Particle orbits, trapping, and acceleration in a filamentary current sheet model

Details Particle orbits, trapping, and acceleration in a filamentary current sheet model Particle orbits, trapping, and acceleration in a filamentary current sheet model

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apjs...90..719k&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 90, no. 2, p. 719-728

Astronomy and Astrophysics

Astrophysics

34

Current Sheets, Magnetically Trapped Particles, Mathematical Models, Orbitals, Particle Acceleration, Solar Prominences, Electric Fields, Energy Transfer, Faddeev Equations, Magnetic Field Reconnection, Magnetohydrodynamic Stability, Two Dimensional Models

Scientific paper

Test particle orbits in the two-dimensional Fadeev equilibrium with a perpendicular electric field added are analyzed to show that impulsive bursty reconnection, which has been proposed as a model for fragmentary energy release in solar flares, may account also for particle acceleration to (near) relativistic energies within a fraction of a second. The convective electric field connected with magnetic island dynamics can play an important role in the acceleration process.

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