The effect of time-dependent random mass density field on frequencies of solar sound waves

Details The effect of time-dependent random mass density field on frequencies of solar sound waves The effect of time-dependent random mass density field on frequencies of solar sound waves

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001a%26a...376..708m&link_type=abstract

Astronomy and Astrophysics, v.376, p.708-712 (2001)

Astronomy and Astrophysics

Astrophysics

8

Convection, Sun: Oscillations, Turbulence

Scientific paper

The effect of a time-dependent random mass density field on the frequencies and amplitudes of solar p-modes approximated as sound waves is considered by analytical perturbative means and numerical simulations for one-dimensional hydrodynamic equations. The analytical results, which are worked out for a Gaussian spectrum of the random mass fluctuations, show frequency increase and amplitude amplification, in agreement with numerical simulations.

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