A Parametric Model of the Solar Full-Disk Seismological Signal
Solar eigenmodes frequencies are most often determined using some kind of modelisation of the Fourier spectrum of the data in one or two dimensions. Many statistical refinements have lead to significant improvements in the determination of the frequencies and widths of the spectral lines. Nevertheless, this technique relies strongly on several
Mouret, D. et al.
Fecha de publicación:
0
1998