Polar confinement of the Sun's interior magnetic field by laminar magnetostrophic flow

DOI10.1017/jfm.2011.93zbMath1241.76462arXiv1005.5482OpenAlexW2166673469WikidataQ58422301 ScholiaQ58422301MaRDI QIDQ2891659

M. E. McIntyre, Toby S. Wood

Publication date: 15 June 2012

Published in: Journal of Fluid Mechanics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1005.5482

zbMATH Keywords

MHD and electrohydrodynamics

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (2)

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Cites Work

• On Ekman and Hartmann boundary layers in a rotating fluid
• Magnetic field confinement by meridional flow and the solar tachocline
• Diamagnetic pumping near the base of a stellar convection zone
• The slender solar tachocline: a magnetic model
• Axisymmetric flow between differentially rotating spheres in a dipole magnetic field
• The magneto-hydrodynamics of a rotating fluid and the earth’s dynamo problem
• The Non-uniform Rotation of the Sun and its Magnetic Field
• Rotation and Stellar Evolution

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