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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| Hlavní autor: | |
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| Médium: | Artigo |
| Jazyk: | Inglês |
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MDPI AG
2025-01-01
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| Edice: | Fluids |
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| On-line přístup: | https://www.mdpi.com/2311-5521/10/2/24 |
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