DocumentCode
2251885
Title
Gaussian noise blind power spectrum estimation from higher order spectra
Author
Turkbeyler, E. ; Constantinides, A.G.
Author_Institution
Dept. of Electr. & Electron. Eng., Imperial Coll. of Sci., Technol. & Med., London, UK
fYear
1993
fDate
1-3 Nov 1993
Firstpage
1167
Abstract
Signal measurements are generally corrupted by some form of noise which is normally taken to be additive noise. Such noise degrades conventional power spectrum estimates. Higher order statistics, however offer a method for power spectrum estimation for which the effect of additive Gaussian noise is eliminated. A new method based on higher order statistics is proposed to estimate the power spectrum. The method employs the trispectrum and bispectrum to calculate the power spectrum, and correspondingly the autocorrelations. Nonparametric and parametric methods (AR, MA, ARMA models) can be employed to estimate the trispectrum and bispectrum, but in this paper, nonparametric bispectrum and trispectrum estimation methods are used. Simulation studies are presented which compare the method with conventional techniques
Keywords
correlation theory; estimation theory; nonparametric statistics; random noise; spectral analysis; statistical analysis; AR models; ARMA models; MA models; additive Gaussian noise; autocorrelations; blind power spectrum estimation; higher order spectra; higher order statistics; nonparametric bispectrum estimation; nonparametric methods; nonparametric trispectrum estimation; signal measurements; simulation studies; Additive noise; Autocorrelation; Degradation; Fourier transforms; Gaussian noise; Higher order statistics; Integrated circuit modeling; Linear systems; Noise measurement; Random processes; Spectral analysis;
fLanguage
English
Publisher
ieee
Conference_Titel
Signals, Systems and Computers, 1993. 1993 Conference Record of The Twenty-Seventh Asilomar Conference on
Conference_Location
Pacific Grove, CA
ISSN
1058-6393
Print_ISBN
0-8186-4120-7
Type
conf
DOI
10.1109/ACSSC.1993.342388
Filename
342388
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