我想知道是否有一种方法可以通过分析图像数据来确定图像是否模糊。
当前回答
我想到了一个完全不同的解决方案。 我需要分析视频静止帧，以便在每(X)帧中找到最清晰的帧。这样，我将检测运动模糊和/或失焦图像。
我最终使用了Canny边缘检测，我得到了非常非常好的结果，几乎每一种视频(与尼基的方法，我有数字化的VHS视频和沉重的交错视频的问题)。
我通过在原始图像上设置感兴趣区域(ROI)来优化性能。
使用EmguCV:
//Convert image using Canny
using (Image<Gray, byte> imgCanny = imgOrig.Canny(225, 175))
{
//Count the number of pixel representing an edge
int nCountCanny = imgCanny.CountNonzero()[0];
//Compute a sharpness grade:
//< 1.5 = blurred, in movement
//de 1.5 à 6 = acceptable
//> 6 =stable, sharp
double dSharpness = (nCountCanny * 1000.0 / (imgCanny.Cols * imgCanny.Rows));
}
其他回答
我目前使用的一种方法是测量图像中边缘的分布。请看这篇论文:
@ARTICLE{Marziliano04perceptualblur,
author = {Pina Marziliano and Frederic Dufaux and Stefan Winkler and Touradj Ebrahimi},
title = {Perceptual blur and ringing metrics: Application to JPEG2000,” Signal Process},
journal = {Image Commun},
year = {2004},
pages = {163--172} }
它通常都是付费版本，但我也看到过一些免费版本。基本上，他们在图像中定位垂直边缘，然后测量这些边缘的宽度。平均宽度给出了图像的最终模糊估计结果。较宽的边缘对应模糊的图像，反之亦然。
该问题属于无参考图像质量估计领域。如果你在谷歌Scholar上查一下，你会得到很多有用的参考资料。
EDIT
下面是nickie发布的5张图片的模糊估计图。数值越高，模糊程度越高。我使用固定大小的11x11高斯滤波器，并改变了标准偏差(使用imagemagick的convert命令来获得模糊的图像)。
如果你比较不同大小的图像，不要忘记通过图像宽度归一化，因为较大的图像会有更宽的边缘。
最后，一个重要的问题是区分艺术模糊和不必要的模糊(由对焦缺失、压缩、拍摄对象相对于相机的运动引起)，但这超出了像这样简单的方法。举个艺术模糊的例子，看看莱娜的形象:莱娜在镜子里的倒影是模糊的，但她的脸是完美的聚焦。这有助于对莱纳图像进行更高的模糊估计。
在一些自动对焦镜头的工作中，我遇到了一组非常有用的检测图像焦点的算法。它是在MATLAB中实现的，但大多数函数都很容易通过filter2D移植到OpenCV中。
它基本上是许多焦点测量算法的一个调查实现。如果您想阅读原始论文，代码中提供了对算法作者的引用。Pertuz等人2012年的论文。通过对焦点形状测量算子(SFF)的分析，对所有这些测量算子及其性能(包括应用于SFF的速度和精度)进行了回顾。
编辑:添加MATLAB代码，以防链接死亡。
function FM = fmeasure(Image, Measure, ROI)
%This function measures the relative degree of focus of
%an image. It may be invoked as:
%
% FM = fmeasure(Image, Method, ROI)
%
%Where
% Image, is a grayscale image and FM is the computed
% focus value.
% Method, is the focus measure algorithm as a string.
% see 'operators.txt' for a list of focus
% measure methods.
% ROI, Image ROI as a rectangle [xo yo width heigth].
% if an empty argument is passed, the whole
% image is processed.
%
% Said Pertuz
% Abr/2010
if ~isempty(ROI)
Image = imcrop(Image, ROI);
end
WSize = 15; % Size of local window (only some operators)
switch upper(Measure)
case 'ACMO' % Absolute Central Moment (Shirvaikar2004)
if ~isinteger(Image), Image = im2uint8(Image);
end
FM = AcMomentum(Image);
case 'BREN' % Brenner's (Santos97)
[M N] = size(Image);
DH = Image;
DV = Image;
DH(1:M-2,:) = diff(Image,2,1);
DV(:,1:N-2) = diff(Image,2,2);
FM = max(DH, DV);
FM = FM.^2;
FM = mean2(FM);
case 'CONT' % Image contrast (Nanda2001)
ImContrast = inline('sum(abs(x(:)-x(5)))');
FM = nlfilter(Image, [3 3], ImContrast);
FM = mean2(FM);
case 'CURV' % Image Curvature (Helmli2001)
if ~isinteger(Image), Image = im2uint8(Image);
end
M1 = [-1 0 1;-1 0 1;-1 0 1];
M2 = [1 0 1;1 0 1;1 0 1];
P0 = imfilter(Image, M1, 'replicate', 'conv')/6;
P1 = imfilter(Image, M1', 'replicate', 'conv')/6;
P2 = 3*imfilter(Image, M2, 'replicate', 'conv')/10 ...
