Including the Sun's radiative interior in inertial mode models slightly modifies frequencies and surface eigenfunctions for most modes but enables mixed Rossby-inertial modes with high interior mode mass that are hard to excite stochastically.
J., Christensen-Dalsgaard , J., Miesch , M
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Effects of the radiative interior on solar inertial modes
Including the Sun's radiative interior in inertial mode models slightly modifies frequencies and surface eigenfunctions for most modes but enables mixed Rossby-inertial modes with high interior mode mass that are hard to excite stochastically.