Magnetic boundary and acceleration of charged particles in spatially nonuniform configurations

Details Magnetic boundary and acceleration of charged particles in spatially nonuniform configurations Magnetic boundary and acceleration of charged particles in spatially nonuniform configurations

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.251..185b&link_type=abstract

In ESA Proceedings of the Joint Varenna-Abastumani International School and Workshop on Plasma Astrophysics p 185-194 (SEE N87-

Astronomy and Astrophysics

Astrophysics

Magnetic Field Reconnection, Particle Acceleration, Space Plasmas, Current Sheets, Magnetic Field Configurations, Magnetohydrodynamic Stability, Plasma Interactions, Stellar Flares, Tearing Modes (Plasmas)

Scientific paper

The formation of current sheets in three dimensional magnetic configurations near zero points and zero lines of a magnetic field is discussed. The separatrix surfaces play an important role. The current sheet stability and its rupture is considered. The acceleration of charged particles near null points of a magnetic field in the presence of a uniform electric field is investigated. Solar and stellar flares are described.

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