- M&TA MONTHLY REPORT -

October 2013

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OUTLINE

  1. Configuration
  2. ACIS
  3. HRC - Dose
  4. Gratings - Focus
  5. Resolving Power, E/dE
  6. SIM Twist
  1. PCAD
  2. Radiation History
  3. Quarterly Trending
  4. Trending
  5. Spacecraft Motions
  6. Past Monthly Report

Science Run Interruptions

Science observations were manually interrupted on Oct 1, 10:04PM EDT.
(see details: Radiation Count Rate Plots for Periods Which Interrupted Science Runs).


ACIS

ACIS DOSE Registered-Photon-Map

The steps we took to compute the dose map are;

Please check more detail plots at Telemetered Photon Dose Trend page.

  • Oct registered-photon-map in fits

  • Oct Dose Map


    TOTAL


    CCD I3


    CCD S3

    Statistics:
    # IMAGE     NPIX        MEAN           RMS              MIN     MAX
    ACIS_oct13 6004901      6.195         15.098            0.0     3019
    
    
    I2 node 0  262654   5.221161    2.779951    0.0  48.0
    I2 node 1  262654   5.440302    4.418455    0.0 756.0
    I2 node 2  262654   5.164371    3.080317    0.0 725.0
    I2 node 3  262654   5.316127    7.314813    0.0 761.0
    
    I3 node 0  262654   5.096943    2.669052    0.0  38.0
    I3 node 1  262654   5.369282    9.512252    0.0 2365.0
    I3 node 2  262654   4.830501    2.506447    0.0  51.0
    I3 node 3  262654   5.164726    8.584370    0.0 1816.0
    
    S2 node 0  262654   6.698790    4.572837    0.0 1694.0
    S2 node 1  262654   6.838838    3.438362    0.0  51.0
    S2 node 2  262654   7.083724    6.986952    0.0 3019.0
    S2 node 3  262654   6.778533    3.186007    0.0 396.0
    
    S3 node 0  262654   29.657564   56.451908   0.0 395.0
    S3 node 1  262654   11.802218   9.879224    0.0 168.0
    S3 node 2  262654   9.562167    4.561976    0.0 1497.0
    S3 node 3  262654   8.611543    3.291536    0.0  46.0
    
  • Jul 1999 - Oct 2013 registered-photon-map in fits
  • Cumulative Dose Map


    TOTAL


    CCD I3


    CCD S3
    
    Statistics:
     IMAGE        NPIX      MEAN             RMS            MIN    MAX
    ACIS_total   6004901    1745.581         2303.503       0.0   102455
    
    
    I2 node 0  262654   1469.951466 290.359582     0.0  8931.0
    I2 node 1  262654   1545.326311 390.514188     0.0 35140.0
    I2 node 2  262654   1573.733234 337.441686     0.0  6712.0
    I2 node 3  262654   1570.189345 398.377258     0.0  9376.0
    
    I3 node 0  262654   1646.728349 402.668202     0.0  6487.0
    I3 node 1  262654   1728.509697 1312.894756    0.0 33447.0
    I3 node 2  262654   1508.433466 279.157190     0.0  7508.0
    I3 node 3  262654   1494.619110 297.245978     0.0 25985.0
    
    S2 node 0  262654   2099.183563 321.151655  1096.0 28647.0
    S2 node 1  262654   2236.942246 492.136249  1149.0 12352.0
    S2 node 2  262654   2474.263120 483.330768  1482.0 42194.0
    S2 node 3  262654   2408.010062 365.221485  1425.0 40008.0
    
    S3 node 0  262654   3668.612565 1738.818884 1508.0 12805.0
    S3 node 1  262654   4755.187706 1925.603778    0.0 13080.0
    S3 node 2  262654   3671.477294 924.795254  1479.0  9207.0
    S3 node 3  262654   2874.365546 447.921744  1641.0  9374.0
    
    
  • Integrated Exposure Maps of Last 12 Months
  • Jul 2013 Apr 2013 Jan 2013 Oct 2012

    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 2013 Focal Temperature

    The Mean (max) FPT:
    -114.83 +/- 3.74 C
    Mean Width:
    0.58 +/- 0.60 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
    Hardest10.00   Beyond 10 keV
    This page shows scientific instrument background data based on Acis observations. A source region file is generated using get_srcregions and then the input event file is filtered using the regions in that file to remove the sources.


    TOP


    HRC

    DOSE of Central 4K Pore-Pairs

    Please refer to Maximum Dose Trends for more details.

  • Oct HRC-I Dose in fits
  •   
            IMAGE                NPIX      MEAN    STDDEV      MIN       MAX  
    HRCI_10_2013.fits          16777216   0.049    0.2226      0.0       4.0 
    
  • AUG 1999 - OCT 2013 HRC-I Dose in fits
  •         IMAGE                NPIX      MEAN    STDDEV      MIN       MAX
    HRCI_08_1999_10_2013.fits  16777216   4.076    4.808       0.0       292.0                                
    
  • Oct HRC-S Dose
  •   
             IMAGE                NPIX      MEAN    STDDEV      MIN       MAX    
    HRCS_10_2013.fits          16777216   0.231    0.8790      0.0        62.0                                 
    
  • AUG 1999 - OCT 2013 HRC-S Dose in fits
  •         IMAGE                NPIX     MEAN      STDDEV      MIN      MAX
    HRCS_08_1999_10_2013.fits  16777216  15.088      25.197      0.0      1655.0                                
    

    Max dose trend plots corrected for events that "pile-up" in the center of the taps due to bad position information.

  • HRC I: Integrated Exposure Maps of Last 12 Months
  • Jul 2013 Apr 2013 Jan 2013 Oct 2012
  • HRC S: Integrated Exposure Maps of Last 12 Months
  • Jul 2013 Apr 2013 Jan 2013 Oct 2012

    TOP


    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:
      Plus side = plus (+)
      Minus side = cross (x)
      1999-2001   green
      A002-2004   blue
      2005-2006   yellow
      2007-2009   orange

    TOP


    PCAD

    ACA Trending

    ACA Trending - Entire Period

    ACA Trending - OCT 2013

    Gyro Bias Drift


    TOP


    Radiation History

    Radiation Zone Timing

    Plotted below are radiation zone timing plots based on the following definitions of radiation zone:

    Sun Spot History


    TOP


    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


    TOP


    Trending

    Quarterly Trends




    Envelope Trending

    ACIS Electronics A



    ACIS Temperature





    EPS Battery





    TOP


    Spacecraft Motions

    Reaction Wheel Rotations

    Note: From Feb 2010, the computation of reaction wheel rotations are slightly modified.

    TOP


    Links to Past Monthly Reports


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    If you have any questions about this page, please contact swolk@head.cfa.harvard.edu.