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Influence of the perturbation of the Reynolds tensor on the stability of the solar 5 minute oscillations

Published online by Cambridge University Press:  03 August 2017

M. Gabriel
M. Gabriel*
Affiliation:
Institut d'Astrophysique de l'Université de Liège

Extract

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The excitation mechanism of the 5 min. oscillations is not yet understood. So far two mechanisms have been discussed. The first one is the linear vibrational instability. The second one is the non linear coupling between convection and pulsation discussed by Goldreich and Keeley (1977) and Goldreich and Kumar (1986).

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. 375 - 378
Copyright
Copyright © Reidel 1988 

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