Motivation
Development of this application was stimulated by the discussion with Marcin Sikorski (meeting on 2012-08-30), doing xcs experiments.
Users need in real-time algorithm for calculation of image vs time auto-correlation function
g2(tau) = <I(t)*I(t+tau)> / (<I(t)> * <I(t+tau)>),
where I(t)
is an image intensity at time t
, and tau
is a delay between two measurements.
Typical experimental condition can be described as follows:
- Run duration is about one hour at frequency up to 120 Hz that gives up to 10^5-10^6 images.
- Currently typical imaging devise is a Princeton camera with 1300x1340 pixels.
- Need to calculate
g2(tau)
for each pixel, averaged over all possible image timest
with time differencetau
between images. - A set of
tau
should have about 30-100 points in log scale uniformly covering the run duration. - Use for example xcsi0112-r0015: 500 images with 8 sec delay between images.
Desired time for evaluation of the auto-correlation function should be comparable with run duration <1 hour. Currently this algorithm takes a few hours that can not be used for fast feedback in real time experiment.
In first approximation this problem was solved, as it is described in the Command Line Interface For Time Correlation Analysis. However, in order to be useful, the command line algorithm needs to be integrated in the global analysis system, which de bene esse called as Integrated Analysis Environment for Time Correlation Experiments and is discussed in IDPE for TCE in XCS - Problems and tentative solutions.
Here is my comment
GUI Implementation
Updated on 2013-04-01
As an example of GUI style Marcin suggested to use XPCSGUI - earlier implementation of similar application.
Three versions of GUI were implemented for this application. It was decided to use the GUIMainTB
layout, where:
- All input windows are integrated in one with tab-bar for switching and custom tool bar on the top
- Logger and File Browser windows are isolated
- All plots are isolated, although similar plots appear in the same windows.
h3 Plots for intensity in q-static bins
Intensity monitors
FEEGasDetEnergy, XCS-IPM-02, XCS-IPM-mono, XcsBeamline.1:Ipimb.4, and XcsBeamline.1:Ipimb.5
Reflective scattering geometry
Source code from Marcin: q_functions.txt
Code location
Everything resides in CorAna
package, which is included in LCLS offline releases beginning from ana-0.7.16
.
References to the specific algorithms can be found in Algorithms for Time Correlation Experiments.
Original data processing code from Marcin is described in Note on XCS code from Marcin.
Modules
In tables below we list modules from packages CorAna
and ImgAlgos
, which were developed for this project.
Notations:
- is done (at least it is assumed for now...)
- needs more work
- test or deprecated modules
Package CorAna
Updated on 2013-10-14
All module names beginning with letters GUI
implements different Graphical User Interfaces.
List of modules in alphabetic order:
Module |
Description |
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Local version with added path to data from src directory. |
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Suprclass for other |
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Class contains methods for batch job submission and monitoring for pedestals. |
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Class has methods to generate psana configuration and other scripts from stubs located in |
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Base class for configuration parameters. |
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Sub-class for |
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Junk for eamples. |
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Class dynamically generates all file names for current configuration parameters. |
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Sub-GUI of GUIFiles.py |
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GUI for the configuration parameters file management. |
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Sub-GUI of GUIFiles.py - manipulations with dark runs |
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Dialog window for submission of messages with attachments to ELog using response ID and Igor's new interface: Python module for posting message into ELog |
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Widget with necessary fields for GUIELogPostingDialog |
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Text file browser for this project |
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Central GUI for file settings contains tab-bar for other widget selection |
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Sub-GUI of GUIFiles.py |
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WIdget for messages, i.e. help |
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depricated GUI |
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Control GUI for intensity monitors |
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GUI manipulation with list of tau indexes |
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GUI for logger |
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The first GUI at start of this application |
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The same as GUIMainTB.py with integrated GUILogger.py |
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The first GUI at start of this application with tab bar |
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Module contains all possible global methods. |
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Re-implemented standard tool-bar (depricated) |
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Core class for logger |
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Demonstration of how to draw something on the top of GUI |
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Main class for array presentation plot |
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Widget for custom button-bar |
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Widget for graphical window |
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Main class for interactive plot with custom button bar |
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Widget for custom button-bar |
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Graphical image for image and spectral histogram |
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Main class for time record presentation plot |
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Widget for graphical window |
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Stub-scripts for ConfigFileGenerator.py |
Modules used from package ImgAlgos
Updated on 2013-10-14
List of modules in alphabetic order:
Module |
Description |
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Superclass for all CorAna* modules |
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Processing of split images, evaluation of correlators |
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Input parameters parser |
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Merges split files with correlatros in a single file |
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Holds common parameters |
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Example of stand-alone processing of the file with correlators |
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Command-line submission procedure for processing |
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Common global methods for |
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Generic |
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Generic |
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Generic |
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Generic |
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Generic |
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Generic |
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Generic |
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Generic |
Functional description
Updated on 2013-10-14
In this section modules are listed in functional order.
