Autoregressive Modeling of Golf Velocity Time Series

R. Ulrich, F. Varadi, L. Bertello
1998 Symposium - International astronomical union  
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.
doi:10.1017/s0074180900238308 fatcat:2pqkbji5sffobiahtdxth5niwi