Quasi-static evolution of sheared force-free fields and the solar flare problem

Details Quasi-static evolution of sheared force-free fields and the solar flare problem Quasi-static evolution of sheared force-free fields and the solar flare problem

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...143...19a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 143, no. 1, Feb. 1985, p. 19-22. Research supported by the Centre National de

Astronomy and Astrophysics

Astrophysics

68

Force-Free Magnetic Fields, Magnetohydrodynamics, Quasi-Steady States, Solar Flares, Solar Magnetic Field, Magnetic Field Configurations, Photosphere, Solar Corona

Scientific paper

The author reports some new results showing the possible evolution of a two-dimensional force-free field in the half-space {z > 0} toward an open field. This evolution is driven by shearing motions applied to the feet of the field lines on the boundary {z = 0}. The author discusses the consequences of his results for a model of the two-ribbon solar flare.

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