Preflare acceleration by magnetic trapping in shearing arcades

Details Preflare acceleration by magnetic trapping in shearing arcades Preflare acceleration by magnetic trapping in shearing arcades

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.251..113s&link_type=abstract

In ESA Proceedings of the Joint Varenna-Abastumani International School and Workshop on Plasma Astrophysics p 113-116 (SEE N87-

Mathematics

Dynamical Systems

Coronal Loops, Magnetically Trapped Particles, Particle Acceleration, Shearing, Solar Flares, Solar Magnetic Field, Astronomical Models, Dynamical Systems, Magnetic Flux

Scientific paper

A dynamical global magnetic configuration of a preflare is presented. It is shown that particles trapped in the solar corona moving shear magnetic field can be accelerated within the order of a cyclotron period by the V(p) x B acceleration mechanism in the preflare stage when the arcade-like magnetic flux ascends. This is accompanied by enhancement of magnetic shear due to photospheric shear motions.

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