MTA Monitoring Report 06/03/11 - 06/09/11

Archive of all weekly reports
Archive of monthly reports


Radiation

High Radiation caused SCS-107 to run at 158/152310z.

06/07/2011 04:45 PM EDT
A Radiation violation of P3 (130keV) scaled from P6 (761keV) has been observed by ACE
Observed = 1.2368e+08
(limit = fluence of 1.2e8 particles/cm2-ster-MeV within 2 hours)

Lost science time: 75 Ks

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: 1.930e-9 CTI/day (1.274e-9 CTI/day)
Detrended slope: 7.230e-9 CTI/day (7.139e-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) (526,66) (334,88) (227,467) (247,364) (283,224) (233,321) (233,322) (233,323) (233,324) (233,325) (233,326) (233,327) (258,797) (263,317) (352,544) (367,511) (369,376) (641,669) (669,577) (843,420) (335,412) (139,109) (829,997) (881,53) (636,819)
Flickering Warm Pixels (692,141) (427,125) (910,239) (206,757) (811,637) (703,739)   (280,313) (745,313) (233,315) (1023,166) (233,328) (792,313) (884,31) (199,678) (662,995) (197,241) (666,165) (833,325) (587,544) (326,978) (356,902) (157,47) (182,474) (40,49)
Current Hot Pixels                    
Flickering Hot Pixels                    
Warm column candidates                    
Flickering Warm Column Candidates 518 509   509 514 1021     509 509   514 1021 509

ACIS Focal Plane Temperature

For this period, 5 peaks are observed.

Weekly focal plane temperature with sun angle and altitude overplotted. Sun angle is the solar array angle, that is the angle between the sun and the optical axis (+X axis). Altitude varies from 34 kkm to 128 kkm.



SIM Movements

11 TSC moves this period

Telemetry

New violations or new extrema are shown in blue cells.

MSID 06/03/11 06/04/11 06/05/11 06/06/11 06/07/11 06/08/11 06/09/11 yellow limits
(lower)
upper
red limits
(lower)
upper
Units Description
HKFBIASLEAKI           4.88 4.88 (-100.0)
4.88
(-200.0)
5.0
uA EPHIN HOUSEKEEPING F-BIAS: LEAKAGE CURRENT (5EHSE900)
LLDIALV 138.00 138.00 138.00 138.00 138.00 138.00   (130.0)
132.0
(129.0)
133.0
(2LLDIALV) Lower level disc setting
3TSMXSPT       295.74 295.74     (203.15)
294.15
(148.15)
354.15
K -X TURTLE SHELL NR ACIS SS
ESAMYI   42.74     42.74     (7.0)
27.0
(6.0)
33.0
AMP S/A -Y CURRENT
ESAPYI   43.30     43.30     (7.0)
27.0
(6.0)
33.0
AMP S/A +Y CURRENT
ELBI   85.74     87.12     (16.0)
62.0
(13.0)
66.0
AMP LOAD BUS CURRENT (ELBI_LOW)
OOBAPWR   758.30     788.40     (-1050)
370.0
(-1100)
400.0
W OBA COMPUTED TOTAL POWER
OOBTHR56 295.17 295.08 295.71     297.32 297.41 (281.04)
293.04
(249.37)
307.15
K RT 158: OBA CONE
OOBTHR60           290.62   (281.04)
290.48
(249.37)
307.15
K RT 153: OBA CONE


IRUs

Recent Observations

OBSID DETECTOR GRATING TARGET ANALYSIS ACA
12448 HRC-S NONE MAXI J1543-564 OK OK
12461 ACIS-67 NONE NGC 6652 OK OK
13258 ACIS-456789 HETG Mkn 841 OK OK
12699 ACIS-235678 NONE GRB 110422A OK OK
12897 ACIS-01236 NONE A2204_Field3 OK OK
11329 ACIS-456789 NONE SDSSJ150233.03+015608.3 OK OK
12507 ACIS-012367 NONE Norma Region OK OK
12508 ACIS-012367 NONE Norma Region OK OK
12509 ACIS-012367 NONE Norma Region OK OK
12333 HRC-I NONE Alpha Centauri OK OK
12510 ACIS-012367 NONE Norma Region OK OK

Trending

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

Last reported on Mar 17.

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