Reconnection and acceleration to high energies in flares

Details Reconnection and acceleration to high energies in flares Reconnection and acceleration to high energies in flares

Jun 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..374..493s&link_type=abstract

High energy solar physics. AIP Conference Proceedings, Volume 374, pp. 493-497 (1996).

Physics

Electric And Magnetic Fields, Solar Magnetism, Plasma Dynamics And Flow

Scientific paper

Acceleration of protons and heavy ions in a reconnecting current sheet (RCS), which forms as a consequence of coronal transient, CME, or filament eruption in the corona, is advocated as a possible mechanism of relativistic particle generation during the late phase of γ-ray flares. The important feature of the mechanism suggested is that neither the maximum energy nor the acceleration rate depend upon the particle mass.

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