A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2020; you can also visit the original URL.
The file type is application/pdf.
Autoregressive Modeling of Golf Velocity Time Series
1998
Symposium - International astronomical union
Preserved Fulltext
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