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Scale method changed #83
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import sys | ||||||||||
from pathlib import Path | ||||||||||
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import numpy as np | ||||||||||
from PIL import Image | ||||||||||
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from instamatic.processing.ImgConversionDM import ImgConversionDM as ImgConversion | ||||||||||
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# Script to process cRED data collecting using the DigitalMicrograph script `insteaDMatic` | ||||||||||
# https://github.com/instamatic-dev/instamatic/tree/master/dmscript | ||||||||||
# | ||||||||||
# To use: | ||||||||||
# Run `python process_dm.py cred_log.txt` | ||||||||||
# | ||||||||||
# Where the first argument is the path to the cred_log.txt file. Assumes the data are stored | ||||||||||
# in a subdirectory `tiff/*.tif` from where cred_log.txt is stored. | ||||||||||
# | ||||||||||
# Defaults to `cred_log.txt` in the current directory if left blank. | ||||||||||
# | ||||||||||
# If the first argument is given as `all`, the script will look for | ||||||||||
# all `cred_log.txt` files in the subdirectories, and iterate over those. | ||||||||||
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def relativistic_wavelength(voltage: float = 200): | ||||||||||
"""Calculate the relativistic wavelength of electrons Voltage in kV Return | ||||||||||
wavelength in Angstrom.""" | ||||||||||
voltage *= 1000 # -> V | ||||||||||
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h = 6.626070150e-34 # planck constant J.s | ||||||||||
m = 9.10938356e-31 # electron rest mass kg | ||||||||||
e = 1.6021766208e-19 # elementary charge C | ||||||||||
c = 299792458 # speed of light m/s | ||||||||||
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wl = h / (2 * m * voltage * e * (1 + (e * voltage) / (2 * m * c**2)))**0.5 | ||||||||||
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return round(wl * 1e10, 6) # m -> Angstrom | ||||||||||
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def img_convert(credlog, tiff_path='tiff2', mrc_path='RED', smv_path='SMV'): | ||||||||||
credlog = Path(credlog) | ||||||||||
drc = credlog.parent | ||||||||||
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image_fns = list(drc.glob('tiff/*.tif')) | ||||||||||
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n = len(image_fns) | ||||||||||
if n == 0: | ||||||||||
print(f'No files found matching `tiff/*.tif`') | ||||||||||
exit() | ||||||||||
else: | ||||||||||
print(n) | ||||||||||
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buffer = [] | ||||||||||
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with open(credlog, 'r') as f: | ||||||||||
for line in f: | ||||||||||
if line.startswith('Data Collection Time'): | ||||||||||
timestamp = line.split(':', 1)[-1].strip() | ||||||||||
if line.startswith('Camera length (mm):'): | ||||||||||
camera_length = float(line.split()[-1]) | ||||||||||
if line.startswith('Oscillation angle'): | ||||||||||
osc_angle = float(line.split()[-1]) | ||||||||||
if line.startswith('High tension (kV):'): | ||||||||||
high_tension = float(line.split()[-1]) | ||||||||||
if line.startswith('Starting angle'): | ||||||||||
start_angle = float(line.split()[-1]) | ||||||||||
if line.startswith('Ending angle'): | ||||||||||
end_angle = float(line.split()[-1]) | ||||||||||
if line.startswith('Rotation axis'): | ||||||||||
rotation_axis = float(line.split()[-1]) | ||||||||||
if line.startswith('Acquisition time'): | ||||||||||
acquisition_time = float(line.split()[-1]) | ||||||||||
if line.startswith('Exposure Time'): | ||||||||||
exposure_time = float(line.split()[-1]) | ||||||||||
if line.startswith('Image pixelsize x/y (1/nm):'): | ||||||||||
inp = line.split() | ||||||||||
pixelsize = (float(inp[-2]), float(inp[-1])) | ||||||||||
if line.startswith('Image physical pixelsize x/y (um):'): | ||||||||||
inp = line.split() | ||||||||||
physical_pixelsize = (float(inp[-2]), float(inp[-1])) | ||||||||||
if line.startswith('Binsize:'): | ||||||||||
binsize = float(line.split()[-1]) | ||||||||||
if line.startswith('Image resolution x/y (px):'): | ||||||||||
inp = line.split() | ||||||||||
resolution = (int(inp[-2]), int(inp[-1])) | ||||||||||
if line.startswith('Camera:'): | ||||||||||
camera = line.split()[-1] | ||||||||||
if line.startswith('Resolution:'): | ||||||||||
resolution = line.split()[-1] | ||||||||||
