view scripts/signal/yulewalker.m @ 20170:af2b7695f1c4 draft default tip @

gallery.m: clean and vectorize part of qmult. * scripts/special-matrix/gallery.m: make qmult() follow Octave guidelines, vectorize last for loop in qmult().
author Antonio Pino Robles <data.script93@gmail.com>
date Thu, 28 May 2015 18:32:47 +0200
parents 4197fc428c7d
children f1d0f506ee78
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## Copyright (C) 1995-2015 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 3 of the License, 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, see
## <http://www.gnu.org/licenses/>.

## -*- 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, @dots{}, 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)

  if (nargin != 1)
    print_usage ();
  endif

  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