Structure of convection in the magnetosphere in cases of southward and northward directions of the IMF

Details Structure of convection in the magnetosphere in cases of southward and northward directions of the IMF Structure of convection in the magnetosphere in cases of southward and northward directions of the IMF

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ge%26ae..29..725a&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 29, Sept.-Oct. 1989, p. 725-729. In Russian.

Physics

2

Convection, Earth Magnetosphere, Interstellar Magnetic Fields, Earth Ionosphere, Electric Potential, Magnetic Field Reconnection

Scientific paper

It is shown that differences in the structure of the magnetospheric magnetic field for southward and northward directions of the IMF are due to different reconnection processes. In the northward case, the reconnection occurs at two neutral points of the magnetic field and has an essentially three-dimensional character. In the southward case, a two-dimensional pattern arises, which is analogous to line-type reconnection.

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