The solar power spectrum - A fractal set

Details The solar power spectrum - A fractal set The solar power spectrum - A fractal set

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ap%26ss..74..149p&link_type=abstract

Astrophysics and Space Science, vol. 74, no. 1, Jan. 1981, p. 149-156.

Astronomy and Astrophysics

Astrophysics

10

Astrophysics, Power Spectra, Solar Oscillations, Spectrum Analysis, Stellar Models, Turbulence, Vibration Mode

Scientific paper

A preliminary numerical analysis of the power spectrum of solar oscillations of the SCLERA group suggests that this curve can be characterized by a Hausdorff-Besicovich dimension close to 3/2 near the present observational resolution (approximately 0.03 MHz). It is shown that this result is not inconsistent with the presence of a component due to nonlinear, turbulent-like motions, which, in addition to linear oscillation modes, is shaping the observed spectral distribution

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