MTA Monitoring Report 06/20/14 - 06/26/14

Archive of all weekly reports
Archive of monthly reports


Radiation

High proton level was observed during the weekend of Jun 6-8. Fluence is around 1.4e9 and ACE P3 rate was 18k as ob Sat night. However, there was no science run interruption.

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: 1.634e-6 CTI/year (4.448e-9 CTI/day)
Detrended slope: 1.587e-6 CTI/year (4.348e-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     (726,537) (21,95)         (881,53)  
Flickering Warm Pixels (153,205) (910,239) (802,665)     (885,460) (607,281) (357,303) (369,376) (669,577) (280,313) (233,314) (161,206) (341,427)   (335,412) (833,325) (182,474) (197,241) (356,902) (139,109) (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, 1 peak is 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

10 TSC moves this period

Telemetry

New violations or new extrema are shown in blue cells.

MSID 06/20/14 06/21/14 06/22/14 06/23/14 06/24/14 06/25/14 06/26/14 yellow limits
(lower)
upper
red limits
(lower)
upper
Units Description
5EPHINT 338.49 339.58 332.48 340.67 340.67 340.67 331.46 (261.15)
331.15
(258.15)
341.15
K #EPHIN TEMP
HKP5V (5.06)     (5.06) (5.06) (5.06) (5.06) (5.08)
5.15
(5.06)
5.17
V #HK 5 Volts Rail - Voltage
HKP5I       53.67   54.06   (35.78)
52.97
(32.78)
55.97
AMP #HK 5 Volts Rail - Current
HKEBOXTEMP 343.76 345.00 338.12 346.29 346.29 346.29 337.10 (268.15)
336.15
(253.15)
346.15
K #EPHIN HOUSEKEEPING EBOX: TEMPERATURE (5EHSE300)
TEIO 349.70 351.27 351.27 351.27 352.84 351.27 351.27 (252.15)
347.26
(249.37)
361.15
K #EPHIN ELECTRONICS HOUSING TEMP
OHRTHR27 297.35 297.35 297.35 297.35 297.34 297.34 297.33 (295.48)
297.15
(279.37)
307.15
K #RT 20 : PERISCOPE
OHRTHR42 294.61 294.65 294.65 294.65 294.69 294.66 294.66 (292.15)
294.37
(279.37)
307.15
K #RT 133: PERISCOPE
OHRTHR43 294.56 294.64 294.64 294.64 294.78 294.67 294.66 (291.59)
293.26
(279.37)
307.15
K #RT 134: PERISCOPE


IRUs

Recent Observations

OBSID DETECTOR GRATING TARGET ANALYSIS ACA
16532 ACIS-456789 HETG HD 206267 OK OK
16220 ACIS-456789 HETG 3C 390.3 OK OK
16521 ACIS-3678 NONE 3C 220.3 OK OK
15784 ACIS-7 NONE SXP 1062 CC OK
16070 ACIS-23678 NONE PKS 1718-649 OK OK
16078 ACIS-7 NONE ESO138-G1 OK OK
14204 ACIS-7 NONE 1E1207.4-5209 CC OK
14886 ACIS-23678 NONE GRB 130427A OK OK
16479 HRC-I NONE Vega CAL OK
16480 HRC-S NONE Vega CAL OK
16481 HRC-S NONE Vega CAL OK
16482 HRC-S NONE Vega CAL OK
16180 ACIS-0123 NONE Chandra Deep Field-South OK OK
16623 ACIS-23678 NONE PKS 1718-649 OK OK
15642 ACIS-7 NONE GJ 436 OK OK
15662 ACIS-5678 LETG NGC 5548 OK OK
16624 ACIS-7 NONE PSR B1259-63 CC OK
14233 HRC-I NONE ALPHA CEN OK OK
15122 ACIS-01236 NONE G253.47-33.72 OK OK
16295 ACIS-012367 NONE M31 BHXNe OK OK
16033 ACIS-23678 NONE NGC 4551 OK OK
16115 ACIS-23678 NONE SDSS J135429.05+132757.2 OK OK
16622 ACIS-5678 HETG Cyg X-3 CAL OK
16424 ACIS-56789 HETG MKN421 CAL OK
16625 ACIS-7 NONE PSR B1259-63 CC OK
16425 ACIS-56789 LETG MKN421 CAL OK
16426 HRC-S LETG MKN421 CAL OK
16427 ACIS-56789 LETG MKN421 CAL OK
16428 HRC-S LETG MKN421 CAL OK
16429 ACIS-56789 LETG MKN421 CAL OK

Trending

This week's focus is Ground Computations..

Last reported on Apr 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