Volume 376, Number 2, September II 2001
|Page(s)||708 - 712|
|Published online||15 September 2001|
The effect of time-dependent random mass density field on frequencies of solar sound waves
Department of Environmental Physics, Technical University of Lublin, ul. Nadbystrzycka 40, 20-618 Lublin, Poland
2 Institute of Atomic and Molecular Physics, National Research Council, Via Moruzzi 1, 56124 Pisa, Italy
Corresponding author: K. Murawski, firstname.lastname@example.org
Accepted: 26 June 2001
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.
Key words: convection / Sun: oscillations / turbulence
© ESO, 2001
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