ACIS
ACIS DOSE Registered-Photon-Map
The steps we took to compute the dose map are;
- Level 1 Event files for a specified month are obtained from archive.
- Image data including I2, I3, S2, S3 CCDs are extracted from all event files.
- All the extracted image data were merged to create a month long exposure map for the month.
- The exposure map is opened with ds9, and check a distribution of count rates against energy. From this, estimate the upper threshold value. Any events beyond this upper threshold are assumed erroneous events such as bad pixels.
- Using this upper threshold, the data is filtered, and create a cleaned exposure map for the month.
- The exposure map from each month from the Sep 1999 is added up to create a cumulative exposure map for each month.
- Using fimgstatistic, we compute count rate statistics for each CCDs.
- For observations with high data drop rates (e.g., Crab nebula, Cas A), we corrected the observations by adding events.
-
Note: Counts and RMS's of Cumulative maps are lower than the previous months.
This is because we excluded extreme outliers.
Please check more detail plots at Telemetered Photon Dose Trend page.
Statistics: # IMAGE NPIX MEAN RMS MIN MAX ACIS_nov12 6004901 7.366 13.647 0.0 5624 I2 node 0 262654 8.429432 3.565557 0.0 61.0 I2 node 1 262654 8.822211 4.049972 0.0 356.0 I2 node 2 262654 8.795792 3.662067 0.0 79.0 I2 node 3 262654 8.903181 11.899718 0.0 5624.0 I3 node 0 262654 9.479678 3.931085 0.0 44.0 I3 node 1 262654 9.950787 9.227771 0.0 218.0 I3 node 2 262654 9.045767 3.640041 0.0 60.0 I3 node 3 262654 9.073116 4.806550 0.0 1558.0 S2 node 0 262654 7.476061 3.826626 0.0 998.0 S2 node 1 262654 7.741161 3.762395 0.0 54.0 S2 node 2 262654 7.911497 8.251334 0.0 3805.0 S2 node 3 262654 7.693192 3.445467 0.0 430.0 S3 node 0 262654 22.370152 37.411901 0.0 279.0 S3 node 1 262654 11.308193 8.300791 0.0 160.0 S3 node 2 262654 9.738109 3.479716 0.0 41.0 S3 node 3 262654 8.881120 3.279498 0.0 28.0
Statistics: IMAGE NPIX MEAN RMS MIN MAX ACIS_total 6004901 1670.140 2208.091 0.0 98584 I2 node 0 262654 1389.279285 272.859678 0.0 7182.0 I2 node 1 262654 1461.226291 364.858053 0.0 31938.0 I2 node 2 262654 1491.625889 321.465010 0.0 6464.0 I2 node 3 262654 1487.002465 376.912236 0.0 6949.0 I3 node 0 262654 1562.571146 383.647397 0.0 6170.0 I3 node 1 262654 1640.783585 1242.389288 0.0 31787.0 I3 node 2 262654 1428.876225 263.904143 0.0 6924.0 I3 node 3 262654 1413.930523 280.648254 0.0 24903.0 S2 node 0 262654 2018.390786 307.238052 1053.0 28549.0 S2 node 1 262654 2154.946845 472.952135 1094.0 11868.0 S2 node 2 262654 2388.481824 470.893792 1433.0 41942.0 S2 node 3 262654 2321.918702 360.538495 1374.0 37803.0 S3 node 0 262654 3490.643176 1674.126820 1450.0 12650.0 S3 node 1 262654 4585.818238 1886.028045 0.0 12929.0 S3 node 2 262654 3537.687109 903.540480 1390.0 8903.0 S3 node 3 262654 2767.198347 445.125914 1573.0 9085.0
Aug 2012 | May 2012 | Feb 2012 | Nov 2011 |
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The Mean Detrended CTI
We report CTIs with a refined data definition. CTIs were computed for the temperature dependency corrected data. Please see CTI page for detailed explanation. CTI's are computed for Mn K alpha, and defined as slope/intercept x10^4 of row # vs ADU. Data file: here
Focal Plane Temperature
Nov 2012 Focal Temperature
The Mean (max) FPT: | |
---|---|
-112.64 | +/- 5.97 C |
Mean Width: | |
0.59 | +/- 0.51 days |
Averaged Focal Plane Temperature
We are using 10 period moving averages to show trends of peak temperatures and peak widths. Note, the gaps in the width plot are due to missing/corrupted data.
Focal Plane Temperature, Sun Angle and Altitude
Bad Pixels
The plots below were generated with a new warm pixel finding script. Please see Acis Bad Pixel Page for details.
Front Side CCDs
Back Side CCD (CCD5)
Science Instrument Background Rates
Name | Low (keV) | High(KeV) | Description |
---|---|---|---|
SSoft | 0.00 | 0.50 | Super soft photons |
Soft | 0.50 | 1.00 | Soft photons |
Med | 1.00 | 3.00 | Moderate energy photons |
Hard | 3.00 | 5.00 | Hard Photons |
Harder | 5.00 | 10.00 | Very Hard photons |
Hardest | 10.00 | Beyond 10 keV |
The following three plots show trends of SIB from year 2000. CCDs shown here are CCD3, CCD5, and CCD7. Fitted lines are linear fit after eliminating extreme outliers. For >10 keV plots, 2 lines are fit. One is with a 13 keV filter, and another without.
