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Auto masking tool (#46)
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* Update center.py

Tool to automatically generate a mask based on the darkest portion of the image. This to skip the manual definition of one and to compensate for possible beam stopper movement (image rotation during acquisition or beam stopper mechanical play).

* formatting, test and documentation

black formatting check, added to the loading by default and updated tutorials section

* improved to avoid hotspot problems, more universal

* Update __init__.py

Black formatting

---------

Co-authored-by: Olivier Donzel-Gargand <[email protected]>
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OliDG and Olivier Donzel-Gargand authored Jun 28, 2024
1 parent a4d438f commit 4c07a35
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36 changes: 36 additions & 0 deletions docs/tutorials/image.rst
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Expand Up @@ -27,7 +27,43 @@ Diffraction patterns can come in a variety of exotic file formats. Scikit-ued ha
* All other file formats supported by `scikit-image`_.

The :func:`diffread` function will transparently distinguish between those formats and dispatch to the right functions.
.. _automatic_mask_generation:

Automatic generation of a mask as needed for the autocenter() function
======================================================================

Automatic mask generation
-------------------------
A mask can be used for the :func: `autocenter` function to exclude the beam stopper from the analysis and only keep valuable
information. Such a mask can automatically be generated using this function; given a diffraction pattern, the mask will be created to block
the darkest regions of the image (default blocks about 10% of the darker values).
Here is an example:

.. plot::

import matplotlib.pyplot as plt
from skued import diffread, auto_masking

image = diffread('data/Cr_1.tif')
mask = auto_masking(image, threshold = 0.1)

# Reduce size of images because of memory usage of ReadTheDocs
image = image[::3, ::3]
mask = mask[::3, ::3]

fig , (ax1, ax2) = plt.subplots(1,2, figsize = (9,3))
ax1.imshow(image, vmin=0, vmax=150, cmap='inferno')
ax2.imshow(mask, vmin=0, vmax=1, cmap='inferno')

for ax in (ax1, ax2):
ax.xaxis.set_visible(False)
ax.yaxis.set_visible(False)

ax1.set_title('Cr_1')
ax2.set_title('Mask')

plt.tight_layout()
plt.show()
.. _alignment:

Automatic center-finding
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1 change: 1 addition & 0 deletions skued/__init__.py
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Expand Up @@ -44,6 +44,7 @@
from .image import (
align,
autocenter,
auto_masking,
azimuthal_average,
brillouin_zones,
combine_masks,
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2 changes: 1 addition & 1 deletion skued/image/__init__.py
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Expand Up @@ -4,7 +4,7 @@
from .alignment import align, ialign, itrack_peak
from .brillouin import brillouin_zones
from .calibration import detector_scattvectors, powder_calq
from .center import autocenter
from .center import autocenter, auto_masking
from .indexing import bragg_peaks, bragg_peaks_persistence
from .metrics import (
combine_masks,
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26 changes: 26 additions & 0 deletions skued/image/center.py
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Expand Up @@ -124,3 +124,29 @@ def _center_of_intensity(im, mask=None):
r_ = np.average(rr, weights=weights)
c_ = np.average(cc, weights=weights)
return int(r_), int(c_)


def auto_masking(im, threshold=0.1):
"""
Generate a mask based on the darkest fraction of an image
Parameters
----------
im : floats, ndarrays of shape (N,M)
image used to generate a mask
threshold: float, optional
fraction of the lowest values to be masked, default = 15%
Yields
------
mask : boolean, ndarrays of shape (N,M)
Mask that evaluates to True on valid pixels.
"""
# Find the median of the highest intensity value of the image to avoid hot spots
max_median = np.median([max(x) for x in np.real(im)])
# Set the threshold value
lower_limit = threshold * max_median
# generate a mask
mask = im >= lower_limit
return mask

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