...

img-xcs-r0015-image-result.bin

Wrapping script

./CorAnaSubmit.pyImgAlgos/app/corana_submit

./CorAnaSubmit.py corana_submit [-c <config-file>] [-t <fname-tau>] [-x] <xtc-file-list>

For example:

./CorAnaSubmit.pycorana_submit -c ImgAlgos/data/psana-xcsi0112-r0015-img-auto-correlation.cfg -t my-tau.txt /reg/d/psdm/XCS/xcsi0112/xtc/e167-r0015-s00-c00.xtc 

...

• File with split-image data for selected events img-xcs-r0015-b000N.bin:
  Currently this file contains <uint16_t> amplitude for each pixel in binary format for:

  Code Block
  <data-for-img-partN-of-img1> <data-for-img-partN-of-img2> ... <data-for-img-partN-of-imgLast>

• File with metadata parameters img-xcs-r0015-med.txt:

  Code Block
  IMAGE_ROWS 1300 IMAGE_COLS 1340 IMAGE_SIZE 1742000 NUMBER_OF_FILES 8 BLOCK_SIZE 217750 REST_SIZE 0 NUMBER_OF_IMGS 500 FILE_TYPE bin DATA_TYPE uint16_t TIME_SEC_AVE 8.088413 TIME_SEC_RMS 0.063639 TIME_INDEX_MAX 499

• File with image time records img-xcs-r0015-time.txt:

  Code Block
  1 0.000000 0.000000 20120616-080236.671607864 5366 0 2 8.026429 8.026429 20120616-080244.698036743 8255 1 3 16.144788 8.118359 20120616-080252.816395836 11177 2 4 24.154835 8.010048 20120616-080300.826443448 14060 3 ...

  where each record has:

  Code Block
  <image-in-file#> <t(sec)-from-the-1st-event> <dt(sec)> <time-stamp> <fiducials> <event#-since-configure>

• File with image time records and evaluated time index img-xcs-r0015-time-ind.txt:

  Code Block
  1 0.000000 0.000000 20120616-080236.671607864 5366 0 0 2 8.026429 8.026429 20120616-080244.698036743 8255 1 1 3 16.144788 8.118359 20120616-080252.816395836 11177 2 2 4 24.154835 8.010048 20120616-080300.826443448 14060 3 3 5 32.281937 8.127102 20120616-080308.953545010 16985 4 4 ...

  where each record has:

  Code Block
  <image-in-file#> <t(sec)-from-the-1st-event> <dt(sec)> <time-stamp> <fiducials> <event#-since-configure> <time-index-starting-from-0>

• File with split-image correlators for each value of tau img-xcs-r0015-b000N-result.bin:
  Currently it saves <float> correlator for each pixel in binary format for:

  Code Block
  <corr-for-img-partN-of-tau1> <corr-for-img-partN-of-tau2> ... <corr-for-img-partN-of-tauLast>

• my-tau.txt:

  Code Block
  1 3 5 7 9 10 12 14 16 18 20 24 28 30 32 36 40 ... 160 180 200 240 280 300 320 360 400

  contains the tau values presented in terms of number of ordered images in the file.

Quick start guide

We assume that everything is set up to work on LCLS analysis farm, otherwise see Computing and Account Setup.

How to run this procedure

If the version of the package ImgAlgos is already current software release, then you may run the script command(s) directly, for example:

cd <your-favorite-directory>
mkdir work_corana
sit_setup
corana_submit [-c <config-file>] [-t <fname-tau>] [-x] <xtc-file-list>

cd <your-favorite-directory>
newrel ana-current myReleaseDirectory
cd myReleaseDirectory
sit_setup
addpkg ImgAlgos HEAD
scons

Where to find results

The procedure will produce a bunch of files in the work_corana directory. The most important files are