Proton Calorimetry/Detector Analysis

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(Image Analysis)
(Photodiode Data Processing)
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=Photodiode Data Processing=
=Photodiode Data Processing=
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Details on how to process hexadecimal data from the [http://www.hep.ucl.ac.uk/pbt/wiki/Proton_Calorimetry/Equipment/ZyboZ7_DDC232, DDC232] to recover the charge in each photodiode.
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Details on how to process hexadecimal data from the [http://www.hep.ucl.ac.uk/pbt/wiki/Proton_Calorimetry/Equipment/ZyboZ7_DDC232 DDC232] to recover the charge in each photodiode.
=Bragg Fit=
=Bragg Fit=
Details on how to fit data with the quenched Bragg model to recover the range.
Details on how to fit data with the quenched Bragg model to recover the range.

Revision as of 15:11, 10 September 2020

This page contains information on the analysis code for the QuARC detector data.

Image Analysis

Details on how to process images taken by the ISDI CMOS Sensor to recover the average light output in each scintillator sheet.

  • First, the 21 images taken by the CMOS sensor must be corrected for non-linearity effects in the photon-electron conversion. The MATLAB script linear_corr_tiff.m does this.
    • The correct full-well mode must be selected in the script, typically high full-well is chosen for its superior linearity.
    • The script loops over each pixel in the 21 images and applies a correction using cubic interpolation of the linearity data (linearity_high.txt). A corrected version of each image is saved.
  • The 21 corrected images are then averaged using averageTiffs.sh, which outputs a single image.
    • On MacOS, this may require ImageMagick, which can be installed with MacPorts: sudo port install ImageMagick
  • To apply background subtraction and corrections for non-linearity in scintillator light output, the MATLAB script edit_runs.m is run.
    • This requires a corrected/averaged background and shoot-through measurements (front and/or back).
    • Important for background and shoot-through to have the same full-well mode as the measurement. Similar spot size for the shoot-through and measurement is also desirable.
    • The script outputs a .txt file containing a column of data, representing the light output in each sheet in arbitrary units. This can be used in the fitting procedure.

Photodiode Data Processing

Details on how to process hexadecimal data from the DDC232 to recover the charge in each photodiode.

Bragg Fit

Details on how to fit data with the quenched Bragg model to recover the range.

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