Solar cycle properties described by simple convection-driven dynamos

DOI10.1088/0031-8949/86/01/018407zbMath1272.85004arXiv1112.3569OpenAlexW3100179194WikidataQ59793877 ScholiaQ59793877MaRDI QIDQ2844889

Radostin D. Simitev, Friedrich H. Busse

Publication date: 20 August 2013

Published in: Physica Scripta (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1112.3569

zbMATH Keywords

convectionBoussinesq approximationsunmagnetic field generationrotating spherical shellsdynamo waves

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Galactic and stellar structure (85A15) Electromagnetic theory (general) (78A25) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

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