Coronal heating by relaxation in a sunspot magnetic field

DOI10.1080/03091928808208829zbMath0642.76061OpenAlexW2131761951WikidataQ114640322 ScholiaQ114640322MaRDI QIDQ3783721

P. K. Browning, A. M. Dixon, Eric R. Priest

Publication date: 1988

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

Full work available at URL: https://doi.org/10.1080/03091928808208829

zbMATH Keywords

heating by resistive turbulencephotospheric footpointssolar coronal magnetic fieldsTaylor- Heyvaerts hypothesis

Mathematics Subject Classification ID

Galactic and stellar dynamics (85A05) Ionized gas flow in electromagnetic fields; plasmic flow (76X05) Stability and instability of geophysical and astrophysical flows (76E20)

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