Force-free magnetic structures in the solar wind

Details Force-free magnetic structures in the solar wind Force-free magnetic structures in the solar wind

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ge%26ae..33...23l&link_type=abstract

Geomagnetizm i Aeronomiya (ISSN 0016-7940), vol. 33, no. 2, p. 23-34.

Computer Science

Force-Free Magnetic Fields, Interplanetary Magnetic Fields, Solar Flares, Solar Magnetic Field, Solar Wind Velocity, Magnetic Field Configurations, Plasma Compression, Solar Terrestrial Interactions

Scientific paper

The possibility of modeling force-free magnetic structures in the solar wind by a cylindrically symmetric force-free field is examined. Ten specific events in the solar wind are modeled, and field parameters for these events are obtained. It is shown that force-free magnetic fields are most frequently observed at the interface of a flare stream and the compressed solar wind. They are observed less frequently in the region of the compressed solar wind and even in the quiet solar wind. A small beta parameter and low speed are characteristic for force-free magnetic structures.

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