About
This page provides examples for selected modules from Psana Module Catalog.
Auxiliary scripts
A few python scripts in ImgPixSpectra/data/
show how to process/plot the spectral array stored in the file.
PlotSpectralArrayFromFile.py
- allows to plot content of the spectral array as a 2-d plot.SpectralArray.py
- provides access to the spectral array stored in the file. Theclass SpectralArray
defined in this script is used in thePlotSpectralArrayFromFile.py
.
MergeArrays.py
- sums the arrays from different files defined in the list and saves resulting array in a single file with the same shape. In this script the list of files is hardwired in theget_list_of_input_file_names()
method. The output file name,out_fname
, is also hardwired in the call tospectra_merging(out_fname)
.
A few auxiliary scripts for example are located in the directory ImgAlgos/data
:
psana.cfg
- set non-default parameters to runpsana
forImgAlgos::ImgPeakFinder
andImgAlgos::ImgPeakFilter
Thepsana
running this script saves images and peaks for event 115 in text files.PlotCameraImageFromFile.py
- Plots image and spectrum for image saved in file.PlotCameraImageAndPeaks.py
- Plots image with found peaks and spectrum.
Examples for package cspad_mod
Example for module cspad_mod::CsPad2x2Pedestals
Configuration file for pedestals calibration of two CSPAD2x2 simultaneously:
[psana] files = /reg/d/psdm/xpp/xpptut13/xtc/e308-r0070-s02-c00.xtc \ /reg/d/psdm/xpp/xpptut13/xtc/e308-r0070-s03-c00.xtc modules = cspad_mod.CsPad2x2Pedestals:0 \ cspad_mod.CsPad2x2Pedestals:1 #skip-events = 100 #events = 1111 [cspad_mod.CsPad2x2Pedestals:0] source = DetInfo(XppGon.0:Cspad2x2.0) output = pedestals-ave-xppi0513-r0070-Cspad2x2.0.dat noise = pedestals-rms-xppi0513-r0070-Cspad2x2.0.dat [cspad_mod.CsPad2x2Pedestals:1] source = DetInfo(XppGon.0:Cspad2x2.1) output = pedestals-ave-xppi0513-r0070-Cspad2x2.1.dat noise = pedestals-rms-xppi0513-r0070-Cspad2x2.1.dat
Command to run this script:
psana -c psana-xppi0513-r0070-cspad2x2-pedestals.cfg
The xtc file name(s) may be passed as an argument:
psana -c psana-xppi0513-r0070-cspad2x2-pedestals.cfg /reg/d/psdm/xpp/xpptut13/xtc/e308-r0070-*.xtc
Output files contain results, which can be plotted for average values:
and rms values:
Example for package CSPadPixCoords
How to write the CSPad image in text file:
[psana] files = /reg/d/psdm/<instrument>/<experiment>/xtc/<file-name-1>.xtc events = 5 modules = cspad_mod.CsPadCalib CSPadPixCoords.CSPadImageProducer ImgAlgos.ImgSaveInFile [cspad_mod.CsPadCalib] inputKey = outputKey = calibrated doPedestals = yes doPixelStatus = no doCommonMode = no #[CSPadPixCoords.CSPadInterpolImageProducer] [CSPadPixCoords.CSPadImageProducer] calibDir = /reg/d/psdm/<instrument>/<experiment>/calib typeGroupName = CsPad::CalibV1 source = CxiDs1.0:Cspad.0 key = calibrated imgkey = Image2D tiltIsApplied = true [ImgAlgos.ImgSaveInFile] source = CxiDs1.0:Cspad.0 #eventSave = 1 saveAll = true
Example for module CSPadPixCoords::CSPad2x2ImageProducer
See Module CSPadPixCoords::CSPad2x2ImageProducer
Example of the configuration script for psana (cspad2x2-test.cfg):
[psana] files = /reg/d/psdm/<instrument>/<experiment>/xtc/<file-name-1>.xtc events = 5 modules = CSPadPixCoords.CSPad2x2ImageProducer ImgAlgos.ImgSaveInFile [CSPadPixCoords.CSPad2x2ImageProducer] source = DetInfo(:Cspad2x2) inkey = outimgkey = Image tiltIsApplied = true print_bits = 15 [ImgAlgos.ImgSaveInFile] source = DetInfo(:Cspad2x2) key = Image fname = cspad2x2 saveAll = true #eventSave = 5
Command to run:
psana -c cspad2x2-test.cfg
One of the saved files cspad2x2-<run>-<timestamp>.txt
is plotted as an image by the command
./PlotCameraImageFromFile.py cspad2x2-<run>-<timestamp>.txt 0 1200
Configuration file for cspad2x2 with pedestal subtraction
Access to the CSPad2x2 aligned geometry is added on 2013-02-13
and is available for offline release > ana-0.9.1
.
Example of <psana-config-file.cfg>:
[psana] files = /reg/d/psdm/mec/mec73313/xtc/e268-r0180-s02-c00.xtc #calib-dir = ./calib modules = cspad_mod.CsPadCalib CSPadPixCoords.CSPad2x2ImageProducer ImgAlgos.ImgSaveInFile events = 5 [cspad_mod.CsPadCalib] source = DetInfo(MecTargetChamber.0:Cspad2x2.3) inputKey = outputKey = calibrated_arr doPedestals = yes doPixelStatus = no doCommonMode = no [CSPadPixCoords.CSPad2x2ImageProducer] calibDir = /reg/d/psdm/mec/mec73313/calib typeGroupName = CsPad2x2::CalibV1 #source = DetInfo(MecTargetChamber.0:Cspad2x2.3) source = :Cspad2x2.3 inkey = calibrated_arr outimgkey = Image tiltIsApplied = true print_bits = 15 [ImgAlgos.ImgSaveInFile] source = DetInfo(MecTargetChamber.0:Cspad2x2.3) key = Image fname = cspad2x2.3 saveAll = true print_bits = 3 #eventSave = 5
Example of psana configuration file to get cspad2x2 images for two detectors and save them in files, one in txt, another in tiff formats:
[psana] files = /reg/d/psdm/xpp/xpptut13/xtc/e308-r0008-s02-c00.xtc \ /reg/d/psdm/xpp/xpptut13/xtc/e308-r0008-s03-c00.xtc #modules = cspad_mod.CsPad2x2Pedestals #calib-dir = ./calib calib-dir = /reg/d/psdm/xpp/xpptut13/xtc/calib modules = cspad_mod.CsPadCalib:0 \ cspad_mod.CsPadCalib:1 \ CSPadPixCoords.CSPad2x2ImageProducer:0 \ CSPadPixCoords.CSPad2x2ImageProducer:1 \ ImgAlgos.ImgSaveInFile:0 \ ImgAlgos.ImgSaveInFile:1 events = 5 [cspad_mod.CsPadCalib:0] source = DetInfo(XppGon.0:Cspad2x2.0) inputKey = outputKey = calibrated_arr0 doPedestals = yes doPixelStatus = no doCommonMode = yes [cspad_mod.CsPadCalib:1] source = DetInfo(XppGon.0:Cspad2x2.1) inputKey = outputKey = calibrated_arr1 doPedestals = yes doPixelStatus = no doCommonMode = yes [CSPadPixCoords.CSPad2x2ImageProducer:0] calibDir = /reg/d/psdm/xpp/xpptut13/xtc/calib typeGroupName = CsPad2x2::CalibV1 source = DetInfo(XppGon.0:Cspad2x2.0) inkey = calibrated_arr0 outimgkey = Image tiltIsApplied = false useWidePixCenter = false print_bits = 15 [CSPadPixCoords.CSPad2x2ImageProducer:1] calibDir = /reg/d/psdm/xpp/xpptut13/xtc/calib typeGroupName = CsPad2x2::CalibV1 source = DetInfo(XppGon.0:Cspad2x2.1) inkey = calibrated_arr1 outimgkey = Image tiltIsApplied = false useWidePixCenter = false print_bits = 15 [ImgAlgos.ImgSaveInFile:0] source = DetInfo(:Cspad2x2.0) key = Image fname = cspad2x2.0 ftype = txt #ftype = tiff saveAll = true print_bits = 3 #eventSave = 5 [ImgAlgos.ImgSaveInFile:1] source = DetInfo(:Cspad2x2.1) key = Image fname = cspad2x2.1 #ftype = txt ftype = tiff saveAll = true print_bits = 3 #eventSave = 5
Example for package ImgPixSpectra
Modules:
- ImgPixSpectra::CSPadPixSpectra
- ImgPixSpectra::CSPad2x2PixSpectra
- ImgPixSpectra::CameraPixSpectra
Example for module ImgPixSpectra::CSPadPixSpectra
See module description in Module ImgPixSpectra::CSPadPixSpectra
Configuration file psana-cxib2313-r0114-cspad-pix-spectra.cfg
:
# Command to run this script: # psana -c psana-cxib2313-r0114-cspad-pix-spectra.cfg # # Other useful commands: # psana -n 5 -m PrintSeparator,PrintEventId,psana_examples.DumpCsPad /reg/d/psdm/cxi/cxib2313/xtc/e336-r0114* # psana -n 5 -m EventKeys exp=cxib2313:run=114:xtc [psana] files = exp=cxib2313:run=114:xtc #calib-dir = ./calib skip-events = 0 events = 100 modules = cspad_mod.CsPadCalib ImgPixSpectra.CSPadPixSpectra [cspad_mod.CsPadCalib] source = DetInfo(CxiDs1.0:Cspad.0) inputKey = outputKey = calibrated doPedestals = yes doPixelStatus = no doCommonMode = yes [ImgPixSpectra.CSPadPixSpectra] source = CxiDs1.0:Cspad.0 inputKey = calibrated amin = -20. amax = 20. nbins = 10 arr_fname = cspad_spectral_array.txt
where module cspad_mod.CsPadCalib
subtracts pedestals, apply common mode correction, and save CSPAD array in the event store with key "calibrated", which is used in the next module ImgPixSpectra.CSPadPixSpectra
.
