Generation of magnetic fields by fluid motions of global scale

DOI10.1080/03091927708240370zbMath0352.76075OpenAlexW2021662126WikidataQ114641060 ScholiaQ114641060MaRDI QIDQ4123038

D. Gubbins, E. C. Bullard

Publication date: 1977

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

Full work available at URL: https://doi.org/10.1080/03091927708240370

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05)

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Ambivalent effects of added layers on steady kinematic dynamos in cylindrical geometry: application to the VKS experiment ⋮ Toward an experimental von Kármán dynamo: Numerical studies for an optimized design ⋮ A trio of simple optimized axisymmetric kinematic dynamos in a sphere ⋮ The role of mean circulation in parity selection by planetary magnetic fields ⋮ A multi-layered kinematic dynamo model: implications of a stratified upper layer in the Earth's core ⋮ Numerical solution of the kinematic dynamo problem for Beltrami flows in a sphere ⋮ The optimal kinematic dynamo driven by steady flows in a sphere ⋮ Numerical simulation of a spherical dynamo excited by a flow of von Kármán type

Cites Work

• Axisymmetric convection in a rotating sphere. Part 1. Stress-free surface
• Dynamo Action of Isotropically Driven Motions of a Rotating Fluid
• Thermal instabilities in rapidly rotating systems
• Generation of magnetic fields by convection
• Numerical solutions of the kinematic dynamo problem

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