Localization and features of the development of reconnection processes at the magnetopause

Details Localization and features of the development of reconnection processes at the magnetopause Localization and features of the development of reconnection processes at the magnetopause

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ge%26ae..25..592s&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 25, July-Aug. 1985, p. 592-597. In Russian.

Physics

2

Geomagnetism, Lines Of Force, Magnetic Field Configurations, Magnetopause, Solar Terrestrial Interactions, Atmospheric Models, Interplanetary Magnetic Fields, Solar Wind, Space Plasmas

Scientific paper

A model for the interaction of the solar wind and the magnetopause is proposed which is based on the anomalous-resistance concept. The length and direction of a reconnection line are determined along with the difference of potentials as a function of interplanetary-magnetic-field orientation. It is shown that reconnection occurs primarily at a subsolar point. In a small range of angles near the northward direction, reconnection is more likely beyond the cusps.

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