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The slender solar tachocline: a magnetic model

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Publication:4362195
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DOI10.1002/ASNA.2113180504zbMath0891.76092OpenAlexW2080695143MaRDI QIDQ4362195

Günther Rüdiger, L. L. Kitchatinov

Publication date: 28 October 1997

Published in: Astronomische Nachrichten (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1002/asna.2113180504


zbMATH Keywords

differential rotationrigid rotationsolar convection zonepoloidal field amplitudetransition layer thickness


Mathematics Subject Classification ID

General theory of rotating fluids (76U05) Magnetohydrodynamics and electrohydrodynamics (76W05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)


Related Items (1)

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







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