To run this script use command
psana -c psana-cxib2313-r0114-cspad-pix-spectra.cfg
which produces two files:
cspad_spectral_array.txt
– array of 10-bin amplitude spectra for all pixelscspad_spectral_array.txt.sha
– file with metadata for array shape:NPIXELS 2296960 NBINS 10 AMIN -20 AMAX 20 NEVENTS 100 ARRFNAME cspad_spectral_array.txt
Plot for content of the file cspad_spectral_array.txt
:
Example for module ImgPixSpectra::CSPad2x2PixSpectra
See module description in Module ImgPixSpectra::CSPad2x2PixSpectra
Configuration file example for CSPad2x2PixSpectra
:
[psana] files = /reg/d/psdm/<instrument>/<experiment>/<file-name>.xtc modules = ImgPixSpectra.CSPad2x2PixSpectra [ImgPixSpectra.CSPad2x2PixSpectra] source = CxiSc1.0:Cspad2x2.0 amin = 500. amax = 1000. nbins = 100 arr_fname = cspad2x2-pix-spectra.txt
To get images from saved file one may execute the auxiliary script:
ImgPixSpectra/data/PlotSpectralArrayFromFile.py cspad2x2-pix-spectra.txt
generates image for limited range of pixels for CSPad, CSPad2x2, or Camera, respectively:
Examples for package ImgAlgos
See Package ImgAlgos
Example for module ImgAlgos::Tahometer
See Module ImgAlgos::Tahometer
Example of the psana configuration file:
[psana] files = /reg/d/psdm/<INSTRUMENT>/<experiment>/xtc/<file-name-1>.xtc\ /reg/d/psdm/<INSTRUMENT>/<experiment>/xtc/<file-name-2>.xtc modules = ImgAlgos.Tahometer [ImgAlgos.Tahometer] dn = 10 print_bits = 7
Example for module ImgAlgos::PnccdImageProducer
See Module ImgAlgos::PnccdImageProducer
Example of the psana configuration file:
[psana] files = /reg/d/psdm/<INSTRUMENT>/<experiment>/xtc/<file-name-1>.xtc\ /reg/d/psdm/<INSTRUMENT>/<experiment>/xtc/<file-name-2>.xtc #skip-events = 100 events = 5 modules = ImgAlgos.PnccdImageProducer ImgAlgos.ImgSaveInFile [ImgAlgos.PnccdImageProducer] source = DetInfo(:pnCCD) inkey = outimgkey = imgpnccd print_bits = 1 [ImgAlgos.ImgSaveInFile] source = DetInfo(:pnCCD) key = imgpnccd fname = pnccd-img-ev saveAll = true #eventSave = 82 print_bits = 1
This script saves text files with images like pnccd-img-ev-<run-date-time.nsec>.txt
, which can be presented as:
Example for module ImgAlgos::CameraImageProducer
See Module ImgAlgos::CameraImageProducer
Example of the psana configuration file:
[psana] files = /reg/d/psdm/<INSTRUMENT>/<experiment>/xtc/<file-name-1>.xtc modules = ImgAlgos.CameraImageProducer ImgAlgos.ImgSaveInFile events = 5 [ImgAlgos.CameraImageProducer] source = DetInfo(:Opal1000) key_in = key_out = img subtract_offset = true print_bits = 15 [ImgAlgos.ImgSaveInFile] source = DetInfo(:Opal1000) key = img fname = img-from-my-experiment saveAll = true #eventSave = 1
This script saves text files with images like img-from-my-experiment-<run-date-time.nsec>.txt
, which can be drawn by the python script
./ImgAlgos/data/PlotCameraImageFromFile.py <filename>.txt <Amin> <Amax>
Example for module ImgAlgos::PrincetonImageProducer
See Module ImgAlgos::PrincetonImageProducer
Example of the psana configuration file:
[psana] files = /reg/d/psdm/<INSTRUMENT>/<experiment>/xtc/<file-name-1>.xtc\ /reg/d/psdm/<INSTRUMENT>/<experiment>/xtc/<file-name-2>.xtc modules = ImgAlgos.PrincetonImageProducer \ ImgAlgos.ImgSaveInFile events = 3 [ImgAlgos.PrincetonImageProducer] source = DetInfo(:Princeton) key_in = key_out = img subtract_offset = true print_bits = 31 [ImgAlgos.ImgSaveInFile] source = DetInfo(:Princeton) key = img fname = img-xcs saveAll = true print_bits = 31
Example for module ImgAlgos::AcqirisArrProducer
See description of parameters in Module ImgAlgos::AcqirisArrProducer
Example of the psana configuration file psana-amo01509-r0125-acqiris.cfg
:
# Command to run this script: # psana -c psana-amo01509-r0125-acqiris.cfg; # # Useful commands: # psana -n 5 -m EventKeys exp=amo01509:run=125:xtc > test-acqiris-file.txt; # psana -n 5 -m psana_examples.DumpAcqiris exp=amo01509:run=125:xtc > test-acqiris-file.txt; (C++ version) # psana -n 1 -m psana_examples.dump_acqiris exp=amo01509:run=125:xtc > test-acqiris-file.txt; (python version) [psana] #files = /reg/d/psdm/AMO/amo01509/xtc/e8-r0125-s00-c00.xtc /reg/d/psdm/AMO/amo01509/xtc/e8-r0125-s01-c00.xtc files = exp=amo01509:run=125:xtc modules = ImgAlgos.AcqirisArrProducer ImgAlgos.ImgSaveInFile:wf ImgAlgos.ImgSaveInFile:wt skip-events = 0 events = 100 [ImgAlgos.AcqirisArrProducer] source = AmoETOF.0:Acqiris.0 key_in = key_wform = acqiris_wform key_wtime = acqiris_wtime fname_prefix = acq print_bits = 11 [ImgAlgos.ImgSaveInFile:wf] source = AmoETOF.0:Acqiris.0 key = acqiris_wform fname = acq-AmoETOF-wform ftype = txt #ftype = tiff #saveAll = true print_bits = 3 eventSave = 5 [ImgAlgos.ImgSaveInFile:wt] source = AmoETOF.0:Acqiris.0 key = acqiris_wtime fname = acq-AmoETOF-wtime ftype = txt #ftype = tiff #saveAll = true print_bits = 3 eventSave = 5
This script with psana does a few things:
- module AcqirisArrProducer gets Acqiris data objects from event store, adjusts trigger time corrections, and saves them back in the event store as uniform ndarrays<double,2> objects for waveforms and times
- two instances of the module ImgSaveInFile save arrays of waveforms and wave-times for locally counted event 5.
