pith:UWZE5O2G
Magnetohydrodynamic drag on an oscillating sphere in a rotating spherical cavity
A unified boundary-layer theory gives the magnetohydrodynamic drag on an oscillating sphere in a rotating cavity.
arxiv:2604.10594 v2 · 2026-04-12 · physics.flu-dyn · physics.geo-ph
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Claims
We derive boundary layers and obtain the magnetohydrodynamic drag from Alfvén-wave radiation, viscous effects and Ohmic dissipation (accounting for pressure effects). The theory is extended to non-axisymmetric equatorial modes and to rotation perturbations of the polar mode... Our magnetohydrodynamic simulations validate our theory, providing a quantitative framework for planetary interiors.
The analysis assumes small-amplitude translational oscillations so that linearised boundary-layer approximations remain valid, and that electromagnetic contrasts between the solid sphere and fluid (or outer boundary) can be treated through standard matching conditions without additional surface effects.
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.
Receipt and verification
| First computed | 2026-07-07T03:18:55.622086Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
a5b24ebb467153ace4dc22f6a646c720b786c829452660e025f1215a5766cd53
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/UWZE5O2GOFJ2ZZG4EL3KMRWHEC \
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Canonical record JSON
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