Three‐dimensional model for generation of the mean solar magnetic field

DOI10.1002/asna.2113060402zbMath0571.76115OpenAlexW2091132695MaRDI QIDQ3688029

T. S. Ivanova, Alexander Ruzmaikin

Publication date: 1985

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

Full work available at URL: https://doi.org/10.1002/asna.2113060402

zbMATH Keywords

finite-difference schemePeaceman-Rachford schemedifferential rotation and mean helicity in the convective shellexpansion over the spherical functionssolar mean magnetic field generationsymmetric solutions relative to equator planethree-dimensional non- axisymmetric model

Mathematics Subject Classification ID

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

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Non-axisymmetric α²Ω-dynamo waves in thin stellar shells ⋮ On the generation of non-axisymmetric magnetic fields in mean-field dynamos

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