The structure of coronal magnetic loops. I - Equilibrium theory

Details The structure of coronal magnetic loops. I - Equilibrium theory The structure of coronal magnetic loops. I - Equilibrium theory

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...54..107c&link_type=abstract

Solar Physics, vol. 54, Sept. 1977, p. 107-122. Research supported by the Consiglio Nazionale delle Ricerche, United States-Ital

Physics

Plasma Physics

37

Magnetic Field Configurations, Magnetohydrodynamic Stability, Solar Corona, Solar Magnetic Field, Far Ultraviolet Radiation, Plasma Physics, Pressure Gradients, Radial Distribution, Skylab Program, Stellar Models

Scientific paper

We present here a model, based on observations, for the magnetic-field equilibrium of a cool coronal loop. The pressure structure, taken from the Harvard/Skylab EUV data, is used to modify the usual force-free-field form in quasi-cylindrical symmetry. The resulting field, which has the same direction but different strength, is calculated and its variation displayed. Finally, localized interchange stability is evaluated and discussed, as the first step in a subsequent complete magnetohydrodynamic-stability analysis.

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