On the Excitation of Solar Five-Minute Oscillations View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

1988

AUTHORS

H. M. Antia , S. M. Chitre , D. O. Gough

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. More... »

PAGES

371-374

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-94-009-4009-3_75

DOI

http://dx.doi.org/10.1007/978-94-009-4009-3_75

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1017098480


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