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On the excitation of solar five-minute oscillations
Published online by Cambridge University Press: 03 August 2017
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.
- Type
- Chapter 6: Excitation and Damping of Solar and Stellar Oscillations
- Information
- Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 371 - 374
- Copyright
- Copyright © Reidel 1988
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