Mercurial > hg > smallbox
view util/sparco utils/pwsmoothfield.m @ 162:88578ec2f94a danieleb
Updated grassmannian function and minor debugs
author | Daniele Barchiesi <daniele.barchiesi@eecs.qmul.ac.uk> |
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date | Wed, 31 Aug 2011 13:52:23 +0100 |
parents | 62f20b91d870 |
children |
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function f = pwsmoothfield(n,var,alpha) % PWSMOOTHFIELD(N,VAR,ALPHA) % Generate an image of piecewise smooth filtered white noise % % N = sidelength of the field in pixels % VAR = variance of original white nose % ALPHA = fraction of FFT coefficents to keep % % Returns an N-by-N array % % This file is used with the kind permission of Stephen J. Wright % (swright@cs.wisc.edu), and was originally included in the GPSR % v1.0 distribution: http://www.lx.it.pt/~mtf/GPSR . % $Id: pwsmoothfield.m 1040 2008-06-26 20:29:02Z ewout78 $ f = sqrt(var)*randn(n); F = fft2(f); a = ceil(n*alpha/2); b = fix(n*(1-alpha)); F(a+1:a+b,:) = 0; F(:,a+1:a+b) = 0; f = real(ifft2(F)); for i = 1:n for j = 1:n if (j/n >= 15*(i/n - 0.5)^3 + 0.4) f(i,j) = f(i,j) + sqrt(var); end end end