-imfilter(Image, M2', 'replicate', 'conv')/5;
P3 = -imfilter(Image, M2, 'replicate', 'conv')/5 ...
+3*imfilter(Image, M2, 'replicate', 'conv')/10;
FM = abs(P0) + abs(P1) + abs(P2) + abs(P3);
FM = mean2(FM);
case 'DCTE' % DCT energy ratio (Shen2006)
FM = nlfilter(Image, [8 8], @DctRatio);
FM = mean2(FM);
case 'DCTR' % DCT reduced energy ratio (Lee2009)
FM = nlfilter(Image, [8 8], @ReRatio);
FM = mean2(FM);
case 'GDER' % Gaussian derivative (Geusebroek2000)
N = floor(WSize/2);
sig = N/2.5;
[x,y] = meshgrid(-N:N, -N:N);
G = exp(-(x.^2+y.^2)/(2*sig^2))/(2*pi*sig);
Gx = -x.*G/(sig^2);Gx = Gx/sum(Gx(:));
Gy = -y.*G/(sig^2);Gy = Gy/sum(Gy(:));
Rx = imfilter(double(Image), Gx, 'conv', 'replicate');
Ry = imfilter(double(Image), Gy, 'conv', 'replicate');
FM = Rx.^2+Ry.^2;
FM = mean2(FM);
case 'GLVA' % Graylevel variance (Krotkov86)
FM = std2(Image);
case 'GLLV' %Graylevel local variance (Pech2000)
LVar = stdfilt(Image, ones(WSize,WSize)).^2;
FM = std2(LVar)^2;
case 'GLVN' % Normalized GLV (Santos97)
FM = std2(Image)^2/mean2(Image);
case 'GRAE' % Energy of gradient (Subbarao92a)
Ix = Image;
Iy = Image;
Iy(1:end-1,:) = diff(Image, 1, 1);
Ix(:,1:end-1) = diff(Image, 1, 2);
FM = Ix.^2 + Iy.^2;
FM = mean2(FM);
case 'GRAT' % Thresholded gradient (Snatos97)
Th = 0; %Threshold
Ix = Image;
Iy = Image;
Iy(1:end-1,:) = diff(Image, 1, 1);
Ix(:,1:end-1) = diff(Image, 1, 2);
FM = max(abs(Ix), abs(Iy));
FM(FM<Th)=0;
FM = sum(FM(:))/sum(sum(FM~=0));
case 'GRAS' % Squared gradient (Eskicioglu95)
Ix = diff(Image, 1, 2);
FM = Ix.^2;
FM = mean2(FM);
case 'HELM' %Helmli's mean method (Helmli2001)
MEANF = fspecial('average',[WSize WSize]);
U = imfilter(Image, MEANF, 'replicate');
R1 = U./Image;
R1(Image==0)=1;
index = (U>Image);
FM = 1./R1;
FM(index) = R1(index);
FM = mean2(FM);
case 'HISE' % Histogram entropy (Krotkov86)
FM = entropy(Image);
case 'HISR' % Histogram range (Firestone91)
FM = max(Image(:))-min(Image(:));
case 'LAPE' % Energy of laplacian (Subbarao92a)
LAP = fspecial('laplacian');
FM = imfilter(Image, LAP, 'replicate', 'conv');
FM = mean2(FM.^2);
case 'LAPM' % Modified Laplacian (Nayar89)
M = [-1 2 -1];
Lx = imfilter(Image, M, 'replicate', 'conv');
Ly = imfilter(Image, M', 'replicate', 'conv');
FM = abs(Lx) + abs(Ly);
FM = mean2(FM);
case 'LAPV' % Variance of laplacian (Pech2000)
LAP = fspecial('laplacian');
ILAP = imfilter(Image, LAP, 'replicate', 'conv');
FM = std2(ILAP)^2;
case 'LAPD' % Diagonal laplacian (Thelen2009)
M1 = [-1 2 -1];
M2 = [0 0 -1;0 2 0;-1 0 0]/sqrt(2);
M3 = [-1 0 0;0 2 0;0 0 -1]/sqrt(2);
F1 = imfilter(Image, M1, 'replicate', 'conv');
F2 = imfilter(Image, M2, 'replicate', 'conv');
F3 = imfilter(Image, M3, 'replicate', 'conv');
