Dynamos driven by convection in rotating spherical shells

DOI10.1002/asna.200410382zbMath1068.85003OpenAlexW2067130599WikidataQ59793922 ScholiaQ59793922MaRDI QIDQ4677685

Friedrich H. Busse, Radostin D. Simitev

Publication date: 12 May 2005

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

Full work available at URL: https://doi.org/10.1002/asna.200410382

zbMATH Keywords

stars: rotationdynamos)stars: interiors (rotating spherical convectionSun: magnetism

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (3)

A study of global magnetic helicity in self-consistent spherical dynamos ⋮ Regimes of thermo-compositional convection and related dynamos in rotating spherical shells ⋮ Large-scale convective dynamos in a stratified rotating plane layer

Cites Work

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