Mercurial > hg > ltpda
view m-toolbox/classes/+utils/@math/spflat.m @ 3:960fe1aa1c10 database-connection-manager
Add LTPDADatabaseConnectionManager implementation. Java code
author | Daniele Nicolodi <nicolodi@science.unitn.it> |
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date | Mon, 05 Dec 2011 16:20:06 +0100 |
parents | f0afece42f48 |
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% spflat measures the flatness of a given spectrum %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% % % DESCRIPTION: spflat measures the flatness of a given spectrum using the % spectral flatness measure method reported in [1]. It outputs the spectral % flatness coefficient: % % 0 <= sw <= 1 % % If the spectrum is peaky then sw is near 0. The more the spectrum is flat % the more sw in near to 1. The sw coefficient is practically calculated by % the ratio between geometric mean and arithmetic mean of the spectrum. % % CALL: % % sw = spflat(S) % % INPUTS: % % - S sample power spectrum. More than one sample spectrum can be % input if they are combined in a single nxm matrix. The algorithm % calculates sw for each spectrum. % % OUTPUT: % % - sw spectral flatness coefficient. If more than one spectrum % are input sw is a row vector. % % REFERENCES: % % [1] S. M. Kay, Modern spectral estimation:Theory and Application, % Prentice Hall, Englewood Cliffs (1988) ISBN-10: 0130151599. Pages % ??. % % % % VERSION: $Id: spflat.m,v 1.2 2009/01/29 08:59:26 luigi Exp $ % % % HISTORY: 28-01-2009 L Ferraioli % Creation % % %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% function sw = spflat(S) % willing to work with columns [a,b] = size(S); if a>1 && b>1 warning('Matlab:MultipleSpectra','A matrix of data was input; Spectral Flatness Coefficient will be calculated for each column') else if a<b S = S.'; end end Ns = size(S,1); gmean = exp(sum(log(S))./Ns); sw = gmean./mean(S); end