PSANA modules
Dark run pre-processing
Scaner
Runs in batch for the dark file to get preliminary information.
ImgAlgos.ImgTimeStampList
- counts number of events in the file
- makes file with time stamps
- evaluate time intervals between frames (for dark run)
Pedestals
Runs in batch for the dark file to get averaged pedestals.
ImgAlgos.PrincetonImageProducer
gets image from event as an ndarray
object
ImgAlgos.Tahometer
evaluates performance of the batch job
ImgAlgos.ImgAverage
produces files with averaged, rms-spread, and hot-pixel mask for images in a given range of events.
Data pre-processing
Scaner
Runs in batch for the data file to get preliminary information.
ImgAlgos.Tahometer
evaluates performance of the batch job, counts number of events in the data file
ImgAlgos.ImgTimeStampList
makes file with time stamps and time record counters for tau
ImgAlgos.IntensityMonitorsData
makes file with intensity monitor records
Average
Runs in batch for the data file to get averaged image
ImgAlgos.Tahometer
evaluates performance of the batch job
ImgAlgos.PrincetonImageProducer
gets image from event as an ndarray
object
ImgAlgos.ImgAverage
produces file with averaged and rms-spread for raw images in a given range of events
ImgAlgos::ImgMaskEvaluation
- module is configured to evaluate masks:
- saturated mask - pixel is considered as saturated if its amplitude exceeds the threshold at least once per run
- noise mask - pixel is considered as noisy if its amplitude exceeds the MEAN+5*RMS in 5% of events. The "noise" MEAN and RMS are evaluated for 8 (or less on the boarder) surrounding pixels. This mask is not used in current analysis.
Data processing
Split
ImgAlgos.Tahometer
for performance evaluation.
ImgAlgos.PrincetonImageProducer
ImgAlgos::ImgCalib
module is configured to:
- subtract pedestals obtained for dark run
- account for threshold (LLD) constant or in number of RMS
ImgAlgos.ImgIntMonCorr
image normalization on intensity monitors data
ImgAlgos.ImgVsTimeSplitInFiles
split image and save blocks for all events in separate files.
ImgAlgos.ImgIntForBins
evaluate intensity (averaged over bin pixels) in bins per event, bin numbers are defined by the map, results are saved in the file.
ImgAlgos.ImgAverage
produces file with averaged and rms-spread for images with subtracted pedestals and allied LLD in a given range of events
Process
Data processing is implemented in stand alone (non-psana) modules
ImgAlgos.CorAna.cpp
ImgAlgos.CorAnaInputParameters.cpp
ImgAlgos.CorAnaData.cpp
Merge
ImgAlgos.CorAna.cpp
ImgAlgos.CorAnaInputParameters.cpp
CorAnaMergeFiles.cpp
- saves binary file for float(32) with shape (Ntau,3,rows,cols), where 3 stands for <Ip>, <If>, and <Ip*If>
Can be acessed in python as
sp.cor_arr = np.fromfile(sp.fname, dtype=np.float32) <image-size> = rows * cols nptau = <file-size>/<image-size>/3 sp.cor_arr.shape = (nptau, 3, rows, cols)
GUI
The system of GUIs, consisting of dozens of CorAna.GUI...
modules is implemented in the draft approximation. Roughly it reproduces all features of the old program.
