Stochastic wave excitation in rotating stars

Details Stochastic wave excitation in rotating stars Stochastic wave excitation in rotating stars

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008coast.157..144m&link_type=abstract

Communications in Asteroseismology, Vol.157, p. 144-148

Computer Science

1

Scientific paper

Wave propagation, excitation and associated transport are modified by the Coriolis and the centrifugal accelerations in rotating stars. In this work, we focus on the influence of the Coriolis acceleration on the volumetric stochastic excitation in convection zones of rotating stars. First, we present the complete formalism which has been derived and discuss the different terms which appear due to the Coriolis acceleration. Then, we use this formalism to compute the solar mode excitation rates and emphasize the peculiar behavior due to rotation. Consequences on wave transport in rotating stars are eventually discussed.

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