Solar oscillations as an algebraic eigenvalue problem

Details Solar oscillations as an algebraic eigenvalue problem Solar oscillations as an algebraic eigenvalue problem

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mmsai..55..305k&link_type=abstract

(European Physical Society, Ministero della Pubblica Istruzione, and Universita di Catania, EPS Study Conference on Oscillations

Astronomy and Astrophysics

Astronomy

Eigenvalues, Solar Oscillations, Adiabatic Conditions, Opacity, Stellar Models

Scientific paper

The 'Cowling approximation', where the Eulerian perturbation of the gravitational potential is neglected, is used to obtain the frequencies of adiabatic solar oscillations as eigenvalues of a real symmetric matrix. The computed p-mode spectra of low and high degree are compared with observational results. It is suggested that the influence of the Coulomb interactions on the equation of state, which is presently neglected, will probably improve the degree of agreement obtained.

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