This script saves 3 text files:
acq-amo01509-r0125.txt
-- with configuration parameters:Acqiris::ConfigV1: nbrBanks=1 channelMask=69905 nbrChannels=5 nbrConvertersPerChannel=4 horiz: sampInterval=2.5e-10 delayTime=0 nbrSegments=1 nbrSamples=10000 vert(0): fullScale=0.1 slope=1.52588e-06 offset=0 coupling=3 bandwidth=0 vert(1): fullScale=0.1 slope=1.52588e-06 offset=0 coupling=3 bandwidth=0 vert(2): fullScale=0.1 slope=1.52588e-06 offset=0 coupling=3 bandwidth=0 vert(3): fullScale=0.1 slope=1.52588e-06 offset=0 coupling=3 bandwidth=0 vert(4): fullScale=0.1 slope=1.52588e-06 offset=0 coupling=3 bandwidth=0
- acq-AmoETOF-wform-r0125-20091018-182512.194787218.txt – with waveforms for 5th event
- acq-AmoETOF-wtime-r0125-20091018-182512.194787218.txt – with wave-times for 5th event
Arrays from these files can be plotted for all channels, shown by different colors:
Example for module ImgAlgos::AcqirisAverage
See description of parameters in Module ImgAlgos::AcqirisAverage
Configuration file psana-amo01509-r0125-acqiris-average.cfg:
# Command to run this script: # psana -c psana-amo01509-r0125-acqiris-average.cfg; # # Useful commands: # psana -n 5 -m EventKeys exp=amo01509:run=125:xtc > test-acqiris-file.txt; # psana -n 5 -m psana_examples.DumpAcqiris exp=amo01509:run=125:xtc > test-acqiris-file.txt; (C++ version) # psana -n 1 -m psana_examples.dump_acqiris exp=amo01509:run=125:xtc > test-acqiris-file.txt; (python version) [psana] #files = /reg/d/psdm/AMO/amo01509/xtc/e8-r0125-s00-c00.xtc /reg/d/psdm/AMO/amo01509/xtc/e8-r0125-s01-c00.xtc files = exp=amo01509:run=125:xtc modules = ImgAlgos.AcqirisArrProducer ImgAlgos.AcqirisAverage skip-events = 0 events = 1000 [ImgAlgos.AcqirisArrProducer] source = AmoETOF.0:Acqiris.0 key_in = key_wform = acqiris_wform key_wtime = acqiris_wtime fname_prefix = acq print_bits = 3 [ImgAlgos.AcqirisAverage] source = AmoETOF.0:Acqiris.0 key_in = acqiris_wform key_ave = acqiris_average fname_ave_prefix = acq thresholds = -0.005 -0.005 -0.005 -0.005 -0.005 is_positive_signal = no do_inverse_selection = yes #skip_events = 0 #proc_events = 100 print_bits = 255
Psana with this script runs over 1000 events apply threshold-based selection algorithm and produces files:
acq-amo01509-r0125-config.txt -- with Acqiris configuration parameters:
Acqiris::ConfigV1: nbrBanks=1 channelMask=69905 nbrChannels=5 nbrConvertersPerChannel=4 horiz: sampInterval=2.5e-10 delayTime=0 nbrSegments=1 nbrSamples=10000 vert(0): fullScale=0.1 slope=1.52588e-06 offset=0 coupling=3 bandwidth=0 vert(1): fullScale=0.1 slope=1.52588e-06 offset=0 coupling=3 bandwidth=0 vert(2): fullScale=0.1 slope=1.52588e-06 offset=0 coupling=3 bandwidth=0 vert(3): fullScale=0.1 slope=1.52588e-06 offset=0 coupling=3 bandwidth=0 vert(4): fullScale=0.1 slope=1.52588e-06 offset=0 coupling=3 bandwidth=0
- acq-amo01509-r0125-ave-wfs.txt with averaged array of waveforms, which were below threshold (averaging for baseline level):
Example for module ImgAlgos::AcqirisCalib
See description of parameters in Module ImgAlgos::AcqirisCalib
Configuration file psana-amo01509-r0125-acqiris-calib.cfg:
# Command to run this script: # psana -c psana-amo01509-r0125-acqiris-calib.cfg; # # Useful commands: # psana -n 5 -m EventKeys exp=amo01509:run=125:xtc > test-acqiris-file.txt; # psana -n 5 -m psana_examples.DumpAcqiris exp=amo01509:run=125:xtc > test-acqiris-file.txt; (C++ version) # psana -n 1 -m psana_examples.dump_acqiris exp=amo01509:run=125:xtc > test-acqiris-file.txt; (python version) [psana] #files = /reg/d/psdm/AMO/amo01509/xtc/e8-r0125-s00-c00.xtc /reg/d/psdm/AMO/amo01509/xtc/e8-r0125-s01-c00.xtc files = exp=amo01509:run=125:xtc modules = ImgAlgos.AcqirisArrProducer ImgAlgos.AcqirisCalib ImgAlgos.ImgSaveInFile:wf_raw ImgAlgos.ImgSaveInFile:wf_calib skip-events = 0 events = 10 [ImgAlgos.AcqirisArrProducer] source = AmoETOF.0:Acqiris.0 key_in = key_wform = acqiris_wform key_wtime = acqiris_wtime fname_prefix = acq print_bits = 1 [ImgAlgos.AcqirisCalib] source = AmoETOF.0:Acqiris.0 key_in = acqiris_wform key_out = wf-calibrated fname_base_line = acq-amo01509-r0125-ave-wfs.txt #skip_events = 0 #proc_events = 100 print_bits = 255 [ImgAlgos.ImgSaveInFile:wf_raw] source = AmoETOF.0:Acqiris.0 key = acqiris_wform fname = acq-AmoETOF-wform-raw ftype = txt #ftype = tiff #saveAll = true print_bits = 3 eventSave = 5 [ImgAlgos.ImgSaveInFile:wf_calib] source = AmoETOF.0:Acqiris.0 key = wf-calibrated fname = acq-AmoETOF-wform-calibrated ftype = txt #ftype = tiff #saveAll = true print_bits = 3 eventSave = 5
In this script the base-line level for all waveforms is loaded from file and is subtracted in module ImgAlgos.AcqirisCalib.
For example, the raw and calibrated waveforms for event 5 were saved in the files:
acq-AmoETOF-wform-raw-r0125-e00000005-20091018-182512.194787218.txt
acq-AmoETOF-wform-calibrated-r0125-e00000005-20091018-182512.194787218.txt
which content is presented on plots:
Example for module ImgAlgos::AcqirisCFD
See description of parameters in Module ImgAlgos::AcqirisCFD
Configuration file psana_cfd.cfg:
# Command to run this script: # psana -c psana_cfd.cfg; # [psana] modules = ImgAlgos.AcqirisArrProducer ImgAlgos.AcqirisCalib ImgAlgos.AcqirisCFD files = /reg/d/psdm/AMO/amo01509/xtc/e8-r0125-s00-c00.xtc [ImgAlgos.AcqirisArrProducer] source = AmoETOF.0:Acqiris.0 key_in = key_wform = acqiris_wform key_wtime = acqiris_wtime fname_prefix = acq print_bits = 0 [ImgAlgos.AcqirisCalib] source = AmoETOF.0:Acqiris.0 key_in = acqiris_wform key_out = wf-calibrated fname_base_line = acq--r0000-ave-wfs.txt #skip_events = 0 #proc_events = 100 print_bits = 0 [ImgAlgos.AcqirisCFD] source = AmoETOF.0:Acqiris.0 key_wform = wf-calibrated baselines = 0.0 0.0 0.0 0.0 0.0 thresholds = -0.005 -0.005 -0.005 -0.005 -0.005 fractions = 0.5 0.5 0.5 0.5 0.5 deadtimes = 20.0e-9 20.0e-9 20.0e-9 20.0e-9 20.0e-9 leading_edges = 1 1 1 1 1
This script analyzes an AMO run where 5 acqiris channels were in use. It uses an AcqirisArrProducer to producer the list of waveforms/times for all channels. It then uses an AcqirisCalib module to do a baseline subtraction using a previously generated file of baselines act--r0000-ave-wfs.txt. Finally, a constant fraction discriminator algorithm is run on all the waveforms with user specified parameters. The edges calculated by AcqirisCFD are saved to the event as one ndarray<double,1> per channel, each with a (default) key "acqiris_edges_N" where N is the channel number. Channels where no edges were found are not saved to the event.
