本文整理匯總了Python中cv2.dft方法的典型用法代碼示例。如果您正苦於以下問題:Python cv2.dft方法的具體用法?Python cv2.dft怎麽用?Python cv2.dft使用的例子?那麽, 這裏精選的方法代碼示例或許可以為您提供幫助。您也可以進一步了解該方法所在類cv2
的用法示例。
在下文中一共展示了cv2.dft方法的15個代碼示例,這些例子默認根據受歡迎程度排序。您可以為喜歡或者感覺有用的代碼點讚,您的評價將有助於係統推薦出更棒的Python代碼示例。
示例1: update
# 需要導入模塊: import cv2 [as 別名]
# 或者: from cv2 import dft [as 別名]
def update(_):
ang = np.deg2rad( cv2.getTrackbarPos('angle', win) )
d = cv2.getTrackbarPos('d', win)
noise = 10**(-0.1*cv2.getTrackbarPos('SNR (db)', win))
if defocus:
psf = defocus_kernel(d)
else:
psf = motion_kernel(ang, d)
cv2.imshow('psf', psf)
psf /= psf.sum()
psf_pad = np.zeros_like(img)
kh, kw = psf.shape
psf_pad[:kh, :kw] = psf
PSF = cv2.dft(psf_pad, flags=cv2.DFT_COMPLEX_OUTPUT, nonzeroRows = kh)
PSF2 = (PSF**2).sum(-1)
iPSF = PSF / (PSF2 + noise)[...,np.newaxis]
RES = cv2.mulSpectrums(IMG, iPSF, 0)
res = cv2.idft(RES, flags=cv2.DFT_SCALE | cv2.DFT_REAL_OUTPUT )
res = np.roll(res, -kh//2, 0)
res = np.roll(res, -kw//2, 1)
cv2.imshow(win, res)
示例2: __init__
# 需要導入模塊: import cv2 [as 別名]
# 或者: from cv2 import dft [as 別名]
def __init__(self, frame, rect):
x1, y1, x2, y2 = rect
w, h = map(cv2.getOptimalDFTSize, [x2-x1, y2-y1])
x1, y1 = (x1+x2-w)//2, (y1+y2-h)//2
self.pos = x, y = x1+0.5*(w-1), y1+0.5*(h-1)
self.size = w, h
img = cv2.getRectSubPix(frame, (w, h), (x, y))
self.win = cv2.createHanningWindow((w, h), cv2.CV_32F)
g = np.zeros((h, w), np.float32)
g[h//2, w//2] = 1
g = cv2.GaussianBlur(g, (-1, -1), 2.0)
g /= g.max()
self.G = cv2.dft(g, flags=cv2.DFT_COMPLEX_OUTPUT)
self.H1 = np.zeros_like(self.G)
self.H2 = np.zeros_like(self.G)
for i in xrange(128):
a = self.preprocess(rnd_warp(img))
A = cv2.dft(a, flags=cv2.DFT_COMPLEX_OUTPUT)
self.H1 += cv2.mulSpectrums(self.G, A, 0, conjB=True)
self.H2 += cv2.mulSpectrums( A, A, 0, conjB=True)
self.update_kernel()
self.update(frame)
示例3: update
# 需要導入模塊: import cv2 [as 別名]
# 或者: from cv2 import dft [as 別名]
def update(self, frame, rate = 0.125):
(x, y), (w, h) = self.pos, self.size
self.last_img = img = cv2.getRectSubPix(frame, (w, h), (x, y))
img = self.preprocess(img)
self.last_resp, (dx, dy), self.psr = self.correlate(img)
self.good = self.psr > 8.0
if not self.good:
return
self.pos = x+dx, y+dy
self.last_img = img = cv2.getRectSubPix(frame, (w, h), self.pos)
img = self.preprocess(img)
A = cv2.dft(img, flags=cv2.DFT_COMPLEX_OUTPUT)
H1 = cv2.mulSpectrums(self.G, A, 0, conjB=True)
H2 = cv2.mulSpectrums( A, A, 0, conjB=True)
self.H1 = self.H1 * (1.0-rate) + H1 * rate
self.H2 = self.H2 * (1.0-rate) + H2 * rate
self.update_kernel()
示例4: correlate
# 需要導入模塊: import cv2 [as 別名]
# 或者: from cv2 import dft [as 別名]
def correlate(self, img):
C = cv2.mulSpectrums(cv2.dft(img, flags=cv2.DFT_COMPLEX_OUTPUT), self.H, 0, conjB=True)
resp = cv2.idft(C, flags=cv2.DFT_SCALE | cv2.DFT_REAL_OUTPUT)
h, w = resp.shape
_, mval, _, (mx, my) = cv2.minMaxLoc(resp)
side_resp = resp.copy()
cv2.rectangle(side_resp, (mx-5, my-5), (mx+5, my+5), 0, -1)
smean, sstd = side_resp.mean(), side_resp.std()
psr = (mval-smean) / (sstd+eps)
return resp, (mx-w//2, my-h//2), psr
示例5: fftd
# 需要導入模塊: import cv2 [as 別名]
# 或者: from cv2 import dft [as 別名]
def fftd(img, backwards=False, byRow=False):
# shape of img can be (m,n), (m,n,1) or (m,n,2)
# in my test, fft provided by numpy and scipy are slower than cv2.dft
# return cv2.dft(np.float32(img), flags=((cv2.DFT_INVERSE | cv2.DFT_SCALE) if backwards else cv2.DFT_COMPLEX_OUTPUT)) # 'flags =' is necessary!