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wavelength = relativistic_wavelength(high_tension) | ||||||||||
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# convert from um to mm | ||||||||||
physical_pixelsize = physical_pixelsize[0] / 1000 | ||||||||||
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# convert from 1/nm to 1/angstrom | ||||||||||
pixelsize = pixelsize[0] / 10 | ||||||||||
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# rotation axis | ||||||||||
# for themisZ/Oneview: -171.0; for 2100LaB6/Orius: 53.0; otherwise: 0.0 | ||||||||||
rotation_axis = np.radians(rotation_axis) | ||||||||||
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print('timestamp:', timestamp) | ||||||||||
print('Wavelength:', wavelength) | ||||||||||
print('Camera:', camera) | ||||||||||
print('Resolution (px):', resolution) | ||||||||||
print('TEM Camera length (mm):', camera_length) | ||||||||||
print('Pixelsize (1/Angstrom):', pixelsize) | ||||||||||
print('Physical pixelsize (um):', physical_pixelsize) | ||||||||||
print('Starting angle (deg.):', start_angle) | ||||||||||
print('Ending angle (deg.):', end_angle) | ||||||||||
print('Oscillation angle (deg./frame):', osc_angle) | ||||||||||
print('Acquisition time (s/frame):', acquisition_time) | ||||||||||
print('Rotation axis (rad.):', rotation_axis) | ||||||||||
# print("Binsize:", binsize) | ||||||||||
max_points = 0 | ||||||||||
for i, fn in enumerate(image_fns): | ||||||||||
img = np.array(Image.open(fn)) | ||||||||||
max_row = np.argmax(img) // img.shape[1] | ||||||||||
max_col = np.argmax(img) % img.shape[1] | ||||||||||
for k in range(20): | ||||||||||
for l in range(20): | ||||||||||
img[max_row - k + 10][max_col - l + 10] = 1 | ||||||||||
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Suggested change
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max_point = img.max() | ||||||||||
if max_point > max_points: | ||||||||||
max_points = max_point | ||||||||||
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for i, fn in enumerate(image_fns): | ||||||||||
img = np.array(Image.open(fn)) | ||||||||||
if img.dtype != np.uint16: | ||||||||||
# cast to 16 bit uint16 | ||||||||||
img = ((img) / (max_points)) * (2 ** 16 - 1) | ||||||||||
img = np.clip(img, 0, 2 ** 16 - 1) | ||||||||||
h = {'ImageGetTime': timestamp, 'ImageExposureTime': exposure_time} | ||||||||||
buffer.append((i, img, h)) | ||||||||||
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img_conv = ImgConversion(buffer=buffer, | ||||||||||
osc_angle=osc_angle, | ||||||||||
start_angle=start_angle, | ||||||||||
end_angle=end_angle, | ||||||||||
rotation_axis=rotation_axis, | ||||||||||
acquisition_time=acquisition_time, | ||||||||||
flatfield=None, | ||||||||||
pixelsize=pixelsize, | ||||||||||
physical_pixelsize=physical_pixelsize, | ||||||||||
wavelength=wavelength) | ||||||||||
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if mrc_path: | ||||||||||
mrc_path = drc / mrc_path | ||||||||||
if smv_path: | ||||||||||
smv_path = drc / smv_path | ||||||||||
if tiff_path: | ||||||||||
tiff_drc_name = tiff_path | ||||||||||
tiff_path = drc / tiff_path | ||||||||||
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img_conv.threadpoolwriter(tiff_path=tiff_path, | ||||||||||
mrc_path=mrc_path, | ||||||||||
smv_path=smv_path, | ||||||||||
workers=8) | ||||||||||
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if mrc_path: | ||||||||||
img_conv.write_ed3d(mrc_path) | ||||||||||
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if smv_path: | ||||||||||
img_conv.write_xds_inp(smv_path) | ||||||||||
# img_conv.to_dials(smv_path) | ||||||||||
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img_conv.write_pets_inp(path=drc, tiff_path=tiff_drc_name) | ||||||||||
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def main(): | ||||||||||
try: | ||||||||||
credlog = sys.argv[1] | ||||||||||
except IndexError: | ||||||||||
credlog = 'cRED_log.txt' | ||||||||||
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if credlog == 'all': | ||||||||||
fns = Path('.').glob('**/cRED_log.txt') | ||||||||||
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for fn in fns: | ||||||||||
print(fn) | ||||||||||
img_convert(fn) | ||||||||||
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else: | ||||||||||
img_convert(credlog) | ||||||||||
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if __name__ == '__main__': | ||||||||||
main() |
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