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Only listed segments are highlighted on plots:

 

Background

Averaged background shape

 

Background shape evaluated in exp=cxif5315:run=162 with common mode correction - central segments got offset to higher intensity

 

Image Added

Background shape evaluated evaluated in exp=cxif5315:run=162 without common mode correction - common mode offsets averaged out to zero and image represents true background shape.

Command to average data with options for processing algorithms:

Code Block
det_ndarr_average -d exp=cxif5315:run=162 -s CxiDs2.0:Cspad.0 -n 10000 -m 5000 -a 3 -f nda-bkgd -p -v

skips 5000 and averages next 10000 events.

Deployed as: /reg/d/psdm/cxi/cxif5315/calib/CsPad::CalibV1/CxiDs2.0:Cspad.0/pixel_bkgd/95-end.data

 

Image AddedImage Added

 

Radial background subtraction

For some reason polarization correction does not work well in this experiment for entire image.

Comparison of the 2-d interpolated radial background subtraction 

  • nbins (rad:500, phi:1)

Image RemovedImage Removed

  • nbins (rad:500, phi:32)

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polarization correction factor map orientation should be consistent with geometry file - in cxif5315 it should be rotated by 90°.

Code Block
from pyimgalgos.RadialBkgd import RadialBkgd, polarization_factor

    X, Y, Z = geo.get_pixel_coords()
    rb = RadialBkgd(X, Y, mask, nradbins=500, nphibins=1) 
    pf = polarization_factor(rb.pixel_rad(), rb.pixel_phi()+90, 91.33e3)

# in event loop:
    nda, title = rb.subtract_bkgd_interpol(arr * pf) * mask

For example we apply this algorithm to the water background averaged sample from exp=cxif5315:run=162:

Image AddedImage Added

Radial background fails to work in the region of shadow, where image miss symmetry. This region can be removed by constraining the range of angles phiedges=(40, 325).

In the next plot the radial range is also constrained as radedges=(5000,100000) for the purpose of example:

Code Block
# the same as in previous case, but
rb = RadialBkgd(X, Y, mask, nradbins=500, nphibins=1, phiedges=(40, 325), radedges=(5000,100000))

Image AddedImage Added

SIngle angular bin still works fine in our ROI defined by both masks.

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Subtract background shape evaluated in run 192

Code Block
    from pyimgalgos.GlobalUtils import subtract_bkgd
		# once per run:
        nda_peds  = det.pedestals(runnum)
        nda_bkgd  = det.bkgd(runnum)      # get n-d array with averaged background from calib/.../pixel_bkgd
        nda_smask = det.mask(evt, calib=False, status=True, edges=True, central=True, unbond=True, unbondnbrs=True)

        # windows for background normalization
        winds_bkgd = [(s, 10, 100, 270, 370) for s in (4,12,20,28)] # use part of segments 4,12,20,28 to subtr bkg

        # in the event loop
        nda_raw = det.raw(evt)
        if nda_raw is not None :
            nda =  np.array(nda_raw, dtype=np.float32, copy=True)
            nda -= nda_peds
 
            # Subtract background shape averaged for pure water
            nda = subtract_bkgd(nda, nda_bkgd, mask=nda_smask, winds=winds_bkgd)

Radial background subtraction

Image corrected up to 80mm, 40<phi< 320:rings span for entire phi

Image ModifiedImage Modified

 

Image corrected up to 80mm, rings span for entire phi40<phi< 320:

Image ModifiedImage Modified 

OLD IMAGE PROCESSING

Subtract background shape evaluated in run 192. 

Note

Background shape was evaluated WITH common mode correction. Central ; central 2x1s got offset due to non-uniform water background shape.

Averaged Fraser- transformed image using angles from fit to 2 arc peaks


Spectrum of intensities


Spectrum of intensities of all quad 2x1-segment 0 (close to beam) and 4 (water ring region)

before background subtraction

Image AddedImage Added

after background subtraction

Image AddedImage Added

  • masked pixels contributes to peak at 0
  • 1-, 2- and 3- photon peaks are seen
  • common mode correction before background subtraction does not work well in this data sample due to significant fraction of 1-photon peak next to noise peak, which makes an offset due to illumination.
  • common mode correction after background subtraction does not work - it moves noise peak to 0 and destroys background subtraction results.

Note

Potentially any non-dark data spectra can be used to calibrate pixel gain.

References