Force free fields and coronal heating part I. The formation of current sheets

DOI10.1080/03091928808208850zbMath0711.76116OpenAlexW2043452356WikidataQ114640313 ScholiaQ114640313MaRDI QIDQ3496113

Adriaan van Ballegooijen

Publication date: 1988

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

Full work available at URL: https://doi.org/10.1080/03091928808208850

zbMATH Keywords

solar coronal loopsideal-MHD instabilitiessmall-scale magnetic structures

Mathematics Subject Classification ID

Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Ionized gas flow in electromagnetic fields; plasmic flow (76X05)

Related Items (1)

Magnetohydrodynamic simulation of coronal magnetic fields

Cites Work

• Equilibrium of magnetic fields with arbitrary interweaving of the lines of force II. Discontinuities in the field
• Equilibrium of magnetic fields with arbitrary interweaving of the lines of force i. discontinuities in the torsion
• Magnetostatic equilibria and analogous Euler flows of arbitrarily complex topology. Part 1. Fundamentals
• The effect of homogeneous turbulence on material lines and surfaces

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