σ-stability analysis of toroidal magnetic fields in stars

DOI10.1080/03091928008241174zbMath0435.76087OpenAlexW2010421430WikidataQ114640812 ScholiaQ114640812MaRDI QIDQ3875624

Marcel Goossens

Publication date: 1980

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

Full work available at URL: https://doi.org/10.1080/03091928008241174

zbMATH Keywords

toroidal magnetic fieldssigma-stabilitymaximum growth-rates

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Galactic and stellar structure (85A15) Stability and instability of magnetohydrodynamic and electrohydrodynamic flows (76E25) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (1)

Dynamical and secular instability of a self-gravitating rotating cylinder in a toroidal magnetic field

Cites Work

• New approach to magnetohydrodynamic stability: I. A practical stability concept
• Stability criteria and the maximum growth rate in magnetohydrodynamics

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