The asymptotic spectrum of gravity modes as a function of the solar structure - Standard solar model

Details The asymptotic spectrum of gravity modes as a function of the solar structure - Standard solar model The asymptotic spectrum of gravity modes as a function of the solar structure - Standard solar model

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..133..127b&link_type=abstract

(IRIS /International Research on the Interior of the Sun/ Workshop, 2nd, Tashkent, Uzbek SSR, Sept. 1989, Proceedings. A91-37551

Physics

4

Asymptotic Properties, Gravity Waves, Solar Rotation, Stellar Models, Stellar Structure, Coriolis Effect, Frequency Distribution, Gravitational Fields

Scientific paper

It is shown that the solution of the second-order differential equation which governs the periods of the gravity modes of a solar model with radial order larger than 10 can be estimated with an accuracy of 0.001 or less by a second-order asymptotic expression of the periods of low-degree gravity modes. It is suggested that the solution can be used to find g-modes in a signal.

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