xenial (1) pyFAI-recalib.1.gz

Provided by: pyfai_0.11.0+dfsg-3build1_all bug

NAME

       pyFAI-recalib - Deprecated

DESCRIPTION

       usage: pyFAI-recalib [options] -i ponifile -w 1 -c calibrant.D imagefile.edf

       Calibrate  the  diffraction setup geometry based on Debye-Sherrer rings images with a priori knowledge of
       your setup (an input PONI-file). You will need to provide a calibrant or a  "d-spacing"  file  containing
       the  spacing  of  Miller  plans  in Angstrom (in decreasing order). Calibrants available: Ni, CrOx, NaCl,
       Si_SRM640e,  Si_SRM640d,  Si_SRM640a,  Si_SRM640c,  Si_SRM640b,  Cr2O3,  AgBh,  Si_SRM640,   CuO,   PBBA,
       alpha_Al2O3,  quartz,  C14H30O,  cristobaltite, Si, LaB6, CeO2, LaB6_SRM660a, LaB6_SRM660b, LaB6_SRM660c,
       TiO2,    ZnO,     Al,     Au     or     search     in     the     American     Mineralogist     database:
       http://rruff.geo.arizona.edu/AMS/amcsd.php The --calibrant option is mandatory !

   positional arguments:
       FILE   List of files to calibrate

   optional arguments:
       -h, --help
              show this help message and exit

       -V, --version
              show program's version number and exit

       -o FILE, --out FILE
              Filename where processed image is saved

       -v, --verbose
              switch to debug/verbose mode

       -c FILE, --calibrant FILE
              Calibrant name or file containing d-spacing of the reference sample (MANDATORY, case sensitive !)

       -w WAVELENGTH, --wavelength WAVELENGTH
              wavelength of the X-Ray beam in Angstrom. Mandatory

       -e ENERGY, --energy ENERGY
              energy of the X-Ray beam in keV (hc=12.398419292keV.A).

       -P POLARIZATION_FACTOR, --polarization POLARIZATION_FACTOR
              polarization  factor,  from  -1  (vertical)  to  +1 (horizontal), default is None (no correction),
              synchrotrons are around 0.95

       -i FILE, --poni FILE
              file containing the diffraction parameter (poni-file).  MANDATORY for pyFAI-recalib!

       -b BACKGROUND, --background BACKGROUND
              Automatic background subtraction if no value are provided

       -d DARK, --dark DARK
              list of comma separated dark images to average and subtract

       -f FLAT, --flat FLAT
              list of comma separated flat images to average and divide

       -s SPLINE, --spline SPLINE
              spline file describing the detector distortion

       -D DETECTOR_NAME, --detector DETECTOR_NAME
              Detector name (instead of pixel size+spline)

       -m MASK, --mask MASK
              file containing the mask (for image reconstruction)

       -n NPT, --pt NPT
              file with datapoints saved. Default: basename.npt

       --filter FILTER
              select the filter, either mean(default), max or median

       -l DISTANCE, --distance DISTANCE
              sample-detector distance in millimeter. Default: 100mm

       --dist DIST
              sample-detector distance in meter. Default: 0.1m

       --poni1 PONI1
              poni1 coordinate in meter. Default: center of detector

       --poni2 PONI2
              poni2 coordinate in meter. Default: center of detector

       --rot1 ROT1
              rot1 in radians. default: 0

       --rot2 ROT2
              rot2 in radians. default: 0

       --rot3 ROT3
              rot3 in radians. default: 0

       --fix-dist
              fix the distance parameter

       --free-dist
              free the distance parameter. Default: Activated

       --fix-poni1
              fix the poni1 parameter

       --free-poni1
              free the poni1 parameter. Default: Activated

       --fix-poni2
              fix the poni2 parameter

       --free-poni2
              free the poni2 parameter. Default: Activated

       --fix-rot1
              fix the rot1 parameter

       --free-rot1
              free the rot1 parameter. Default: Activated

       --fix-rot2
              fix the rot2 parameter

       --free-rot2
              free the rot2 parameter. Default: Activated

       --fix-rot3
              fix the rot3 parameter

       --free-rot3
              free the rot3 parameter. Default: Activated

       --fix-wavelength
              fix the wavelength parameter. Default: Activated

       --free-wavelength
              free the wavelength parameter. Default: Deactivated

       --tilt Allow initially detector tilt to be refined (rot1, rot2, rot3). Default: Activated

       --no-tilt
              Deactivated tilt refinement and set all rotation to 0

       --saturation SATURATION
              consider all pixel>max*(1-saturation) as saturated and reconstruct them, default: 0 (deactivated)

       --weighted
              weight fit by intensity, by default not.

       --npt NPT_1D
              Number of point in 1D integrated pattern, Default: 1024

       --npt-azim NPT_2D_AZIM
              Number of azimuthal sectors in 2D integrated images.  Default: 360

       --npt-rad NPT_2D_RAD
              Number of radial bins in 2D integrated images.  Default: 400

       --unit UNIT
              Valid units for radial range: 2th_deg, 2th_rad, q_nm^-1, q_A^-1, r_mm. Default: 2th_deg

       --no-gui
              force the program to run without a Graphical interface

       --no-interactive
              force the program to run and exit without prompting for refinements

       -r MAX_RINGS, --ring MAX_RINGS
              maximum number of rings to extract. Default: all accessible

       -k, --keep
              Keep existing control point and append new

       The main difference with pyFAI-calib is the way control-point hence  DebyeSherrer  rings  are  extracted.
       While  pyFAI-calib  relies  on  the  contiguity  of  a region of peaks called massif; pyFAI-recalib knows
       approximatly the geometry and is able to select the region where the ring should be. From this region  it
       selects automatically the various peaks; making pyFAI-recalib able to run without graphical interface and
       without human intervention (--no-gui and --nointeractive options). Note that `pyFAI-recalib`  program  is
       obsolete  as the same functionnality is available from within pyFAI-calib, using the `recalib` command in
       the refinement process. Two option are available for recalib: the numbe of rings to extract  (similar  to
       the  -r  option  of  this  program)  and a new option which lets you choose between the original `massif`
       algorithm and newer ones like `blob` and `watershed` detection.