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 times t with time difference tau 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 [PCDS: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 [PCDS:IDPE for TCE in XCS - Problems and tentative solutions].

GUI Implementation

Updated on 2013-04-01

As an example of GUI style Marcin suggested to use [XPCSGUI|^xpcsgui_screen_shots_edited.pdf] - 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.

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.

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 2013-04-24

All module names beginning with letters GUI implements different Graphical User Interfaces.

Modules used from package ImgAlgos

Updated on 2013-04-24

Status of the project

Updated on 2013-04-24

PSANA modules

For 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.

For 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 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.

For 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.

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 - [PCDS: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.

Comparison of results

Comparison conditions

1. dark run: /reg/d/ana12/xcs/xcsi0112/xtc/e167-r0020-s00-c00.xtc use all 75 events
2. data run: /reg/d/ana12/xcs/xcsi0112/xtc/e167-r0015-s00-c00.xtc use all 500 events
3. do not use any intensity monitor selection or correction
4. do not use any mask including hot pixel, saturation, blemish, ROI, and restriction on the image size.
5. use LLD as a constant ADU threshold = 20
6. use a single q-phi static bin
7. use a single q-phi dynamic bin
8. q value is not an issue for current comparison, so geometry does not matter.

Results from Marcin

Progress

See [PCDS: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

[en.wikipedia.org/wiki/Photon_Correlation_Spectroscopy]