Mercurial > hg > octave-nkf
view scripts/signal/yulewalker.m @ 6828:d069de22e9aa
[project @ 2007-08-24 16:59:47 by jwe]
author | jwe |
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date | Fri, 24 Aug 2007 16:59:48 +0000 |
parents | 4c8a2e4e0717 |
children | 93c65f2a5668 |
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## Copyright (C) 1995, 1996, 1997 Friedrich Leisch ## ## This file is part of Octave. ## ## Octave is free software; you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation; either version 2, or (at your option) ## any later version. ## ## Octave is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Octave; see the file COPYING. If not, write to the Free ## Software Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA ## 02110-1301, USA. ## -*- texinfo -*- ## @deftypefn {Function File} {[@var{a}, @var{v}] =} yulewalker (@var{c}) ## Fit an AR (p)-model with Yule-Walker estimates given a vector @var{c} ## of autocovariances @code{[gamma_0, ..., gamma_p]}. ## ## Returns the AR coefficients, @var{a}, and the variance of white ## noise, @var{v}. ## @end deftypefn ## Author: FL <Friedrich.Leisch@ci.tuwien.ac.at> ## Description: Fit AR model by Yule-Walker method function [a, v] = yulewalker (c) p = length (c) - 1; if (columns (c) > 1) c = c'; endif cp = c(2 : p+1); CP = zeros(p, p); for i = 1:p for j = 1:p CP (i, j) = c (abs (i-j) + 1); endfor endfor a = inv (CP) * cp; v = c(1) - a' * cp; endfunction