The cross-over to magnetostrophic convection in planetary dynamo systems

DOI10.1098/rspa.2016.0731zbMath1404.85016OpenAlexW2606141625WikidataQ53354275 ScholiaQ53354275MaRDI QIDQ4647150

E. M. King, Jonathan M. Aurnou

Publication date: 4 January 2019

Published in: Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1098/rspa.2016.0731

zbMATH Keywords

rotating convectiondynamosscaling theorymagnetostrophic balance

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Geo-electricity and geomagnetism (86A25)

Related Items (9)

The inherent instability of axisymmetric magnetostrophic dynamo models ⋮ Solenoidal force balances in numerical dynamos ⋮ Determination of the instantaneous geostrophic flow within the three-dimensional magnetostrophic regime ⋮ Thermoelectric precession in turbulent magnetoconvection ⋮ Rotating thermal convection in liquid gallium: multi-modal flow, absent steady columns ⋮ Evolution of forced magnetohydrodynamic waves in a stratified fluid ⋮ The turbulent dynamo ⋮ Prograde, retrograde, and oscillatory modes in rotating Rayleigh–Bénard convection ⋮ Oscillatory thermal–inertial flows in liquid metal rotating convection

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