A boundary-layer model unifies viscous, Alfvén-wave, and Ohmic contributions to the drag on an oscillating sphere in a rotating MHD cavity, extended to equatorial modes and validated by simulations for planetary applications.
equation 89 of Smylie & McMillan 1998), e.g
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Magnetohydrodynamic drag on an oscillating sphere in a rotating cavity
A boundary-layer model unifies viscous, Alfvén-wave, and Ohmic contributions to the drag on an oscillating sphere in a rotating MHD cavity, extended to equatorial modes and validated by simulations for planetary applications.