On high degree F modes

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Equations Of Motion, Solar Oscillations, Vibration Mode, Astronomical Models, Eigenvalues, Perturbation Theory

Scientific paper

The objective of the analysis presented here is to demonstrate that
there is always a finite difference between the eigenvalue of the f
modes of a spherical star and that of a plane atmosphere. This is shown
to be true for any degree of the f modes. The analysis employs the
Cowling approximation.

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