(250.2)
308.0
K RT 67: TFTE COVER
OOBTHR52 292.93 292.88           (281.9)
292.0
(250.2)
308.0
K RT 78: S/C STRUT
OOBTHR56 295.35 295.98 295.08 295.98 296.33 296.07 295.80 (281.9)
295.0
(250.2)
308.0
K RT 158: OBA CONE


Pitch Angle and System Temperature

This is a test implementation, not all #'s have been verified.
On the weekly plots, long green ticks indicate obsid starts. The shorter orange ticks indicate rad zone events.

The following table shows the maximum temperature (in K) appeared during the observations. All data are taken between Oct 06 and Oct 12, 2009- DOY 279-285.

IRUs

Recent Observations

OBSID DETECTOR GRATING TARGET ANALYSIS ACA
12046 ACIS-01236 NONE Chandra Deep Field-South OK OK
11067 ACIS-012367 NONE GS0834-430 OK OK
11458 ACIS-7 NONE SDSS J113638.38+424552.9 OK OK
11845 ACIS-235678 NONE 3C 310 OK OK
11979 ACIS-012367 NONE NGC 602 OK OK
11390 ACIS-235678 NONE Cen A NML Filament OK OK
11512 ACIS-7 NONE M87 OK OK
11978 ACIS-012367 NONE NGC 602 OK OK
12047 ACIS-01236 NONE Chandra Deep Field-South OK OK
11720 ACIS-23567 NONE EN1-349 OK OK
12082 ACIS-23678 NONE Q0957+561 OK OK
11513 ACIS-7 NONE M87 OK OK
11783 ACIS-235678 NONE NGC4486A OK OK
12140 ACIS-23567 NONE EN1-349 OK OK
11324 ACIS-456789 NONE SDSSJ150033.02+021349.1 OK OK
11848 ACIS-456789 HETG ESO 323-G077 OK OK
11097 ACIS-2367 NONE SNR 0049-73.6 OK OK
11514 ACIS-7 NONE M87 OK OK

Trending

This week's focus is Spacecraft Bus and Subsystem Trends.

Last reported on Jan 21.

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