Effect of pressure gradients and line-tying on the magnetic stability of coronal loops

DOI10.1080/03091928208213655zbMath0496.76048OpenAlexW1965864868WikidataQ114640649 ScholiaQ114640649MaRDI QIDQ3960349

G. Einaudi, A. W. Hood, Eric R. Priest

Publication date: 1982

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

Full work available at URL: https://doi.org/10.1080/03091928208213655

zbMATH Keywords

equilibriumpressure gradientsstability criterionkink instabilitydense photosphereline-tying effectsmagnetostatics of solar coronal loops

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

• Unnamed Item
• Hydromagnetic stability of a diffuse linear pinch
• The instability of a pinched fluid with a longitudinal magnetic field
• An energy principle for hydromagnetic stability problems
• Stability of a diffuse linear pinch with axial boundaries
• Critical conditions for magnetic instabilities in force-free coronal loops

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