An energy method for the stability of solar magneto hydrostatic atmospheres

DOI10.1080/03091928408230365zbMath0557.76046OpenAlexW1992790053WikidataQ114640520 ScholiaQ114640520MaRDI QIDQ3221610

A. W. Hood

Publication date: 1984

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

Full work available at URL: https://doi.org/10.1080/03091928408230365

zbMATH Keywords

energy methodsolar flaresthree dimensional perturbationstwo dimensional magnetohydrostatic fields

Mathematics Subject Classification ID

Stability and instability of magnetohydrodynamic and electrohydrodynamic flows (76E25) Planetary atmospheres (85A20) Stability and instability of geophysical and astrophysical flows (76E20)

Cites Work

• An energy principle for hydromagnetic stability problems
• Stability of a diffuse linear pinch with axial boundaries
• On the Necessity of the Energy Principle of Kruskal and Oberman for Stability