Covariant description of non-relativistic magnetohydrodynamics

DOI10.1080/03091920600744356zbMath1206.76077OpenAlexW2009360381MaRDI QIDQ3081229

Paul H. Roberts, Andrew M. Soward

Publication date: 5 March 2011

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

Full work available at URL: https://doi.org/10.1080/03091920600744356

zbMATH Keywords

magnetohydrodynamicsrotating fluidsgeneral tensors

Mathematics Subject Classification ID

General theory of rotating fluids (76U05) Magnetohydrodynamics and electrohydrodynamics (76W05)

Related Items (8)

A geometric look at MHD and the Braginsky dynamo ⋮ A geometric look at momentum flux and stress in fluid mechanics ⋮ The hybrid Euler–Lagrange procedure using an extension of Moffatt's method ⋮ Eulerian–Lagrangian means in rotating, magnetohydrodynamic flows I. General results ⋮ Geometric generalised Lagrangian-mean theories ⋮ Geometric Lagrangian averaged Euler–Boussinesq and primitive equations ⋮ The Navier–Stokes-αequations revisited ⋮ Eulerian and Lagrangian means in rotating, magnetohydrodynamic flows II. Braginsky’s nearly axisymmetric dynamo

Cites Work

• Eulerian–Lagrangian means in rotating, magnetohydrodynamic flows I. General results
• An exact theory of nonlinear waves on a Lagrangian-mean flow
• On wave-action and its relatives
• A kinematic theory of large magnetic Reynolds number dynamos
• Lagrangian averages, averaged Lagrangians, and the mean effects of fluctuations in fluid dynamics
• Unnamed Item

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