Magneto-Gravito-Inertial waves in strongly stratified stellar interiors

Details Magneto-Gravito-Inertial waves in strongly stratified stellar interiors Magneto-Gravito-Inertial waves in strongly stratified stellar interiors

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1170..635m&link_type=abstract

STELLAR PULSATION: CHALLENGES FOR THEORY AND OBSERVATION: Proceedings of the International Conference. AIP Conference Proceedin

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Stellar Characteristics And Properties, Cepheids, Gravitational Radiation, Magnetic Fields, And Other Observations

Scientific paper

Stellar radiation zones are stable strongly stratified rotating magnetic regions. The buoyancy force, the Coriolis acceleration and the Lorentz force are thus ruling the gravity waves dynamics. In this work, we examine the behaviour of these waves in stellar interiors and we show how the approximations assumed in the non-magnetic case (for gravito-inertial waves) can be generalized.

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