Heliospheric Plasma and Current Sheet Structure

Details Heliospheric Plasma and Current Sheet Structure Heliospheric Plasma and Current Sheet Structure

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679...93c&link_type=abstract

SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 93-97

Physics

Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

Recent analyses using suprathermal electrons as sensors of true magnetic polarity indicate that the steady-state concepts of the heliospheric current sheet and its encasing plasma sheet often break down at solar wind time scales of less than a day owing to transient and turbulent effects. These create magnetic configurations with localized current and plasma sheets and sometimes cause the current to split off from the surface separating fields of true opposite polarity.

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