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Autoregressive Modeling of Golf Velocity Time Series
Published online by Cambridge University Press: 08 February 2017
Extract
The frequencies of solar p-modes are usually computed by fitting Lorentzian profiles to the observed signals’ Fourier spectra. We offer a new technique to estimate mode parameters: direct modeling by autoregressive stochastic processes, in conjunction with Singular Spectrum Analysis.
- Type
- I. Global Structure and Evolution of the Solar and Stellar Interior
- Information
- Symposium - International Astronomical Union , Volume 185: New Eyes to See Inside the Sun and Stars , 1998 , pp. 57 - 58
- Copyright
- Copyright © Kluwer 1998