Equilibrium and non-equilibrium of two-arch structures in the solar atmosphere

Details Equilibrium and non-equilibrium of two-arch structures in the solar atmosphere Equilibrium and non-equilibrium of two-arch structures in the solar atmosphere

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989acaps...9..363s&link_type=abstract

(Acta Astrophysica Sinica, vol. 9, no. 4, 1989, p. 363-372) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 13, Dec. 1

Astronomy and Astrophysics

Astrophysics

1

Coronal Loops, Magnetostatic Fields, Nonequilibrium Conditions, Plasma Equilibrium, Power Series, Solar Atmosphere, Convergence, Equilibrium Equations, Similarity Theorem, Solar Activity, Solar Flares, Solar Magnetic Field

Scientific paper

A similarity solution has been derived in the form of a power series of the nonlinear magnetostatic equilibrium equation, and the region of convergence in the parameter space has been identified. Equilibrium configurations are observed in this region, and non-equilibrium configurations outside it. An example of nonlinear equilibrium configuration is shown graphically. The results can be used to explain the generation of multiribbon flares, two-arch structures, and the structures of the magnetic fields above elongated sunspot groups.

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