Example for combination of Acqiris modules
See description of parameters in Modules ImgAlgos::AcqirisArrProducer, AcqirisAverage, and AcqirisCalib
Configuration file psana-amo01509-r0125-acqiris-comb.cfg:
# Command to run this script: # psana -c psana-amo01509-r0125-acqiris-comb.cfg; [psana] files = exp=amo01509:run=125:xtc modules = ImgAlgos.AcqirisArrProducer ImgAlgos.AcqirisAverage:bl ImgAlgos.AcqirisCalib ImgAlgos.AcqirisAverage:signal ImgAlgos.Tahometer #skip-events = 0 events = 2010 [ImgAlgos.AcqirisArrProducer] source = AmoETOF.0:Acqiris.0 key_in = key_wform = acqiris_wform key_wtime = acqiris_wtime fname_prefix = acq print_bits = 7 [ImgAlgos.AcqirisAverage:bl] source = AmoETOF.0:Acqiris.0 key_in = acqiris_wform #key_ave = fname_ave_prefix = acq-bline thresholds = -0.005 -0.005 -0.005 -0.005 -0.005 is_positive_signal = no do_inverse_selection = yes skip_events = 0 proc_events = 1000 print_bits = 31 [ImgAlgos.AcqirisCalib] source = AmoETOF.0:Acqiris.0 key_in = acqiris_wform key_out = wf-calibrated fname_base_line = acq-bline skip_events = 1001 proc_events = 1000 print_bits = 47 [ImgAlgos.AcqirisAverage:signal] source = AmoETOF.0:Acqiris.0 key_in = wf-calibrated #key_ave = fname_ave_prefix = acq-signal thresholds = -0.01 -0.01 -0.01 -0.01 -0.01 is_positive_signal = no do_inverse_selection = no skip_events = 1001 proc_events = 1000 print_bits = 31 [ImgAlgos.Tahometer] print_bits = 7
This script works with psana as follows:
- for the 1st 1000 events averages waveforms below threshold and saves results in the file acq-bline-amo01509-r0125-ave-wfs.txt;
- for the next 1000 events subtracts baseline level and averages waveforms above thresholds and saves results in the file acq-signal-amo01509-r0125-ave-wfs.txt.
This script produces three files:
acq-amo01509-r0125-config.txt - with Acqris configuration parameters:
Acqiris::ConfigV1: nbrBanks=1 channelMask=69905 nbrChannels=5 nbrConvertersPerChannel=4 horiz: sampInterval=2.5e-10 delayTime=0 nbrSegments=1 nbrSamples=10000 vert(0): fullScale=0.1 slope=1.52588e-06 offset=0 coupling=3 bandwidth=0 vert(1): fullScale=0.1 slope=1.52588e-06 offset=0 coupling=3 bandwidth=0 vert(2): fullScale=0.1 slope=1.52588e-06 offset=0 coupling=3 bandwidth=0 vert(3): fullScale=0.1 slope=1.52588e-06 offset=0 coupling=3 bandwidth=0 vert(4): fullScale=0.1 slope=1.52588e-06 offset=0 coupling=3 bandwidth=0
- acq-bline-amo01509-r0125-ave-wfs.txt - contains baseline averaged arrays, which can be presented by full scale and zoomed plots:
- acq-signal-amo01509-r0125-ave-wfs.txt- contains signal averaged arrays, which can be presented by full scale and zoomed plots:
Example for module ImgAlgos::NDArrAverage
- See Module ImgAlgos::NDArrAverage
The
NDArrAverage
module can be used for evaluation of averaged pedestals or background using dedicated runs.
Typical configuration file may looks like this:# Run this script: # psana -c psana-meca1113-r0045-cspad-cspad-dark-hotpix.cfg [psana] files = exp=meca1113:run=45 events = 400 #skip-events = 0 modules = CSPadPixCoords.CSPadNDArrProducer \ ImgAlgos.NDArrAverage \ ImgAlgos.Tahometer [CSPadPixCoords.CSPadNDArrProducer] source = MecTargetChamber.0:Cspad.0 inkey = outkey = cspad_ndarr outtype = int16 is_fullsize = yes print_bits = 3 [ImgAlgos.NDArrAverage] source = MecTargetChamber.0:Cspad.0 key = cspad_ndarr avefile = cspad.0-ave rmsfile = cspad.0-rms maskfile = cspad.0-msk hotpixfile = cspad.0-hot thr_rms_ADU = 10 thr_min_ADU = 4 thr_max_ADU = 10000 print_bits = 29 [ImgAlgos.Tahometer] dn = 100 print_bits = 7
Example for module ImgAlgos::ImgAverage
- See Module ImgAlgos::ImgAverage
- The
ImgAverage
module can be used for evaluation of averaged pedestals or background using dedicated runs. Typical configuration file may looks like this:
[psana] files = /reg/d/psdm/<instrument>/<experiment>/xtc/<file-name>.xtc modules = ImgAlgos.CameraImageProducer \ ImgAlgos.ImgAverage events = 1000 [ImgAlgos.CameraImageProducer] source = DetInfo(:Opal1000) key_in = key_out = img subtract_offset = true print_bits = 1 [ImgAlgos.ImgAverage] source = DetInfo(:Opal1000) key = img avefile = img-ave.dat rmsfile = img-rms.dat print_bits = 31 evts_stage1 = 100 evts_stage2 = 100 gate_width1 = 200 gate_width2 = 20
Example for module ImgAlgos::ImgMaskEvaluation
- See Module ImgAlgos::ImgMaskEvaluation
- Configuration parameters for psana:
[ImgAlgos.ImgMaskEvaluation] source = DetInfo(:Opal1000) key = img file_mask_satu = img-mask-satu.dat file_mask_nois = img-mask-nois.dat file_mask_comb = img-mask-comb.dat file_frac_satu = img-frac-satu.dat file_frac_nois = img-frac-nois.dat thre_satu = 400 frac_satu = 0 dr = 1 thre_SoN = 3 frac_nois = 0.05 print_bits = 63
In this example parameters were chosen in order to get a small number of "noisy" pixel just due to statistics.
