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scienceopen committed Aug 18, 2016
1 parent ca70c6e commit dd296e5
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Showing 2 changed files with 101 additions and 101 deletions.
64 changes: 32 additions & 32 deletions Demo_localBinaryPattern.py
@@ -1,32 +1,32 @@
#!/usr/bin/env python
"""
read an AVI and do LBP on it
"""
from pyimagevideo import Path
import cv2 #used to read AVI and for high-speed display
from skimage.feature import local_binary_pattern
#
#from cvutils.getaviprop import getaviprop

def demoLBP(fn):
fn = Path(fn).expanduser()
vid = cv2.VideoCapture(str(fn))
# vidparam = getaviprop(vid)

while True:
ret,img = vid.read()
if not ret:
break
if img.ndim==3:
img = cv2.cvtColor(img, cv2.COLOR_BGR2GRAY)
lbp = local_binary_pattern(img,8,3,'default')
cv2.imshow('lbp',lbp)
cv2.waitKey(delay=1)

if __name__ == '__main__':
from argparse import ArgumentParser
p= ArgumentParser(description='load avi and demo LBP alg.')
p.add_argument('avifn',help='.avi file to process')
p = p.parse_args()

demoLBP(p.avifn)
#!/usr/bin/env python
"""
read an AVI and do LBP on it
"""
from pyimagevideo import Path
import cv2 #used to read AVI and for high-speed display
from skimage.feature import local_binary_pattern
#
#from cvutils.getaviprop import getaviprop

def demoLBP(fn):
fn = Path(fn).expanduser()
vid = cv2.VideoCapture(str(fn))
# vidparam = getaviprop(vid)

while True:
ret,img = vid.read()
if not ret:
break
if img.ndim==3:
img = cv2.cvtColor(img, cv2.COLOR_BGR2GRAY)
lbp = local_binary_pattern(img,8,3,'default')
cv2.imshow('lbp',lbp)
cv2.waitKey(delay=1)

if __name__ == '__main__':
from argparse import ArgumentParser
p= ArgumentParser(description='load avi and demo LBP alg.')
p.add_argument('avifn',help='.avi file to process')
p = p.parse_args()

demoLBP(p.avifn)
138 changes: 69 additions & 69 deletions wavelength2rgb.py
@@ -1,69 +1,69 @@
#!/usr/bin/env python
from __future__ import division

def wavelength_to_rgb(wavelength, gamma=0.8):

'''
noah.org
http://www.noah.org/wiki/Wavelength_to_RGB_in_Python
This converts a given wavelength into an approximate RGB value.
The given wavelength is in nanometers.
The range of wavelength is 380 nm through 750 nm.
Based on code by Dan Bruton
http://www.physics.sfasu.edu/astro/color/spectra.html
'''

wavelength = float(wavelength)
if 440. >= wavelength >= 380.:
attenuation = 0.3 + 0.7 * (wavelength - 380) / (440 - 380)
R = ((-(wavelength - 440) / (440 - 380)) * attenuation) ** gamma
G = 0.
B = (1. * attenuation) ** gamma
elif wavelength >= 440 and wavelength <= 490:
R = 0.0
G = ((wavelength - 440) / (490 - 440)) ** gamma
B = 1.
elif wavelength >= 490 and wavelength <= 510:
R = 0.
G = 1.
B = (-(wavelength - 510) / (510 - 490)) ** gamma
elif wavelength >= 510 and wavelength <= 580:
R = ((wavelength - 510) / (580 - 510)) ** gamma
G = 1.
B = 0.
elif wavelength >= 580 and wavelength <= 645:
R = 1.0
G = (-(wavelength - 645) / (645 - 580)) ** gamma
B = 0.
elif wavelength >= 645 and wavelength <= 750:
attenuation = 0.3 + 0.7 * (750 - wavelength) / (750 - 645)
R = (1.0 * attenuation) ** gamma
G = 0.
B = 0.
else:
R = 0.
G = 0.
B = 0.

R = int(R*255)
G = int(G*255)
B = int(B*255)

assert 255>=R>=0 and 255>=G>=0 and 255>=B>=0

return R,G,B

if __name__ == '__main__':
from argparse import ArgumentParser
p = ArgumentParser()
p.add_argument('wavelength_nm',help='wavelength in nm',type=float)
p.add_argument('--gamma',type=float,default=0.8)
p = p.parse_args()

R,G,B = wavelength_to_rgb(p.wavelength_nm,p.gamma)

print(R)
print(G)
print(B)
#!/usr/bin/env python
from __future__ import division

def wavelength_to_rgb(wavelength, gamma=0.8):

'''
noah.org
http://www.noah.org/wiki/Wavelength_to_RGB_in_Python
This converts a given wavelength into an approximate RGB value.
The given wavelength is in nanometers.
The range of wavelength is 380 nm through 750 nm.
Based on code by Dan Bruton
http://www.physics.sfasu.edu/astro/color/spectra.html
'''

wavelength = float(wavelength)
if 440. >= wavelength >= 380.:
attenuation = 0.3 + 0.7 * (wavelength - 380) / (440 - 380)
R = ((-(wavelength - 440) / (440 - 380)) * attenuation) ** gamma
G = 0.
B = (1. * attenuation) ** gamma
elif wavelength >= 440 and wavelength <= 490:
R = 0.0
G = ((wavelength - 440) / (490 - 440)) ** gamma
B = 1.
elif wavelength >= 490 and wavelength <= 510:
R = 0.
G = 1.
B = (-(wavelength - 510) / (510 - 490)) ** gamma
elif wavelength >= 510 and wavelength <= 580:
R = ((wavelength - 510) / (580 - 510)) ** gamma
G = 1.
B = 0.
elif wavelength >= 580 and wavelength <= 645:
R = 1.0
G = (-(wavelength - 645) / (645 - 580)) ** gamma
B = 0.
elif wavelength >= 645 and wavelength <= 750:
attenuation = 0.3 + 0.7 * (750 - wavelength) / (750 - 645)
R = (1.0 * attenuation) ** gamma
G = 0.
B = 0.
else:
R = 0.
G = 0.
B = 0.

R = int(R*255)
G = int(G*255)
B = int(B*255)

assert 255>=R>=0 and 255>=G>=0 and 255>=B>=0

return R,G,B

if __name__ == '__main__':
from argparse import ArgumentParser
p = ArgumentParser()
p.add_argument('wavelength_nm',help='wavelength in nm',type=float)
p.add_argument('--gamma',type=float,default=0.8)
p = p.parse_args()

R,G,B = wavelength_to_rgb(p.wavelength_nm,p.gamma)

print(R)
print(G)
print(B)

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