Mercurial > hg > smallbox
annotate util/sparco utils/pwsmoothfield.m @ 77:62f20b91d870
add routines from sparco problems privite folder to {root}\util
some changes to ksvd vs rlsdla image denoising example
author | Ivan <ivan.damnjanovic@eecs.qmul.ac.uk> |
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date | Fri, 25 Mar 2011 14:01:50 +0000 |
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children |
rev | line source |
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ivan@77 | 1 function f = pwsmoothfield(n,var,alpha) |
ivan@77 | 2 % PWSMOOTHFIELD(N,VAR,ALPHA) |
ivan@77 | 3 % Generate an image of piecewise smooth filtered white noise |
ivan@77 | 4 % |
ivan@77 | 5 % N = sidelength of the field in pixels |
ivan@77 | 6 % VAR = variance of original white nose |
ivan@77 | 7 % ALPHA = fraction of FFT coefficents to keep |
ivan@77 | 8 % |
ivan@77 | 9 % Returns an N-by-N array |
ivan@77 | 10 % |
ivan@77 | 11 % This file is used with the kind permission of Stephen J. Wright |
ivan@77 | 12 % (swright@cs.wisc.edu), and was originally included in the GPSR |
ivan@77 | 13 % v1.0 distribution: http://www.lx.it.pt/~mtf/GPSR . |
ivan@77 | 14 |
ivan@77 | 15 % $Id: pwsmoothfield.m 1040 2008-06-26 20:29:02Z ewout78 $ |
ivan@77 | 16 |
ivan@77 | 17 f = sqrt(var)*randn(n); |
ivan@77 | 18 F = fft2(f); |
ivan@77 | 19 a = ceil(n*alpha/2); |
ivan@77 | 20 b = fix(n*(1-alpha)); |
ivan@77 | 21 F(a+1:a+b,:) = 0; |
ivan@77 | 22 F(:,a+1:a+b) = 0; |
ivan@77 | 23 f = real(ifft2(F)); |
ivan@77 | 24 |
ivan@77 | 25 for i = 1:n |
ivan@77 | 26 for j = 1:n |
ivan@77 | 27 if (j/n >= 15*(i/n - 0.5)^3 + 0.4) |
ivan@77 | 28 f(i,j) = f(i,j) + sqrt(var); |
ivan@77 | 29 end |
ivan@77 | 30 end |
ivan@77 | 31 end |
ivan@77 | 32 |