- Typical image:
- Plots for fraction of noisy pixels:
- Plots for fraction of saturated pixels:
- Masks: noisy, saturated, and combined:
Example for module ImgAlgos::ImgCalib
- See Module ImgAlgos::ImgCalib
[ImgAlgos.CameraImageProducer] source = DetInfo(:Opal1000) key_in = key_out = img subtract_offset = true print_bits = 1 [ImgAlgos.ImgCalib] source = DetInfo(:Opal1000) key_in = img key_out = calibrated fname_peds = <pedestal-file-name> fname_mask = <mask-file-name> fname_bkgd = fname_gain = print_bits = 31
- Example of the mask file and resulting image:
Example for module ImgAlgos::ImgRadialCorrection
- See Module ImgAlgos::ImgRadialCorrection
[psana] files = /reg/d/psdm/<instrument>/<experiment>/xtc/<file-name-1>.xtc \ /reg/d/psdm/<instrument>/<experiment>/xtc/<file-name-2>.xtc \ ... /reg/d/psdm/<instrument>/<experiment>/xtc/<file-name-N>.xtc skip-events = 500 events = 10 modules = cspad_mod.CsPadCalib \ # ImgAlgos.CSPadBkgdSubtract \ CSPadPixCoords.CSPadImageProducer \ ImgAlgos.ImgRadialCorrection \ ImgAlgos.ImgSaveInFile:1 [cspad_mod.CsPadCalib] inputKey = outputKey = calibrated doPedestals = yes doPixelStatus = no doCommonMode = no [ImgAlgos.CSPadBkgdSubtract] source = DetInfo(CxiDs1.0:Cspad.0) inputKey = calibrated outputKey = bkgd_subtracted_arr bkgd_fname = <the-file-name-with-background-array> norm_sector = 0 print_bits = 0 [CSPadPixCoords.CSPadImageProducer] calibDir = /reg/d/psdm/<instrument>/<experiment>/calib typeGroupName = CsPad::CalibV1 source = CxiDs1.0:Cspad.0 key = calibrated imgkey = current_img #tiltIsApplied = true [ImgAlgos.ImgRadialCorrection] source = DetInfo(CxiDs1.0:Cspad.0) inkey = current_img outkey = r_cor_img xcenter = 866 ycenter = 857 rmin = 100 rmax = 810 n_phi_bins = 60 event = 0 print_bits = 3 [ImgAlgos.ImgSaveInFile:1] source = CxiDs1.0:Cspad.0 key = r_cor_img fname = <file-name-for-image-array> #saveAll = true eventSave = 8
- Note: the option of the background subtraction (
ImgAlgos.CSPadBkgdSubtract
) is commented out in this configuration file . In order to evoke this option, the comment sign (#) should be removed from the list ofmodules
and thekey=bkgd_subtracted_arr
should be used inCSPadPixCoords.CSPadImageProducer
. - Calibrated image and spectrum:
- Calibrated and radial-corrected image, spectrum, and subtracted r-phi65 distribution for
n_phi_bins
=65: - Calibrated and radial-corrected image, spectrum, and subtracted r-phi12 distribution for
n_phi_bins
=12: Example for module ImgAlgos::ImgPeakFinder
- See Module ImgAlgos::ImgPeakFinder
- Configuration file example:
[psana] files = /reg/d/psdm/<instrument>/<experiment>/xtc/<file-name-1>.xtc \ /reg/d/psdm/<instrument>/<experiment>/xtc/<file-name-2>.xtc \ ... /reg/d/psdm/<instrument>/<experiment>/xtc/<file-name-N>.xtc modules = ImgAlgos.ImgPeakFinder PrintSeparator #skip-events = 500 events = 120 [ImgAlgos.ImgPeakFinder] source = DetInfo(:Opal1000) key = peaksKey = peaks threshold_low = 20 threshold_high = 50 sigma = 1.5 smear_radius = 2 peak_radius = 3 xmin = 200 xmax = 800 ymin = 100 ymax = 900 testEvent = 115 print_bits = 0 finderIsOn = true
- This algorithm consumes ~15 ms/event on psana0101 for full Opal1000 (1024x1024) camera image.
- Smearing algorithm use a "safety margin" which is currently set to 10 pixels (offset from each boarder of the full image size).
- Image on different stages of this algorithm:
- raw image,
- image in the window with amplitudes above the
threshold_low
- few peaks at the edges were discarded by the window limits,
- image still contains many 1-photon pixels, which need to be eliminated,
- smeared image,
- raw image with found peaks (marked by the red circles)
- zoom of the previous plot.
Example for module ImgAlgos::ImgPeakFilter
[ImgAlgos.ImgPeakFilter] source = DetInfo(:Opal1000) key = peaks threshold_peak = 5 threshold_total= 0 n_peaks_min = 10 print_bits = 11 fname = img selection_mode = SELECTION_ON
Example for module ImgAlgos::ImgPeakFinderAB
- See Module ImgAlgos::ImgPeakFinderAB
- Configuration file example:
[psana] files = /reg/d/psdm/<instrument>/<experiment>/xtc/<file-name>.xtc modules = ImgAlgos.CameraImageProducer \ ImgAlgos.ImgPeakFinderAB events = 10 [ImgAlgos.CameraImageProducer] source = DetInfo(:Opal1000) key_in = key_out = img subtract_offset = true print_bits = 1 [ImgAlgos.ImgPeakFinderAB] source = DetInfo(:Opal1000) key = img key_peaks_out = peaks #key_signal_out = signal-arr #hot_pix_mask_inp_file = ana-misc-exp/mask.dat #hot_pix_mask_out_file = noise-mask-out.dat #frac_noisy_evts_file = noise-frac-out.dat evt_file_out = tmp/img- rmin = 10 dr = 1 SoNThr_noise = 3 SoNThr_signal = 3 frac_noisy_imgs = 0.9 peak_npix_min = 3 peak_npix_max = 100 peak_amp_tot_thr = 0. peak_SoN_thr = 4. event_npeak_min = 5 event_npeak_max = 1000 event_amp_tot_thr = 0. nevents_mask_update = 0 nevents_mask_accum = 50 selection_mode = SELECTION_ON out_file_bits = 15 print_bits = 513
- Results:
Example for module ImgAlgos::ImgHitFinder
- See Module ImgAlgos::ImgHitFinder
- ImgHitFinder in regular mode needs in file with pedestals (offset) to correct the image and file with threshold.
- In amo74213 run 93 these files can be obtained directly from data, discarding signal hits as outliers using
- ImgAlgos.ImgAverage module as follows with configuration file:
# File: psana-amo74213-r0093-opal-img-average.cfg [psana] #files = /reg/d/psdm/AMO/amo74213/xtc/e269-r0093-s05-c00.xtc files = exp=amo74213:run=93:xtc modules = ImgAlgos.CameraImageProducer \ ImgAlgos.ImgAverage skip-events = 0 events = 1000 [ImgAlgos.CameraImageProducer] source = DetInfo(:Opal1000) key_in = key_out = img subtract_offset = true print_bits = 1 [ImgAlgos.ImgAverage] source = DetInfo(:Opal1000) key = img avefile = img-ave-for-peds rmsfile = img-rms-for-thre evts_stage1 = 100 evts_stage2 = 100 gate_width1 = 50 gate_width2 = 10 print_bits = 31
- Run psana using command:
psana -c psana-amo74213-r0093-opal-img-average.cfg
- At the end of this procedure two files will be created:
- img-ave-for-peds-r0093.dat - may be used for pedestal subtraction:
- img-rms-for-thre-r0093.dat - may be used multiplied by number of rms as a threshold:
- The file with accumulated pixel hits can be obtained using configuration file:
# File: psana-amo74213-r0093-opal-img-hit-finder.cfg [psana] #files = /reg/d/psdm/AMO/amo74213/xtc/e269-r0093-s05-c00.xtc files = exp=amo74213:run=93:xtc modules = ImgAlgos.CameraImageProducer \ ImgAlgos.ImgHitFinder \ ImgAlgos.ImgAverage skip-events = 0 events = 1000 [ImgAlgos.CameraImageProducer] source = DetInfo(:Opal1000) key_in = key_out = img subtract_offset = true print_bits = 1 [ImgAlgos.ImgHitFinder] source = DetInfo(:Opal1000) key_in = img key_out = img_hits fname_peds = img-ave-for-peds-r0093.dat fname_mask = fname_gain = fname_thre = img-rms-for-thre-r0093.dat masked_value = 0 thre_mode = 3 #thre_mode = 2 thre_param = 5 thre_below_value = 0 thre_above_value = 1 win_row_min = 10 win_row_max = 1000 win_col_min = 10 win_col_max = 1000 print_bits = 39 [ImgAlgos.ImgAverage] source = DetInfo(:Opal1000) key = img_hits sumfile = img-sum-result print_bits = 25
- and run it by the command:
psana -c psana-amo74213-r0093-opal-img-hit-finder.cfg
- Which creates the file: img-sum-result-r0093.dat for
thre_mode = 2
andthre_mode = 3
, respectively: Example for module ImgAlgos::ImgSpectra
- See Module ImgAlgos::ImgSpectra
- Configuration file for psana:
[psana] files = /reg/d/psdm/<instrument>/<experiment>/xtc/<file-name>.xtc modules = ImgAlgos.CameraImageProducer \ ImgAlgos.ImgSpectra \ ImgAlgos.ImgSaveInFile:2 # ImgAlgos.ImgSaveInFile # psana_examples.DumpOpal1k \ events = 100 [ImgAlgos.CameraImageProducer] source = DetInfo(:Opal1000) key_in = key_out = img subtract_offset = true print_bits = 1 [ImgAlgos.ImgSpectra] source = DetInfo(:Opal1000) key_in = img key_out = spectra sig_band_rowc = 512. ref_band_rowc = 552. sig_band_tilt = 0. ref_band_tilt = 0. sig_band_width = 10 ref_band_width = 10 print_bits = 3 [ImgAlgos.ImgSpectraProc] source = DetInfo(:Opal1000) key_in = spectra print_bits = 15 [ImgAlgos.ImgSaveInFile:2] source = DetInfo(:Opal1000) key = spectra fname = spec-xppi0412 saveAll = true [ImgAlgos.ImgSaveInFile] source = DetInfo(:Opal1000) key = img fname = img-xppi0412 saveAll = true
- This script can be used in order to produce text files with image and spectral array:
- or graphics for several images:
Example for module ImgAlgos::ImgSpectraProc
- See Module ImgAlgos::ImgSpectraProc
- Configuration file for psana:
[ImgAlgos.ImgSpectraProc] source = DetInfo(:Opal1000) key_in = spectra print_bits = 15
- For each event it prints something similar to:
[info:ImgAlgos.ImgSpectraProc] Spectral array shape =3, 1024 [info:ImgAlgos.ImgSpectraProc] Image spectra for run=0060 Evt=000100 Column: 0 100 200 300 400 500 600 700 800 900 1000 Signal: 1211 4062 11150 17070 16406 12949 7991 5168 3968 3542 3811 Refer.: 933 3485 10425 17128 17791 13522 8315 5000 3390 2967 3193 Diff. : 0.259 0.153 0.067 -0.003 -0.081 -0.043 -0.040 0.033 0.157 0.177 0.176 [info:ImgAlgos.ImgSpectraProc] Run=0060 Evt=000100 Time=20120507-125420.982421325 done...