# DFT_INVERSE: 用一維或二維逆變換取代默認的正向變換,
# DFT_SCALE: 縮放比例標識符,根據數據元素個數平均求出其縮放結果,如有N個元素,則輸出結果以1/N縮放輸出,常與DFT_INVERSE搭配使用。
# DFT_COMPLEX_OUTPUT: 對一維或二維的實數數組進行正向變換,這樣的結果雖然是複數陣列,但擁有複數的共軛對稱性
if byRow:
return cv2.dft(np.float32(img), flags=(cv2.DFT_ROWS | cv2.DFT_COMPLEX_OUTPUT))
else:
return cv2.dft(np.float32(img), flags=((cv2.DFT_INVERSE | cv2.DFT_SCALE) if backwards else cv2.DFT_COMPLEX_OUTPUT))
# 實部圖像
示例6: fft2
# 需要導入模塊: import cv2 [as 別名]
# 或者: from cv2 import dft [as 別名]
def fft2(img):
img = np.float32(img)
if img.ndim == 2:
out = cv2.dft(img, flags=cv2.DFT_COMPLEX_OUTPUT)
elif img.ndim == 3:
out = []
for c in range(img.shape[2]):
out.append(cv2.dft(
img[..., c], flags=cv2.DFT_COMPLEX_OUTPUT))
out = np.stack(out, axis=2)
else:
raise Exception('only supports 2 or 3 dimensional array')
return out
示例7: ifft2
# 需要導入模塊: import cv2 [as 別名]
# 或者: from cv2 import dft [as 別名]
def ifft2(img):
img = np.float32(img)
if img.ndim == 3:
out = cv2.dft(img, flags=cv2.DFT_INVERSE | cv2.DFT_SCALE)
elif img.ndim == 4:
out = []
for c in range(img.shape[2]):
out.append(cv2.dft(
img[:, :, c, :], flags=cv2.DFT_INVERSE | cv2.DFT_SCALE))
else:
raise Exception('only supports 3 or 4 dimensional array')
return out
示例8: fft1
# 需要導入模塊: import cv2 [as 別名]
# 或者: from cv2 import dft [as 別名]
def fft1(img):
img = np.float32(img)
if img.ndim == 1:
img = img[np.newaxis, :]
out = cv2.dft(img, flags=cv2.DFT_ROWS | cv2.DFT_COMPLEX_OUTPUT)
out = out.squeeze(0)
elif img.ndim == 2:
out = cv2.dft(img, flags=cv2.DFT_ROWS | cv2.DFT_COMPLEX_OUTPUT)
else:
raise Exception('only supports 1 or 2 dimensional array')
return out
示例9: ifft1
# 需要導入模塊: import cv2 [as 別名]
# 或者: from cv2 import dft [as 別名]
def ifft1(img):
img = np.float32(img)
if img.ndim == 2:
img = img[np.newaxis, :, :]
out = cv2.dft(img, flags=cv2.DFT_ROWS | cv2.DFT_SCALE)
out = out.squeeze(0)
elif img.ndim == 3:
out = cv2.dft(img, flags=cv2.DFT_ROWS | cv2.DFT_SCALE)
else:
raise Exception('only supports 2 or 3 dimensional array')
return out
示例10: init
# 需要導入模塊: import cv2 [as 別名]
# 或者: from cv2 import dft [as 別名]
def init(self, image, init_rect):
if image.ndim == 3:
image = cv2.cvtColor(image, cv2.COLOR_BGR2GRAY)
init_rect = init_rect.astype(int)
init_rect[2:] += init_rect[:2]
x1, y1, x2, y2 = init_rect
w, h = map(cv2.getOptimalDFTSize, [x2 - x1, y2 - y1])
x1, y1 = (x1 + x2 - w) // 2, (y1 + y2 - h) // 2
self.t_center = x, y = x1 + 0.5 * (w - 1), y1 + 0.5 * (h - 1)
self.t_sz = w, h
img = cv2.getRectSubPix(image, (w, h), (x, y))
self.win = cv2.createHanningWindow((w, h), cv2.CV_32F)
g = np.zeros((h, w), np.float32)
g[h // 2, w // 2] = 1
g = cv2.GaussianBlur(g, (-1, -1), self.cfg.sigma)
g /= g.max()
self.G = cv2.dft(g, flags=cv2.DFT_COMPLEX_OUTPUT)
self.A = np.zeros_like(self.G)
self.B = np.zeros_like(self.G)
for _i in range(128):
patch = self._preprocess(self._random_warp(img))
F = cv2.dft(patch, flags=cv2.DFT_COMPLEX_OUTPUT)
self.A += cv2.mulSpectrums(self.G, F, 0, conjB=True)
self.B += cv2.mulSpectrums(F, F, 0, conjB=True)
self._update_kernel()
self.update(image)
示例11: _linear_correlation
# 需要導入模塊: import cv2 [as 別名]
# 或者: from cv2 import dft [as 別名]
def _linear_correlation(self, img):
