Effects of the solar wind-magnetosphere coupling in March 1989

Details Effects of the solar wind-magnetosphere coupling in March 1989 Effects of the solar wind-magnetosphere coupling in March 1989

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sowi.conf..102s&link_type=abstract

Buenos Aires Univ., International Solar Wind 8 Conference, p. 102

Astronomy and Astrophysics

Astronomy

Solar Wind, Stellar Magnetospheres, Electromagnetic Coupling, Geomagnetism, Auroral Electrojets, Solar Activity, Magnetic Disturbances, Interplanetary Magnetic Fields, Astronomical Models

Scientific paper

The March 1989 solar and geophysical activity are reinvestigated. To describe the geomagnetic disturbance fields, the auroral electrojet indices are calculated. Eight southern Geomagnetic Observatories placed at high latitudes are selected and their geomagnetic data are used. The models of a storm like an addition of substorms are analyzed. During disturbed periods. the temporal evolution of the solar wind parameters and the interplanetary magnetic field components are discussed. Plasmoids could be identified and their energy are estimated. Differences in both auroral rings behaviour are seen.

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