Example for module ImgAlgos::ImgSaveInFile
modules = ... ImgAlgos.ImgSaveInFile:1 ... [ImgAlgos.ImgSaveInFile:1] source = DetInfo(:Opal1000) # or CxiDs1.0:Cspad.0 key = img fname = my-img #ftype = txt #ftype = bin #ftype = png ftype = tiff #eventSave = 5 saveAll = true
- See Module ImgAlgos::ImgSaveInFile
Example for module ImgPeakFinder and ImgPeakFilter for CSPad
- Module
ImgAlgos::ImgPeakFinder
works on image. In order to apply this algorithm to CSPad the image should be produced. In next example the image is produced using consequtive modulescspad_mod.CsPadCalib
,ImgAlgos.CSPadMaskApply
, andCSPadPixCoords.CSPadImageProducer
:
[psana] files = /reg/d/psdm/<instrument>/<experiment>/xtc/<file-name-1>.xtc \ ... /reg/d/psdm/<instrument>/<experiment>/xtc/<file-name-N>.xtc events = 1000 experiment = cxii0212 calib-dir = ana-cxii0212/calib modules = cspad_mod.CsPadCalib \ ImgAlgos.CSPadMaskApply \ CSPadPixCoords.CSPadImageProducer \ ImgAlgos.ImgPeakFinder \ ImgAlgos.ImgPeakFilter \ ImgAlgos.ImgSaveInFile:1 [cspad_mod.CsPadCalib] inputKey = outputKey = calibrated doPedestals = yes doPixelStatus = no doCommonMode = yes [ImgAlgos.CSPadMaskApply] source = DetInfo(CxiDs1.0:Cspad.0) inkey = calibrated outkey = masked_arr mask_fname = <your-local-directory>/<mask-file-name>.dat masked_amp = 0 print_bits = 5 mask_control_bits = 15 [CSPadPixCoords.CSPadImageProducer] calibDir = /reg/d/psdm/<instrument>/<experiment>/calib typeGroupName = CsPad::CalibV1 source = CxiDs1.0:Cspad.0 key = masked_arr imgkey = img print_bits = 0 #tiltIsApplied = true [ImgAlgos.ImgPeakFinder] source = DetInfo(CxiDs1.0:Cspad.0) key = img peaksKey = peaks threshold_low = 2 threshold_high = 5 sigma = 1.5 smear_radius = 5 peak_radius = 7 xmin = 20 xmax = 1700 ymin = 20 ymax = 1700 #testEvent = 5 print_bits = 3 #finderIsOn = true [ImgAlgos.ImgPeakFilter] source = DetInfo(CxiDs1.0:Cspad.0) key = peaks threshold_peak = 5 threshold_total= 0 n_peaks_min = 10 print_bits = 11 fname = cspad-img selection_mode = SELECTION_ON [ImgAlgos.ImgSaveInFile:1] source = CxiDs1.0:Cspad.0 key = img fname = cspad-img #eventSave = 1 saveAll = true
Example for module ImgAlgos::CSPadArrAverage
- See Module ImgAlgos::CSPadArrAverage
- Configuration file example for evaluation of pedestals:
[psana] modules = ImgAlgos.CSPadArrAverage files = <path-to-the-dark-run-file>.xtc [ImgAlgos.CSPadArrAverage] source = DetInfo(CxiDs1.0:Cspad.0) key = avefile = cspad-pedestals-ave.dat rmsfile = cspad-pedestals-rms.dat print_bits = 15 evts_stage1 = 100 evts_stage2 = 100 gate_width1 = 100 gate_width2 = 10
- Configuration file example for evaluation of background:
[psana] files = <path-to-the-background-run-file>.xtc modules = cspad_mod.CsPadCalib ImgAlgos.CSPadArrAverage skip-events = 500 events = 1000000 [cspad_mod.CsPadCalib] inputKey = outputKey = calibrated doPedestals = yes doPixelStatus = no doCommonMode = no [ImgAlgos.CSPadArrAverage] source = DetInfo(CxiDs1.0:Cspad.0) key = calibrated avefile = cspad-background-ave.dat rmsfile = cspad-background-rms.dat print_bits = 15
- Images of the CSPad arrays for averaged and rms values, respectively, in one of the CXI runs:
Example for module ImgAlgos::CSPadBkgdSubtract
- See Module ImgAlgos::CSPadBkgdSubtract
[psana] files = /reg/d/psdm/<instrument>/<experiment>/xtc/<file-name-1>.xtc \ /reg/d/psdm/<instrument>/<experiment>/xtc/<file-name-2>.xtc \ ... /reg/d/psdm/<instrument>/<experiment>/xtc/<file-name-N>.xtc skip-events = 500 events = 10 modules = cspad_mod.CsPadCalib ImgAlgos.CSPadBkgdSubtract [cspad_mod.CsPadCalib] inputKey = outputKey = calibrated doPedestals = yes doPixelStatus = no doCommonMode = no [ImgAlgos.CSPadBkgdSubtract] source = DetInfo(CxiDs1.0:Cspad.0) inputKey = calibrated outputKey = bkgd_subtracted bkgd_fname = <the-file-name-with-background-array> norm_sector = 0 print_bits = 3
- The file with the background array,
bkgd_fname
, was obtained by averaging 1000 events using module CSPadArrAverage. Subtraction is done with normalization fornorm_sector=0
. - Event image and pixel amplitude spectrum before and after the background subtraction are shown in plots:
- Other event with better subtracted background:
Example for Module ImgAlgos::CSPadMaskApply
- See Module ImgAlgos::CSPadMaskApply
- The array for mask contains zeros and ones for masked and passed pixels, respectively, and has a shape of full-size CSPad array 4*8*185388.