CCD 3
CCD 5
CCD 7
ACIS Histogram Mode Trends
We collected data from acis histogram mode data, and created trend plots of peak portions and peak widths against time (DOM). The peaks were estimated by fitting a simple Gaussian on three peaks (Al, Ti, and Mn), and the widths were estimated by a width at the half max from the peak.
All histogram data are taken under TIMED and GRADED_HIST mode, SIM position is at an external calibration source position, the focal temperature is around -119.7 C, and parameter settings in aciselec, acistemp are set to about same for all.
CCD 3, Peak Position
CCD 3, Peak Widths
CCD 3, Count Rates
HRC
DOSE of Central 4K Pore-Pairs
Please refer to Maximum Dose Trends for more details.
No Data
IMAGE NPIX MEAN STDDEV MIN MAX HRCI_08_1999_11_2012.fits 16777216 3.904 4.745 0.0 292.0
IMAGE NPIX MEAN STDDEV MIN MAX HRCS_11_2012.fits 16777216 0.011 0.104 0.0 3.0
IMAGE NPIX MEAN STDDEV MIN MAX HRCS_08_1999_11_2012.fits 16777216 14.219 23.912 0.0 1634.0
Max dose trend plots corrected for events that "pile-up"
in the center of the taps due to bad position information.
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Aug 2012 | May 2012 | Feb 2012 | Nov 2011 |
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Aug 2012 | May 2012 | Feb 2012 | Nov 2011 |
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Gratings
Focus
We plot the width of the zero order streak of ACIS/HETG observations and the width of the zero order image for HRC/LETG observations of point sources. No significant defocusing trend is seen at this time. See Gratings Focus pages.
PCAD
ACA Trending
Gyro Bias Drift
Radiation History
Radiation Zone Timing
Plotted below are radiation zone timing plots based on the following definitions of radiation zone:
- RADZONE - Ephin levels (in any of the E1300,P4GM,P41GM channels) are more than 1/3 of RADMON safing thresholds.
- RADMON - Radmon is disabled for radiation zone (as commanded based on OFLS model, for comparison with actual radiation levels).
- PERIGEE - Time of closest earth approach (for comparison)
Radiation Count Rates of Nov 2012
Sun Spot History
Trending
Quarterly Trends
- HRMA Thermal
Previous Quarter | ||||||
MSID | MEAN | RMS | DELTA/YR | DELTA/YR/YR | UNITS | DESCRIPTION |
4RT575T | 292.06 | 1.11 | 8.533e-01 | -6.422e+01 | K | RT 575 - OB CONE TEMP |
4RT577T | 292.91 | 2.09 | -2.804e+00 | -1.511e+02 | K | RT 577 - OB CONE TEMP |
4RT578T | 290.67 | 1.83 | -2.711e+00 | -1.437e+02 | K | RT 578 - OB CONE TEMP |
- HRMA Struts
Previous Quarter | ||||||
MSID | MEAN | RMS | DELTA/YR | DELTA/YR/YR | UNITS | DESCRIPTION |
4RT590T | 294.77 | 1.61 | 4.876e-01 | -1.733e+02 | K | RT 590 - STRUT TEMP |
4RT591T | 294.44 | 1.51 | 4.037e-01 | -1.541e+02 | K | RT 591 - STRUT TEMP |
4RT597T | 293.15 | 1.51 | 2.209e+00 | -4.449e+01 | K | RT 597 - TFTE TEMP |
4RT598T | 292.79 | 1.53 | 2.048e+00 | -4.818e+01 | K | RT 598 - TFTE TEMP |
- OB Forwared Bulk Head
Previous Quarter | ||||||
MSID | MEAN | RMS | DELTA/YR | DELTA/YR/YR | UNITS | DESCRIPTION |
4RT704T | 288.81 | 0.88 | 2.313e-01 | -6.543e+01 | K | RT 704 - OB BULKHEAD TEMP |
4RT705T | 283.81 | 0.78 | 7.174e-02 | -6.156e+01 | K | RT 705 - OB BULKHEAD TEMP |
4RT706T | 282.32 | 0.81 | -4.068e-02 | -6.360e+01 | K | RT 706 - OB BULKHEAD TEMP |
4RT707T | 284.89 | 0.79 | 1.106e-01 | -6.035e+01 | K | RT 707 - OB BULKHEAD TEMP |
Envelope Trending
EPS Battery
HRMA Heater
Spacecraft Motions
Reaction Wheel Rotations
Note: From Feb 2010, the computation of reaction wheel rotations are slightly modified.
Links to Past Monthly Reports
Year | Month | |||||||||||
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1999 | Jul | Aug | Sep | Oct | Nov | Dec | ||||||
2000 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2001 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2002 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2003 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2004 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2005 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2006 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2007 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2008 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2009 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2010 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2011 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2012 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct |