Non-axisymmetric α2Ω-dynamo waves in thin stellar shells

DOI10.1080/03091920500159887zbMath1206.85007OpenAlexW2147633550MaRDI QIDQ3081186

Andrew P. Bassom, K. M. Kuzanyan, Andrew M. Soward, Dmitry D. Sokoloff

Publication date: 5 March 2011

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

Full work available at URL: https://doi.org/10.1080/03091920500159887

zbMATH Keywords

differential rotationphase mixingdynamo waves

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Galactic and stellar structure (85A15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (1)

The WKB approximation for the interface dynamo

Cites Work

• Asymptotic solution of the α²-dynamo problem
• THE LINEAR STRABILITY OF THE FLOW IN THE NARROW GAP BETWEEN TWO CONCENTRIC ROTATING SPHERES
• Symmetry breaking in stellar dynamos
• Three‐dimensional model for generation of the mean solar magnetic field
• Investigations of spherical kinematic mean-field dynamo models
• Non-axisymmetric spherical interface dynamos

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