C = cv2.mulSpectrums(
cv2.dft(img, flags=cv2.DFT_COMPLEX_OUTPUT), self.H, 0, conjB=True)
resp = cv2.idft(C, flags=cv2.DFT_SCALE | cv2.DFT_REAL_OUTPUT)
h, w = resp.shape
_, mval, _, (mx, my) = cv2.minMaxLoc(resp)
side_resp = resp.copy()
cv2.rectangle(side_resp, (mx - 5, my - 5), (mx + 5, my + 5), 0, -1)
smean, sstd = side_resp.mean(), side_resp.std()
psr = (mval - smean) / (sstd + self.cfg.eps)
return resp, (mx - w // 2, my - h // 2), psr
示例12: fftd
# 需要導入模塊: import cv2 [as 別名]
# 或者: from cv2 import dft [as 別名]
def fftd(img, backwards=False):
# shape of img can be (m,n), (m,n,1) or (m,n,2)
# in my test, fft provided by numpy and scipy are slower than cv2.dft
return cv2.dft(np.float32(img), flags = ((cv2.DFT_INVERSE | cv2.DFT_SCALE) if backwards else cv2.DFT_COMPLEX_OUTPUT)) # 'flags =' is necessary!
示例13: fourier_transform
# 需要導入模塊: import cv2 [as 別名]
# 或者: from cv2 import dft [as 別名]
def fourier_transform(ch_bd):
dft = cv2.dft(np.float32(ch_bd), flags=cv2.DFT_COMPLEX_OUTPUT)
dft_shift = np.fft.fftshift(dft)
# get the Power Spectrum
magnitude_spectrum = 20. * np.log(cv2.magnitude(dft_shift[:, :, 0], dft_shift[:, :, 1]))
psd1D = azimuthal_avg(magnitude_spectrum)
return list(cv2.meanStdDev(psd1D))
示例14: main
# 需要導入模塊: import cv2 [as 別名]
# 或者: from cv2 import dft [as 別名]
def main():
# read an image
img = cv2.imread('../figures/flower.png')
# create cropped grayscale image from the original image
crop_gray = cv2.cvtColor(img[100:400, 100:400], cv2.COLOR_BGR2GRAY)
# take discrete fourier transform
dft = cv2.dft(np.float32(crop_gray),flags = cv2.DFT_COMPLEX_OUTPUT)
dft_shift = np.fft.fftshift(dft)
magnitude_spectrum = 20*np.log(cv2.magnitude(dft_shift[:,:,0],dft_shift[:,:,1]))
# plot results
plot_dft(crop_gray, magnitude_spectrum)
示例15: _get_channel_sal_magn
# 需要導入模塊: import cv2 [as 別名]
# 或者: from cv2 import dft [as 別名]
def _get_channel_sal_magn(self, channel):
"""Returns the log-magnitude of the Fourier spectrum
This method calculates the log-magnitude of the Fourier spectrum
of a single-channel image. This image could be a regular grayscale
image, or a single color channel of an RGB image.
:param channel: single-channel input image
:returns: log-magnitude of Fourier spectrum
"""
# do FFT and get log-spectrum
if self.use_numpy_fft:
img_dft = np.fft.fft2(channel)
magnitude, angle = cv2.cartToPolar(np.real(img_dft),
np.imag(img_dft))
else:
img_dft = cv2.dft(np.float32(channel),
flags=cv2.DFT_COMPLEX_OUTPUT)
magnitude, angle = cv2.cartToPolar(img_dft[:, :, 0],
img_dft[:, :, 1])
# get log amplitude
log_ampl = np.log10(magnitude.clip(min=1e-9))
# blur log amplitude with avg filter
log_ampl_blur = cv2.blur(log_ampl, (3, 3))
# residual
residual = np.exp(log_ampl - log_ampl_blur)
# back to cartesian frequency domain
if self.use_numpy_fft:
real_part, imag_part = cv2.polarToCart(residual, angle)
img_combined = np.fft.ifft2(real_part + 1j*imag_part)
magnitude, _ = cv2.cartToPolar(np.real(img_combined),
np.imag(img_combined))
else:
img_dft[:, :, 0], img_dft[:, :, 1] = cv2.polarToCart(residual,
angle)
img_combined = cv2.idft(img_dft)
magnitude, _ = cv2.cartToPolar(img_combined[:, :, 0],
img_combined[:, :, 1])
return magnitude