arXiv · 2006.12596
Improved Asymptotic Expressions for the Eigenvalues of Laplace's Tidal Equations
Abstract
Laplace's tidal equations govern the angular dependence of oscillations in stars when uniform rotation is treated within the so-called traditional approximation. Using a perturbation expansion approach, I derive improved expressions for the eigenvalue associated with these equations, valid in the asymptotic limit of large spin parameter $q$. These expressions have a relative accuracy of order $q^{-3}$ for gravito-inertial modes, and $q^{-1}$ for Rossby and Kelvin modes; the corresponding absolute accuracy is of order $q^{-1}$ for all three mode types. I validate my analysis against numerical calculations, and demonstrate how it can be applied to derive formulae for the periods and eigenfunctions of Rossby modes.
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R. H. D. Townsend. 2020-07-21. Improved Asymptotic Expressions for the Eigenvalues of Laplace's Tidal Equations. https://doi.org/10.1093/mnras%2Fstaa2159
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