Magnetic field geometry, not just strength, reshapes tidal dissipation spectra in rotating convective envelopes, though frequency-averaged dissipation usually stays near the hydrodynamical prediction.
Journal of Fluid Mechanics , year = 1967, month = jan, volume =
1 Pith paper cite this work, alongside 162 external citations. Polarity classification is still indexing.
1
Pith paper citing it
162
external citations · OpenAlex
fields
astro-ph.EP 1years
2026 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations
Magnetic field geometry, not just strength, reshapes tidal dissipation spectra in rotating convective envelopes, though frequency-averaged dissipation usually stays near the hydrodynamical prediction.