Magnetohyrodynamic Turbulence in a Spherical Shell: Galerkin Models, Boundary Conditions, and the Dynamo Problem

The ‘dynamo problem’ requires that the origin of the primarily dipole geomagnetic field be found. The source of the geomagnetic field lies within the outer core of the Earth, which contains a turbulent magnetofluid whose motion is described by the equations of magnetohydrodynamics (MHD). A mathemati...

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Bibliographic Details
Main Author: John V. Shebalin
Format: Article
Language:English
Published: MDPI AG 2025-01-01
Series:Fluids
Subjects:
Online Access:https://www.mdpi.com/2311-5521/10/2/24
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