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Lab 4:Image Restoration
By obverting the histograms of four input figures, we can determine the noise types of them.
We can know the first figure has pepper noise, the second input figure has salt noise, for first two figure, we can use median filter to reduce the noise. The third input figure has alt-and-pepper noise, we can use adaptive median filter. The fourth input figure has Gaussian noise, we can use Gaussian filter to restore the figure.
function f = RAMF(img) % adaptive median filter [Im,In] = size(img); nmin = 3; nmax = 9; Imf = img; I_ex = [zeros((nmax-1)/2,In+(nmax-1));zeros(Im,(nmax-1)/2),img,zeros(Im,(nmax-1)/2);zeros((nmax-1)/2,In+(nmax-1))]; for x = 1:Im for y = 1:In for n = nmin:2:nmax Sxy = I_ex(x+(nmax-1)/2-(n-1)/2:x+(nmax-1)/2+(n-1)/2,y+(nmax-1)/2-(n-1)/2:y+(nmax-1)/2+(n-1)/2); Smax = max(max(Sxy));% Find the maximum number of pixels in the window Smin = min(min(Sxy));%Find the minimum number of pixels in the window Smed = median(median(Sxy));%Find the middle value of pixels in the window % Determine if the median is a noise point if Smed > Smin && Smed < Smax % if the median is both greater than the minimum and less than the maximum % If is, exit the if statement, increase the window size, and judge again % is not, then the original value of the point is not a noise point if Imf(x,y) <= Smin || Imf(x,y) >= Smax % if the original value of the point is both greater than the minimum and less than the maximum, then it is not %If not, then the output value, that is, not for processing %If so, the median is printed Imf(x,y) = Smed; end break end end
Imf(x,y) = Smed; end end f = Imf; end
function L=GaussianLow_11711118(I,setD0) I=im2double(I); M=2*size(I,1); N=2*size(I,2); %the size of filter u=-M/2:(M/2-1); v=-N/2:(N/2-1); [U,V]=meshgrid(u,v); D=sqrt(U.^2+V.^2); D0=setD0; H=exp(-(D.^2)./(2*(D0^2))); %generate the Guassian filter J=fftshift(fft2(I,size(H,1),size(H,2))); G=J.*H; L=ifft2(fftshift(G)); L=L(1:size(I,1),1:size(I,2)); end |
We can see that the output figure had lost some high frequency information. And another question is the figure had an edge which I cannot reduce. For instance, like on the top edge of the output figure of the third figure has a line:
We can find that the input figure of question 2 is a figure blurred by atmosphere turbulence. So that we can use full inverse filter to restore the figure.
image_d=imread('Q4_2.tif'); ff=im2double(image_d);%The image gray value is normalized to 0-1 % Fourier transfrom f_Id=fft2(ff); f_Id=fftshift(f_Id); fH_Id=f_Id; [M,N]=size(fH_Id); % set the threshold threshold=90; if threshold>M/2
fH_Id=fH_Id./(H+eps); else %Filter within a certain radius for i=1:M for j=1:N if sqrt((i-M/2).^2+(j-N/2).^2)<threshold fH_Id(i,j)=fH_Id(i,j)./(H(i,j)+eps); end end end end
% Perform the inverse Fourier transform fH_Id1ftshift(fH_Id); f_new=ifft2(fH_Id1); f_new=uint8(abs(f_new)*255);
imshow(f_new); title('output figure with threshold=90'); |
With the threshold value is 90, we can find that the effect of atmosphere turbulence had been reduced.
We can see that the first two picture have noise easily. Then we can take a look at the histogram and frequency domain to determine which kind of noise the input figures have.
We can find that the frequency domain figure can give us nothing. So we need to look at the histogram, we can guess the noise is Gaussian noise.
So, we use the Gaussian lowpass filter to reduce the noise.
This figure is the first two figure pass the Gaussian filter. We can see that the noise has been reduced.
clc; clear; i1=imread('Q4_3_1.tiff'); i2=imread('Q4_3_2.tiff'); i3=imread('Q4_3_3.tiff');
o1=fftshift(fft2(i1)); o2=fftshift(fft2(i2)); o3=fftshift(fft2(i3));
figure(1) subplot(231),imshow(i1); subplot(234),imshow(o1);
subplot(232),imshow(i2); subplot(235),imshow(o2);
subplot(233),imshow(i3); subplot(236),imshow(o3);
figure(4) subplot(221) imhist(i1); subplot(222) imhist(i2); subplot(223) imhist(i3);
n1 = RAMF_11711118(i1); n2 = RAMF_11711118(i2); figure(5) subplot(121) imhist(n1); subplot(122) imhist(n2);
figure(6) subplot(221),imshow(i1); subplot(222),imshow(n1); subplot(223),imshow(i2); subplot(224),imshow(n2);
G1 = GaussianLow_11711118(i1,160); G2 = GaussianLow_11711118(i2,160); figure(7) subplot(121) imhist(G1); subplot(122) imhist(G2);
figure(8) subplot(221),imshow(i1); subplot(222),imshow(G1); subplot(223),imshow(i2); subplot(224),imshow(G2); |
We can take at the question one:
Because the pepper noise is showed as small black points in the figure and slat noise is showed as white points. By the formula we get:
We need to make the black points become brighter; the white points become darker. So we need to thins the dark part for Q>0, and thickens the black part for Q<0?
We can take at the question two:
We can take a look at the formula:
If the σn2 is larger than the actual global variance, the value of fx,y will be decreasing. So the figure may become darker. And become brighter when σn2 is small than the actual global variance
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