Author:
Antia H.M.,Chitre S.M.,Gough D.O.
Abstract
A simple prescription for the dynamics of convection perturbed by stellar pulsation is used in an estimation of the growth rates of solar five-minute modes. Convection appears to enhance the excitation of the modes, and the maximum in the growth rate versus frequency found previously when oscillatory convective perturbations were ignored is still present.
Publisher
Cambridge University Press (CUP)
Cited by
1 articles.
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