- For example, it can be generated by the command
./MakePixelMask.py <input-background-cspad-arr-file-name> <threshold> <output-file-name>
- for the averaged background amplitude array
<input-background-cspad-arr-file-name>
abtained as a result ofImgAlgos::CSPadArrAverage
module. - Plots show the averaged background, and the mask arrays generated from this background for three thresholds 10, 20, and 30 EDU:
- The best results in filtering can be achieved in combination of modiles:
modules = cspad_mod.CsPadCalib \ ImgAlgos.CSPadBkgdSubtract \ ImgAlgos.CSPadMaskApply \ ... [cspad_mod.CsPadCalib] inputKey = outputKey = calibrated_arr doPedestals = yes doPixelStatus = no doCommonMode = no [ImgAlgos.CSPadBkgdSubtract] source = DetInfo(CxiDs1.0:Cspad.0) inputKey = calibrated_arr outputKey = bkgd_subtracted_arr bkgd_fname = ana-cxi49012/cspad-cxi49012-r0025-background-ave.dat norm_sector = 0 print_bits = 0 [ImgAlgos.CSPadMaskApply] source = DetInfo(CxiDs1.0:Cspad.0) inkey = bkgd_subtracted_arr outkey = masked_arr mask_fname = ana-cxi49012/cspad-cxi49012-r0025-mask-40.dat masked_amp = 0 print_bits = 3 mask_control_bits = 1
- where
cspad_mod.CsPadCalib
- subtracts the pedestals from raw CSPad data,ImgAlgos.CSPadBkgdSubtract
- subtracts the background,ImgAlgos.CSPadMaskApply
- apply the mask.- In the test with images for background represented by the water and solvent rings this filter provides the background suppression factor about 100.
- The background images that still pass this filter have significantly larger intensity with respect to averaged background:
- Input parameter
mask_control_bits
allows to control masking regions of 2x1. For example, if all edges need to be masked, then usemask_control_bits = 15
, which gives image array like: - where red regions/lines of pixels of amplitude=8 are masked.
Example for module ImgAlgos::CSPadArrNoise
- See Module ImgAlgos::CSPadArrNoise
[psana] modules = cspad_mod.CsPadCalib ImgAlgos.CSPadArrNoise files = /reg/d/psdm/cxi/cxi49012/xtc/e158-r0020-s00-c00.xtc \ /reg/d/psdm/cxi/cxi49012/xtc/e158-r0020-s01-c00.xtc \ /reg/d/psdm/cxi/cxi49012/xtc/e158-r0020-s02-c00.xtc \ /reg/d/psdm/cxi/cxi49012/xtc/e158-r0020-s03-c00.xtc \ /reg/d/psdm/cxi/cxi49012/xtc/e158-r0020-s04-c00.xtc \ /reg/d/psdm/cxi/cxi49012/xtc/e158-r0020-s05-c00.xtc #skip-events = 1000 events = 10 [cspad_mod.CsPadCalib] inputKey = outputKey = calibrated doPedestals = yes doPixelStatus = no doCommonMode = no [ImgAlgos.CSPadArrNoise] source = DetInfo(CxiDs1.0:Cspad.0) key = calibrated statusfile = ana-cxi49012/cspad-cxi49012-r0020-noise-status.dat maskfile = ana-cxi49012/cspad-cxi49012-r0200-noise-mask.dat print_bits = 255 rmin = 3 dr = 1 SoNThr = 3 frac_noisy_imgs = 0.15
- Index map in median algorithm for rmin=3, dr=1:
CSPadArrNoise::printMatrixOfIndexesForMedian(): 0 0 0 0 1 0 0 0 0 0 0 1 1 1 1 1 0 0 0 1 0 0 0 0 0 1 0 0 1 0 0 0 0 0 1 0 1 1 0 0 + 0 0 1 1 0 1 0 0 0 0 0 1 0 0 1 0 0 0 0 0 1 0 0 0 1 1 1 1 1 0 0 0 0 0 0 1 0 0 0 0
- Pixel status (fraction of events where
S/N > SoNThr
): - For cspad-cxi49012-r0020 with parameters from confguration file (
frac_noisy_imgs=0.15
) we get, depending on number of events: Nnoisy, Ntotal, Nnoisy/Ntotal pixels =94585 2296960 0.041
for 10 eventsNnoisy, Ntotal, Nnoisy/Ntotal pixels =2112 2296960 0.00092
for 100 events- Pixel mask for noisy pixels with
|S/N| > SoNThr
: Example for Module ImgAlgos::CSPadArrPeakFinder
- See Module ImgAlgos::CSPadArrPeakFinder
[psana] files = \ /reg/d/psdm/cxi/cxi49012/xtc/e158-r0150-s00-c00.xtc \ /reg/d/psdm/cxi/cxi49012/xtc/e158-r0150-s01-c00.xtc \ /reg/d/psdm/cxi/cxi49012/xtc/e158-r0150-s02-c00.xtc \ /reg/d/psdm/cxi/cxi49012/xtc/e158-r0150-s03-c00.xtc \ # /reg/d/psdm/cxi/cxi49012/xtc/e158-r0150-s04-c00.xtc \ suddenly it became unavailable... /reg/d/psdm/cxi/cxi49012/xtc/e158-r0150-s05-c00.xtc #skip-events = 1000 #events = 200 modules = cspad_mod.CsPadCalib \ ImgAlgos.CSPadMaskApply \ ImgAlgos.CSPadArrPeakFinder [cspad_mod.CsPadCalib] inputKey = outputKey = calibrated doPedestals = yes doPixelStatus = no doCommonMode = no [ImgAlgos.CSPadMaskApply] source = DetInfo(CxiDs1.0:Cspad.0) inkey = calibrated outkey = masked_arr mask_fname = ana-cxi49012/cspad-cxi49012-r0150-mask-badregs.dat #mask_fname = ana-cxi49012/cspad-cxi49012-r0150-mask-bkgd.dat #mask_fname = ana-cxi49012/cspad-cxi49012-r0150-mask-rects.dat masked_amp = 8 print_bits = 1 mask_control_bits = 15 [ImgAlgos.CSPadArrPeakFinder] source = DetInfo(CxiDs1.0:Cspad.0) key = masked_arr key_peaks_out = peaks hot_pix_mask_inp_file = ana-cxi49012/cspad-cxi49012-r0150-noise-mask.dat hot_pix_mask_out_file = ana-cxi49012/cspad-cxi49012-r0150-noise-mask-out.dat frac_noisy_evts_file = ana-cxi49012/cspad-cxi49012-r0150-noise-frac.dat evt_file_out = tmp/cspad-ev- rmin = 3 dr = 1 SoNThr = 3 frac_noisy_imgs = 0.1 peak_npix_min = 4 peak_npix_max = 25 peak_amp_tot_thr = 100. event_npeak_min = 10 event_amp_tot_thr = 1000. nevents_mask_update = 100 nevents_mask_accum = 50 selection_mode = SELECTION_ON out_file_bits = 15 print_bits = 512
- Results:
[info:TimeInterval::startTime] Start time: 2012-06-12 15:32:02 [info:ImgAlgos.CSPadArrPeakFinder] N processed events = 1000 N selected = 55 Fraction of selected = 0.055 [info:ImgAlgos.CSPadArrPeakFinder] N processed events = 2000 N selected = 62 Fraction of selected = 0.031 [info:ImgAlgos.CSPadArrPeakFinder] N processed events = 3000 N selected = 81 Fraction of selected = 0.027 [info:ImgAlgos.CSPadArrPeakFinder] N processed events = 4000 N selected = 95 Fraction of selected = 0.02375 [info:ImgAlgos.CSPadArrPeakFinder] N processed events = 5000 N selected = 150 Fraction of selected = 0.03 [info:ImgAlgos.CSPadArrPeakFinder] N processed events = 6000 N selected = 265 Fraction of selected = 0.0441667 [info:ImgAlgos.CSPadArrPeakFinder] N processed events = 7000 N selected = 404 Fraction of selected = 0.0577143 [info:ImgAlgos.CSPadArrPeakFinder] ===== JOB SUMMARY ===== [info:TimeInterval::stopTime] Time to process 7945 events is 3747.48 sec, or 0.471678 sec/event
- Selected events
- ev-007713:
- ev-008944:
Example for module ImgAlgos::CSPadArrPeakAnalysis
- See Module ImgAlgos::CSPadArrPeakAnalysis
- Example of the psana configuration file:
modules = cspad_mod.CsPadCalib \ ImgAlgos.CSPadMaskApply \ ImgAlgos.CSPadArrPeakFinder \ ImgAlgos.CSPadArrPeakAnalysis # ...configuration parameters of other modules... [ImgAlgos.CSPadArrPeakAnalysis] source = DetInfo(CxiDs1.0:Cspad.0) key = peaks print_bits = 7 fname_root = file.root
- After execution in psana the
file.root
containing histogram(s) and ntuple(s) will be produced. Then, auxiliary script in root, running by the commend root -q -f proc.C
- produces the plots with histograms:
Example for TimeStampFilter and XtcOutputModule
- This example demonstrates how to run psana with the time stamp filter and event writer in xtc file.
