Solar flares: an extreme of reconnection

Details Solar flares: an extreme of reconnection Solar flares: an extreme of reconnection

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mare.conf.....c&link_type=abstract

Presented at Chapman Conf. on Magnetic Reconnection, Los Alamos, N. Mex., 3 Oct. 1983

Physics

Plasma Physics

Flux Density, Force-Free Magnetic Fields, Magnetic Field Configurations, Magnetic Flux, Magnetohydrodynamics, Solar Flares, Solar Flux, Annihilation Reactions, Axial Strain, Lines Of Force, Magnetohydrodynamic Waves, Plasma Pinch, Plasma Turbulence, Shear Flow, Simulation, Solar Magnetic Field

Scientific paper

Three points are emphasized: that the solar flare is that particular astrophysical phenomenon that is the extremum of reconnection, no other phenomenon demands as rapid magnetic flux annihilation as is seen in the solar flare; that plasma physics experiments can and should be performed in the laboratory that model reconnection as observed in astrophysics; and that stochastic field lines derived from something similar to Alfven wave turbulence are a neccesary part of reconnection.

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