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_oct12 6004901 7.087 10.614 0.0 3172 I2 node 0 262654 5.503841 2.745299 0.0 26.0 I2 node 1 262654 5.764513 3.069267 0.0 177.0 I2 node 2 262654 5.781319 2.817320 0.0 39.0 I2 node 3 262654 6.082613 3.332630 0.0 220.0 I3 node 0 262654 6.667004 4.772508 0.0 101.0 I3 node 1 262654 6.646149 6.011661 0.0 331.0 I3 node 2 262654 6.012385 2.984891 0.0 54.0 I3 node 3 262654 5.847321 2.845884 0.0 130.0 S2 node 0 262654 8.880308 3.630683 0.0 482.0 S2 node 1 262654 9.181182 4.156384 0.0 70.0 S2 node 2 262654 9.444550 4.930201 0.0 1547.0 S2 node 3 262654 9.315085 3.657688 0.0 478.0 S3 node 0 262654 18.012852 19.499236 0.0 156.0 S3 node 1 262654 13.130805 6.030065 0.0 90.0 S3 node 2 262654 11.967004 3.691615 0.0 57.0 S3 node 3 262654 10.762586 3.449656 0.0 35.0
Statistics: IMAGE NPIX MEAN RMS MIN MAX ACIS_total 6004901 1662.774 2198.599 0.0 98151 I2 node 0 262654 1380.849854 271.020140 0.0 7121.0 I2 node 1 262654 1452.404080 362.293096 0.0 31582.0 I2 node 2 262654 1482.830097 319.556162 0.0 6438.0 I2 node 3 262654 1478.099284 374.376424 0.0 6912.0 I3 node 0 262654 1553.091467 381.481025 0.0 6134.0 I3 node 1 262654 1630.832798 1233.807075 0.0 31569.0 I3 node 2 262654 1419.830458 262.066943 0.0 6864.0 I3 node 3 262654 1404.857407 278.685699 0.0 24773.0 S2 node 0 262654 2010.138342 305.783797 1048.0 28542.0 S2 node 1 262654 2146.425552 470.903524 1089.0 11802.0 S2 node 2 262654 2379.755821 470.072341 1429.0 41917.0 S2 node 3 262654 2313.416257 360.588601 1369.0 37593.0 S3 node 0 262654 3467.166854 1664.987452 1446.0 12640.0 S3 node 1 262654 4573.280952 1884.954516 0.0 12923.0 S3 node 2 262654 3526.794317 903.681669 1375.0 8880.0 S3 node 3 262654 2757.279455 445.604713 1565.0 9062.0
Jul 2012 | Apr 2012 | Jan 2012 | Oct 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
Oct 2012 Focal Temperature
The Mean (max) FPT: | |
---|---|
-109.35 | +/- 4.24 C |
Mean Width: | |
0.27 | +/- 0.08 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 |
HRC
DOSE of Central 4K Pore-Pairs
Please refer to Maximum Dose Trends for more details.
IMAGE NPIX MEAN STDDEV MIN MAX HRCI_10_2012.fits 16777216 0.001 0.0351 0.0 2.0
IMAGE NPIX MEAN STDDEV MIN MAX HRCI_08_1999_10_2012.fits 16777216 3.905 4.745 0.0 292.0
IMAGE NPIX MEAN STDDEV MIN MAX HRCS_10_2012.fits 16777216 0.003 0.054 0.0 2.0
IMAGE NPIX MEAN STDDEV MIN MAX HRCS_08_1999_10_2012.fits 16777216 14.207 23.898 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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Jul 2012 | Apr 2012 | Jan 2012 | Oct 2011 |
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Jul 2012 | Apr 2012 | Jan 2012 | Oct 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.
Gratings Resolving Power
We plot E/dE vs. E for fits to detected lines with fwhm_error/fwhm less than 0.15 for the plus and minus arms of HEG, MEG, and LEG. Also shown are conservative (dotted line) and optimistic (dashed line) pre-launch resolving power expectations.
We have selected only calibration observations of Capella, HR1099, and Sigma Gem. See MIT technotes for a parallel analysis.
Plot symbol indicates dispersion arm: | Color indicates observation date: |
Minus side = cross (x) |
A002-2004   blue 2005-2006   yellow 2007-2009   orange |
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 Oct 2012
Sun Spot History
SIM
SIM Shift and Twist
SIM Shift and Twist Trend The following plots show trends of SIM shifts (dy and dz) and twist (dtheta). All quantities are directly taken from pcaf*_asol1.fits files. The units are mm for dy and dz, and degree for dtheta. We fit three lines separated before and after (Days of Mission)= 1400 (May 21, 2003), and 2700 (Dec 11, 2006). The unit of slopes are mm per day or degree per day.
The sudden shift around DOM = 1400 and 2700 are due to fid light drift (see a memo by Aldcroft fiducial light drift). On the dtheta plot, two tracks are clearly observed. The track around 0.01 is due to HRC-I, and all others are clustered around -0.002. For more detail, please see SIM Shift and Twist Trend page
Trending
Quarterly Trends
- OBA Heaterse
Previous Quarter | ||||||
MSID | MEAN | RMS | DELTA/YR | DELTA/YR/YR | UNITS | DESCRIPTION |
OOBTHR08 | 291.40 | 1.19 | 1.793e-01 | -8.136e+01 | K | RT 31: OBA CONE |
OOBTHR09 | 290.70 | 1.14 | 4.079e-02 | -8.366e+01 | K | RT 32: OBA CONE |
OOBTHR18 | 290.57 | 1.14 | 4.853e-03 | -8.023e+01 | K | RT 40: OBA CONE |
OOBTHR19 | 292.16 | 1.89 | -2.037e+00 | -1.446e+02 | K | RT 41: OBA CONE |
- HRMA Heaterse
Previous Quarter | ||||||
MSID | MEAN | RMS | DELTA/YR | DELTA/YR/YR | UNITS | DESCRIPTION |
OHRTHR22 | 295.26 | 1.225e-03 | 6.761e-03 | 3.761e-02 | K | RT 6: HRMA FOWARD APERTURE PLATE |
OHRTHR45 | 295.25 | 8.762e-04 | -4.249e-03 | 2.404e-02 | K | RT 4: HRMA FORWARD APERTURE PLATE |
OHRTHR46 | 295.27 | 1.399e-03 | 9.958e-03 | 5.530e-02 | K | RT 7: HRMA FORWARD APERTURE PLATE |
OHRTHR47 | 295.29 | 4.826e-03 | -3.831e-02 | -1.068e-01 | K | RT 10: HRMA PRECOLLIMATOR PLATE 10 |
Envelope Trending
HRMA Struts
MUPS
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 |