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%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% % Integration of Wilson model with the Euler method %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% clear; clf

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% % Integration of Wilson model with the Euler method %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% clear; clf

/* fft/hc_pass_n.c * * Copyright (C) 1996, 1997, 1998, 1999, 2000 Brian Gough * * This program is free software; you can redistribute it and/or modify * it under the terms of the GNU General Pu

/* fft/c_pass_n.c * * Copyright (C) 1996, 1997, 1998, 1999, 2000 Brian Gough * * This program is free software; you can redistribute it and/or modify * it under the terms of the GNU General Pub

/* fft/real_pass_n.c * * Copyright (C) 1996, 1997, 1998, 1999, 2000 Brian Gough * * This program is free software; you can redistribute it and/or modify * it under the terms of the GNU General

fu<mark>n</mark>ctio<mark>n</mark> [A1_mi<mark>n</mark>, A2_mi<mark>n</mark>, A3_mi<mark>n</mark>, A4_mi<mark>n</mark>] = L4<mark>n</mark>(s_size, levelc, model, i<mark>n</mark>i_poi<mark>n</mark>t, xx0, sf, <mark>N</mark>p, <mark>N</mark>d, dm, ws, wp, out<mark>n</mark>ame) % Desig<mark>n</mark> of qui<mark>n</mark>cu<mark>n</mark>x filter ba<mark>n</mark>ks with four lifti<mark>n</mark>g steps w ...

function [p_min, u_min] = L2n(s_size, Np, Nu, levelc, model, ini_point, x00, sf, dm, ws, wp, outname) % optimize the coding gain subject to the error of h1 is less than dh1 % with second-order cone pr

function [A1_min, A2_min, A3_min] = L3n(s_size, level, model, ini_point, x00, sf, Np, Nd, dm, ws, wp, outname) % optimize the coding gain subject to the error of h1 is less than dh1 % with second-orde

function y=mmpx2n(x,Hf) %MMPX2N Pixel to Normalized Coordinate Transformation. % MMPX2N(X) converts the position vector X from % pixel coordinates to normalized coordinates w.r.t. % the computer scree