F4 = imfilter(Image, M1', 'replicate', 'conv');
FM = abs(F1) + abs(F2) + abs(F3) + abs(F4);
FM = mean2(FM);
case 'SFIL' %Steerable filters (Minhas2009)
% Angles = [0 45 90 135 180 225 270 315];
N = floor(WSize/2);
sig = N/2.5;
[x,y] = meshgrid(-N:N, -N:N);
G = exp(-(x.^2+y.^2)/(2*sig^2))/(2*pi*sig);
Gx = -x.*G/(sig^2);Gx = Gx/sum(Gx(:));
Gy = -y.*G/(sig^2);Gy = Gy/sum(Gy(:));
R(:,:,1) = imfilter(double(Image), Gx, 'conv', 'replicate');
R(:,:,2) = imfilter(double(Image), Gy, 'conv', 'replicate');
R(:,:,3) = cosd(45)*R(:,:,1)+sind(45)*R(:,:,2);
R(:,:,4) = cosd(135)*R(:,:,1)+sind(135)*R(:,:,2);
R(:,:,5) = cosd(180)*R(:,:,1)+sind(180)*R(:,:,2);
R(:,:,6) = cosd(225)*R(:,:,1)+sind(225)*R(:,:,2);
R(:,:,7) = cosd(270)*R(:,:,1)+sind(270)*R(:,:,2);
R(:,:,7) = cosd(315)*R(:,:,1)+sind(315)*R(:,:,2);
FM = max(R,[],3);
FM = mean2(FM);
case 'SFRQ' % Spatial frequency (Eskicioglu95)
Ix = Image;
Iy = Image;
Ix(:,1:end-1) = diff(Image, 1, 2);
Iy(1:end-1,:) = diff(Image, 1, 1);
FM = mean2(sqrt(double(Iy.^2+Ix.^2)));
case 'TENG'% Tenengrad (Krotkov86)
Sx = fspecial('sobel');
Gx = imfilter(double(Image), Sx, 'replicate', 'conv');
Gy = imfilter(double(Image), Sx', 'replicate', 'conv');
FM = Gx.^2 + Gy.^2;
FM = mean2(FM);
case 'TENV' % Tenengrad variance (Pech2000)
Sx = fspecial('sobel');
Gx = imfilter(double(Image), Sx, 'replicate', 'conv');
Gy = imfilter(double(Image), Sx', 'replicate', 'conv');
G = Gx.^2 + Gy.^2;
FM = std2(G)^2;
case 'VOLA' % Vollath's correlation (Santos97)
Image = double(Image);
I1 = Image; I1(1:end-1,:) = Image(2:end,:);
I2 = Image; I2(1:end-2,:) = Image(3:end,:);
Image = Image.*(I1-I2);
FM = mean2(Image);
case 'WAVS' %Sum of Wavelet coeffs (Yang2003)
[C,S] = wavedec2(Image, 1, 'db6');
H = wrcoef2('h', C, S, 'db6', 1);
V = wrcoef2('v', C, S, 'db6', 1);
D = wrcoef2('d', C, S, 'db6', 1);
FM = abs(H) + abs(V) + abs(D);
FM = mean2(FM);
case 'WAVV' %Variance of Wav...(Yang2003)
[C,S] = wavedec2(Image, 1, 'db6');
H = abs(wrcoef2('h', C, S, 'db6', 1));
V = abs(wrcoef2('v', C, S, 'db6', 1));
D = abs(wrcoef2('d', C, S, 'db6', 1));
FM = std2(H)^2+std2(V)+std2(D);
case 'WAVR'
[C,S] = wavedec2(Image, 3, 'db6');
H = abs(wrcoef2('h', C, S, 'db6', 1));
V = abs(wrcoef2('v', C, S, 'db6', 1));
D = abs(wrcoef2('d', C, S, 'db6', 1));
A1 = abs(wrcoef2('a', C, S, 'db6', 1));
A2 = abs(wrcoef2('a', C, S, 'db6', 2));
A3 = abs(wrcoef2('a', C, S, 'db6', 3));
A = A1 + A2 + A3;
WH = H.^2 + V.^2 + D.^2;
WH = mean2(WH);
WL = mean2(A);
FM = WH/WL;
otherwise
error('Unknown measure %s',upper(Measure))
end
end
%************************************************************************
function fm = AcMomentum(Image)
[M N] = size(Image);