- Both modules are available in psana library and they need only to be described in the configuration file. For example, the configuration file
tstamp-filter-and-event-writer.cfg
may looks like:
[psana] files = /reg/d/psdm/<INSTRUMENT>/<experiment>/xtc/e158-r0021-s00-c00.xtc \ /reg/d/psdm/<INSTRUMENT>/<experiment>/xtc/e158-r0021-s01-c00.xtc \ /reg/d/psdm/<INSTRUMENT>/<experiment>/xtc/e158-r0021-s02-c00.xtc \ /reg/d/psdm/<INSTRUMENT>/<experiment>/xtc/e158-r0021-s03-c00.xtc \ /reg/d/psdm/<INSTRUMENT>/<experiment>/xtc/e158-r0021-s04-c00.xtc \ /reg/d/psdm/<INSTRUMENT>/<experiment>/xtc/e158-r0021-s05-c00.xtc skip-events = 10 events = 100 modules = ImgAlgos.TimeStampFilter PSXtcOutput.XtcOutputModule [PSXtcOutput.XtcOutputModule] dirName = ./test_out [ImgAlgos.TimeStampFilter] tsinterval = 2012-02-02 18:17:00.409143728 / 2012-02-02 18:17:00.525853474 filterIsOn = true print_bits = 11
- Command to run psana is:
psana -c ./tstamp-filter-and-event-writer.cfg
- For this configuration file psana will skip 10 events and loop over the next 100 events from the
/reg/d/psdm/<INSTRUMENT>/<experiment>/xtc/e158-r0021-s0*-c00.xtc
files and run consecutivelymodules = ImgAlgos.TimeStampFilter PSXtcOutput.XtcOutputModule
. Parameters of these modules are described in the bottom part of the configuration file. ModuleTimeStampFilter
passes events from the specified time interval and prints some useful information. ModuleXtcOutputModule
will write passed events in the file with auto-generated name./test_out/e158-r0021.xtcf
. - See also: Module ImgAlgos::TimeStampFilter and PSXtcOutput::PSXtcOutput
Examples for Package pyimgalgos
- Package pyimgalgos contains python modules which work with both frameworks pyana and psana.
- Configuration file for pyana and/or psana should have relevant sections with parameters for
[pyana]
and/or[psana]
. Alean section is ignored in each framework at run time. This is the only difference between two frameworks in the configuration file. All module descriptions are the same for two frameworks, as shown in examples below. - See description of modules in Package pyimgalgos.
Example of configuration file for CSPAD
- File
py-xcs72913-r0049-cspad.cfg
:
# Run this script: # psana -c py-xcs72913-r0049-cspad.cfg # pyana -c py-xcs72913-r0049-cspad.cfg # # Useful commands: # psana -m EventKeys -n 5 /reg/d/psdm/xcs/xcs72913/xtc/e265-r0049-* # psana -m psana_examples.dump_cspad -n 5 exp=xcs72913:run=49 # pyana -m pyana_examples.dump_cspad -n 5 /reg/d/psdm/xcs/xcs72913/xtc/e265-r0049-* [pyana] files = /reg/d/psdm/xcs/xcs72913/xtc/e265-r0049-s00-c00.xtc /reg/d/psdm/xcs/xcs72913/xtc/e265-r0049-s04-c00.xtc /reg/d/psdm/xcs/xcs72913/xtc/e265-r0049-s05-c00.xtc num-events = 5 #skip-events = 0 #num-cpu = 1 verbose = 1 ; logging output: 0-nothing?, 1+INFO, 2+DEBUG, ... modules = pyimgalgos.tahometer pyimgalgos.cspad_arr_producer pyimgalgos.cspad_image_producer pyimgalgos.image_save_in_file [psana] files = exp=xcs72913:run=49 events = 5 #skip-events = 0 modules = pyimgalgos.tahometer pyimgalgos.cspad_arr_producer pyimgalgos.cspad_image_producer pyimgalgos.image_save_in_file verbose = 1 [pyimgalgos.tahometer] dn = 10 print_bits = 255 [pyimgalgos.cspad_arr_producer] #source = -|Cspad-* source = XcsEndstation-0|Cspad-0 data_type = double #data_type = float #data_type = unsigned #data_type = uint16 val_miss = 0 key_out = cspad_array print_bits = 1 [pyimgalgos.cspad_image_producer] calib_dir = /reg/d/psdm/xcs/xcs72913/calib/CsPad::CalibV1/XcsEndstation.0:Cspad.0/ key_in = cspad_array key_out = cspad_image print_bits = 1 # Supported output file formats tiff, gif, png, eps, jpg, jpeg, txt, npy(default), npz [pyimgalgos.image_save_in_file] key_in = cspad_image ofname = img-for-cspad.txt print_bits = 255
- To run this script use command
psana -c py-xcs72913-r0049-cspad.cfg
- or
pyana -c py-xcs72913-r0049-cspad.cfg
Example of configuration file for CSPAD2x2
- File
py-meca6113-r0028-cspad2x2.cfg
# Run this script: # psana -c py-meca6113-r0028-cspad2x2.cfg # pyana -c py-meca6113-r0028-cspad2x2.cfg # # Useful commands: # psana -m EventKeys -n 5 /reg/d/psdm/mec/meca6113/xtc/e332-r0028-s03-c00.xtc # psana -m psana_examples.dump_cspad -n 5 exp=meca6113:run=28 # pyana -m pyana_examples.dump_cspad -n 5 /reg/d/psdm/mec/meca6113/xtc/e332-r0028-s03-c00.xtc [pyana] files = /reg/d/psdm/mec/meca6113/xtc/e332-r0028-s03-c00.xtc num-events = 5 #skip-events = 0 #num-cpu = 1 verbose = 0 ; logging output: 0-nothing?, 1+INFO, 2+DEBUG, ... modules = pyimgalgos.tahometer pyimgalgos.cspad_arr_producer pyimgalgos.cspad_image_producer pyimgalgos.image_save_in_file [psana] files = exp=meca6113:run=28 events = 5 #skip-events = 0 modules = pyimgalgos.tahometer pyimgalgos.cspad_arr_producer pyimgalgos.cspad_image_producer pyimgalgos.image_save_in_file [pyimgalgos.tahometer] dn = 10 print_bits = 255 [pyimgalgos.cspad_arr_producer] #source = -|Cspad-* source = MecTargetChamber-0|Cspad2x2-3 #data_type = double data_type = float #data_type = unsigned #data_type = uint16 #data_type = uint32 val_miss = 0 key_out = cspad2x2_array print_bits = 255 [pyimgalgos.cspad_image_producer] calib_dir = /reg/d/psdm/mec/meca6113/calib/CsPad2x2::CalibV1/MecTargetChamber.0:Cspad2x2.3/ key_in = cspad2x2_array key_out = cspad2x2_image print_bits = 1 # Supported output file formats tiff, gif, png, eps, jpg, jpeg, txt, npy(default), npz [pyimgalgos.image_save_in_file] key_in = cspad2x2_image ofname = img-for-cspad2x2.tiff print_bits = 255
- To run this script use command
psana -c py-meca6113-r0028-cspad2x2.cfg
- or
pyana -c py-meca6113-r0028-cspad2x2.cfg
References
- Psana Module Catalog