How can α 2‐dynamos generate axisymmetric magnetic fields?

DOI10.1002/ASNA.200710864zbMath1130.85310OpenAlexW2026256577MaRDI QIDQ5440155

Detlef Elstner, Günther Rüdiger

Publication date: 31 January 2008

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

Full work available at URL: https://doi.org/10.1002/asna.200710864

zbMATH Keywords

magnetohydrodynamics (MHD)stars: magnetic fields

Mathematics Subject Classification ID

Galactic and stellar structure (85A15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (1)

Spectral properties of oscillatory and non-oscillatory α²-dynamos

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