Sensitivity to luminosity, centrifugal force, and boundary conditions in spherical shell convection

DOI10.1080/03091929.2019.1571586zbMath1482.76065arXiv1807.09309OpenAlexW2953173374WikidataQ114640067 ScholiaQ114640067MaRDI QIDQ5065690

Petri J. Käpylä, N. Olspert, Maarit J. Käpylä, Frederick A. Gent, Axel Brandenburg

Publication date: 22 March 2022

Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1807.09309

zbMATH Keywords

convectionturbulencemagnetohydrodynamicsdynamos

Mathematics Subject Classification ID

Convective turbulence (76F35)

Related Items (3)

The time step constraint in radiation hydrodynamics ⋮ Introduction ⋮ Ill-posedness of the mean-field dynamo equations with a linear electromotive force

Uses Software

• EULAG

Cites Work

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• Hydromagnetic turbulence in computer simulations
• Convective dynamos in spherical wedge geometry
• Turbulent viscosity, magnetic diffusivity, and heat conductivity under the influence of rotation and magnetic field
• Mean-field concept and direct numerical simulations of rotating magnetoconvection and the geodynamo
• Effects of a subadiabatic layer on convection and dynamos in spherical wedge simulations
• Effect of the radiative background flux in convection

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