Input parameters GUIs
CorAna.GUI...
most of them are available. Will be added or extended if necessary.
Files - define input files and do pre-processing
Setup Info
Analysis Info
System
Intensity Monitor
Run GUI
Input - short summary of input info for data processing
Split - control and monitoring for the 1st stage of processing
Process - ... 2nd stage ...
Merge - ... 3d stage ...
Auto - ... for all 3 stages ...
View Results GUI
Contains a set of control fields for presentation of results
Direct and reflected beam geometry is implemented in
ViewResults.py
. Currently the switch between the direct and reflected beam geometry is used from tab status variable: cp.exp_setup_geom.value()
.
If the PV variable will be used, then the switch should be changed in
ViewResults.get_q_map(sp)
module.
Graphics
PlotArray*.py
- for intensity monitors
PlotImgSpe*.py
- for images, partition maps, masks etc.
PlotTime*.py
- for time stamp monitoring
PlotG2*.py
- G2 plot
PlotGraph*.py
- I(q) and I(q,t) plot
MaskEditor*.py
, Drag*.py
- Mask Editor for
- region of interest (ROI-mask)
- blemish mask
ViewResults.pyQ
- all evaluations for resulting array of correlators - maps for pixel x,y coordinates, r, phi
- q maps for transmission and reflective geometry
- etc.
Infrastructural modules
Infrastructural modules provide basic infrastructure of the project.
ConfigParameters.py
, ConfigParametersCorAna.py
, and GUIConfigParameters.py
provides convenient approach for maintenance of all configuration parameters.
Infrastructural modules
Logger.py
and GUILogger.py
provides a generic approach to logging system.
Module
ConfigFileGenerator.py
use current settings of configuration parameters and stub-file scripts from CorAna/data/scripts/
and generates the psana configuration files.
Module
FileNameManager.py
is a single place which provides a dynamic file names for current version of the configuration parameters.
GlobalUtils.py
- global utilities for common operations.
BatchJob.py
- superclass for batch job submission.
BatchJobPedestals.py
- pre-processing for dark run files.
BatchJobData.py
- re-processing for data files.
BatchJobCorAna.py
- main data processing - calculation algorithm.
RecordsFromFiles.py
- class helps to access data in files.
Status of the project
- This project is in the stage of comparison of results between old Marcin's scripts and this application.
Comparison of results
Conditions
- dark run:
/reg/d/ana12/xcs/xcsi0112/xtc/e167-r0020-s00-c00.xtc
use all 75 events - data run:
/reg/d/ana12/xcs/xcsi0112/xtc/e167-r0015-s00-c00.xtc
use all 500 events - do not use any intensity monitor selection or correction
- do not use any mask including hot pixel, saturation, blemish, ROI, and restriction on the image size.
- use LLD as a constant ADU threshold = 20
- use a single q-phi static bin
- use a single q-phi dynamic bin
- q value is not an issue for current comparison, so geometry does not matter.
Compare g2 at 14 tau values with indexes:
1 2 3 4 5 6 7 8 9 10 12 14 16 20
See Progress section for more details on comparison.
Progress
Weekly progress of the IDPE project for TCE
To-do list
Processing (at psana Split level)
Get
cp.photon_energy
, cp.nominal_angle
and other PV variables from data scan and setup confiruration
Comparison of results
- Search for the reason of difference in results for single-q-bin g2.
View Results
more plots for results
g2(tau) for q-dynamic
Average intensity and Intensity(q-static)
Intensity(q-static, t)
Histogram for intensity monitor
Fit results for function g2(tau|pars) = C*exp[-(2t/tau0)**beta] + B
- plot for all fits with beta=1 and float,
- tau0 vs q-dynamic
- C vs q-dynamic
- B vs q-dynamic
- beta vs q-dynamic
References
Photon Correlation Spectroscopy, article in wikipedia
Algorithms for Time Correlation Experiments
Note on XCS code from Marcin