Hist = imhist(Image)/(M*N);
Hist = abs((0:255)-255*mean2(Image))'.*Hist;
fm = sum(Hist);
end
%******************************************************************
function fm = DctRatio(M)
MT = dct2(M).^2;
fm = (sum(MT(:))-MT(1,1))/MT(1,1);
end
%************************************************************************
function fm = ReRatio(M)
M = dct2(M);
fm = (M(1,2)^2+M(1,3)^2+M(2,1)^2+M(2,2)^2+M(3,1)^2)/(M(1,1)^2);
end
%******************************************************************
OpenCV版本的几个例子:
// OpenCV port of 'LAPM' algorithm (Nayar89)
double modifiedLaplacian(const cv::Mat& src)
{
cv::Mat M = (Mat_<double>(3, 1) << -1, 2, -1);
cv::Mat G = cv::getGaussianKernel(3, -1, CV_64F);
cv::Mat Lx;
cv::sepFilter2D(src, Lx, CV_64F, M, G);
cv::Mat Ly;
cv::sepFilter2D(src, Ly, CV_64F, G, M);
cv::Mat FM = cv::abs(Lx) + cv::abs(Ly);
double focusMeasure = cv::mean(FM).val[0];
return focusMeasure;
}
// OpenCV port of 'LAPV' algorithm (Pech2000)
double varianceOfLaplacian(const cv::Mat& src)
{
cv::Mat lap;
cv::Laplacian(src, lap, CV_64F);
cv::Scalar mu, sigma;
cv::meanStdDev(lap, mu, sigma);
double focusMeasure = sigma.val[0]*sigma.val[0];
return focusMeasure;
}
// OpenCV port of 'TENG' algorithm (Krotkov86)
double tenengrad(const cv::Mat& src, int ksize)
{
cv::Mat Gx, Gy;
cv::Sobel(src, Gx, CV_64F, 1, 0, ksize);
cv::Sobel(src, Gy, CV_64F, 0, 1, ksize);
cv::Mat FM = Gx.mul(Gx) + Gy.mul(Gy);
double focusMeasure = cv::mean(FM).val[0];
return focusMeasure;
}
// OpenCV port of 'GLVN' algorithm (Santos97)
double normalizedGraylevelVariance(const cv::Mat& src)
{
cv::Scalar mu, sigma;
cv::meanStdDev(src, mu, sigma);
double focusMeasure = (sigma.val[0]*sigma.val[0]) / mu.val[0];
return focusMeasure;
}
不能保证这些措施是否是您的问题的最佳选择，但如果您追踪与这些措施相关的论文，它们可能会给您更多的见解。希望您觉得代码有用!我知道我说过。
谢谢妮基的拉普拉斯建议。 OpenCV文档给我指出了同样的方向: 使用python, cv2 (opencv 2.4.10)和numpy…
gray = cv2.cvtColor(img, cv2.COLOR_BGR2GRAY)
numpy.max(cv2.convertScaleAbs(cv2.Laplacian(gray, 3)))
结果在0-255之间。我发现任何超过200的东西都非常清晰，而到了100，就明显模糊了。Max从来没有真正低于20，即使它完全模糊。
我在matlab中使用FFT实现了它，并检查FFT的直方图，计算平均值和STD，还可以做拟合函数
fa = abs(fftshift(fft(sharp_img)));
fb = abs(fftshift(fft(blured_img)));
f1=20*log10(0.001+fa);
f2=20*log10(0.001+fb);
figure,imagesc(f1);title('org')
figure,imagesc(f2);title('blur')
figure,hist(f1(:),100);title('org')
figure,hist(f2(:),100);title('blur')
mf1=mean(f1(:));
mf2=mean(f2(:));
mfd1=median(f1(:));
mfd2=median(f2(:));
sf1=std(f1(:));
sf2=std(f2(:));
在高度重视的期刊(IEEE Transactions on Image Processing)上发表的两种方法的Matlab代码可在这里获得:https://ivulab.asu.edu/software
检查CPBDM和JNBM算法。如果你检查代码，它并不难移植，顺便说一下，它是基于Marzialiano的方法作为基本特征。
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