Energy dissipation in substorms: plasmoids ejection

Details Energy dissipation in substorms: plasmoids ejection Energy dissipation in substorms: plasmoids ejection

Jul 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997jastp..59.1355s&link_type=abstract

Journal of Atmospheric and Terrestrial Physics, v. 59, p. 1355-1358.

Physics

1

Scientific paper

Intense solar events in March 1989 caused important effects in the Earth's magnetosphere. This is demonstrated by the temporal evolution of the auroral electrojet index (AE), the mid-latitude geomagnetic index (SYM-H), the solar wind coupling parameter (ɛ) and the total energy rate dissipated by the magnetosphere (UT) for the substorm detected on 5 March 1989. For this event the energy dissipated by plasmoids ejection (PE) in the antisolar direction is estimated using a new approach.

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