MTA Monitoring Report 02/18/11 - 02/24/11

Archive of all weekly reports
Archive of monthly reports


Radiation

New sunspot 1163 produced an M3-class flare on Feb 24 from just behind the sun's eastern limb. This active sunspot will be rotating into Earth's view in coming days.

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: 1.838e-9 CTI/day (1.259e-9 CTI/day)
Detrended slope: 7.352e-9 CTI/day (7.211e-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) (206,757) (526,66) (334,88) (703,739)   (233,321) (233,322) (233,323) (233,324) (233,325) (233,326) (258,797) (263,317) (280,313) (352,544) (367,511) (369,376) (641,669) (669,577) (792,313) (843,420) (884,31) (335,412) (139,109) (829,997) (881,53)  
Flickering Warm Pixels (153,205) (802,665) (910,239) (206,757) (526,66) (703,739) (811,637) (247,364) (227,467) (331,244) (233,321) (233,322) (233,323) (233,324) (233,325) (233,326) (233,327) (263,317) (280,313) (369,376) (367,511) (352,544) (258,797) (669,577) (641,669) (745,313) (233,328) (233,315) (282,385) (1023,166) (843,420) (335,412) (662,995) (199,678) (139,109) (881,53) (829,997) (197,241) (356,902) (587,544) (1024,454) (1024,455) (1024,456) (1024,453) (1024,457) (1024,458) (1024,432) (326,978) (833,325) (636,819) (569,1016) (40,49) (991,128)
Current Hot Pixels                    
Flickering Hot Pixels                    
Warm column candidates                    
Flickering Warm Column Candidates 518 509   509 514 1021     1021 509 514 518 1021   509 514 1021 509 514 515 1021

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

7 TSC moves this period

Telemetry

New violations or new extrema are shown in blue cells.

MSID 02/18/11 02/19/11 02/20/11 02/21/11 02/22/11 02/23/11 02/24/11 yellow limits
(lower)
upper
red limits
(lower)
upper
Units Description
1CRAT 150.00 150.00     150.00 150.00   (-137.0)
-100.0
(-142.0)
-90.0
C COLD RADIATOR TEMP. A
TB1T1 (270.09) (270.09) (270.09)     (270.09) (270.09) (270.37)
303.15
(268.15)
314.26
K BATT 1 TEMP 1
OOBTHR56 295.53 296.96 295.35 296.15   295.98   (281.04)
293.04
(249.37)
307.15
K RT 158: OBA CONE


IRUs

Recent Observations

OBSID DETECTOR GRATING TARGET ANALYSIS ACA
13225 ACIS-7 NONE CXOGClb J174804.8-244648 OK OK
13197 ACIS-5678 HETG GX 13+1 CAL OK
12955 ACIS-235678 NONE NGC4342 OK OK
12259 ACIS-01236 NONE ACT J0438-5419 OK OK
12375 ACIS-235678 NONE NGC 6445 OK OK
12159 ACIS-235678 NONE Protocluster at z=1.30 OK OK
12748 ACIS-7 NONE NGC 4178 OK OK
12506 HRC-I NONE IGR J17597-2201 OK OK
12499 HRC-I NONE IGR J18219-1347 OK OK
12498 HRC-I NONE IGR J18293-1213 OK OK
12463 ACIS-456789 NONE J1840-14 OK OK
12266 ACIS-01236 NONE ACT J0237-4939 OK OK
12888 ACIS-345678 NONE NGC 4472 OK OK
12490 ACIS-35678 NONE 1RXS J143157.4+370635 OK OK
12398 ACIS-235678 NONE HD 179958 OK OK
12696 ACIS-2367 NONE SN 1979C OK OK

Trending

This week's focus is SIM.

Last reported on Dec 02.

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