Port dft.py sample from cv to cv2

pull/723/head
Dustin Spicuzza 12 years ago
parent e143706ef9
commit b08432cfe7
  1. 100
      samples/python2/dft.py

@ -0,0 +1,100 @@
#/usr/bin/env python
import cv2
import numpy as np
import sys
def shift_dft(src, dst=None):
'''
Rearrange the quadrants of Fourier image so that the origin is at
the image center. Swaps quadrant 1 with 3, and 2 with 4.
src and dst arrays must be equal size & type
'''
if dst is None:
dst = np.empty(src.shape, src.dtype)
elif src.shape != dst.shape:
raise ValueError("src and dst must have equal sizes")
elif src.dtype != dst.dtype:
raise TypeError("src and dst must have equal types")
if src is dst:
ret = np.empty(src.shape, src.dtype)
else:
ret = dst
h, w = src.shape[:2]
cx1 = cx2 = w/2
cy1 = cy2 = h/2
# if the size is odd, then adjust the bottom/right quadrants
if w % 2 != 0:
cx2 += 1
if h % 2 != 0:
cy2 += 1
# swap quadrants
# swap q1 and q3
ret[h-cy1:, w-cx1:] = src[0:cy1 , 0:cx1 ] # q1 -> q3
ret[0:cy2 , 0:cx2 ] = src[h-cy2:, w-cx2:] # q3 -> q1
# swap q2 and q4
ret[0:cy2 , w-cx2:] = src[h-cy2:, 0:cx2 ] # q2 -> q4
ret[h-cy1:, 0:cx1 ] = src[0:cy1 , w-cx1:] # q4 -> q2
if src is dst:
dst[:,:] = ret
return dst
if __name__ == "__main__":
if len(sys.argv)>1:
im = cv2.imread(sys.argv[1])
else :
im = cv2.imread('../c/baboon.jpg')
print "usage : python dft.py <image_file>"
# convert to grayscale
im = cv2.cvtColor(im, cv2.COLOR_BGR2GRAY)
h, w = im.shape[:2]
realInput = im.astype(np.float64)
# perform an optimally sized dft
dft_M = cv2.getOptimalDFTSize(w)
dft_N = cv2.getOptimalDFTSize(h)
# copy A to dft_A and pad dft_A with zeros
dft_A = np.zeros((dft_N, dft_M, 2), dtype=np.float64)
dft_A[:h, :w, 0] = realInput
# no need to pad bottom part of dft_A with zeros because of
# use of nonzeroRows parameter in cv2.dft()
cv2.dft(dft_A, dst=dft_A, nonzeroRows=h)
cv2.imshow("win", im)
# Split fourier into real and imaginary parts
image_Re, image_Im = cv2.split(dft_A)
# Compute the magnitude of the spectrum Mag = sqrt(Re^2 + Im^2)
magnitude = cv2.sqrt(image_Re**2.0 + image_Im**2.0)
# Compute log(1 + Mag)
log_spectrum = cv2.log(1.0 + magnitude)
# Rearrange the quadrants of Fourier image so that the origin is at
# the image center
shift_dft(log_spectrum, log_spectrum)
# normalize and display the results as rgb
cv2.normalize(log_spectrum, log_spectrum, 0.0, 1.0, cv2.cv.CV_MINMAX)
cv2.imshow("magnitude", log_spectrum)
cv2.waitKey(0)
cv2.destroyAllWindows()
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