Physics
Scientific paper
Jul 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994kofu.symp..251t&link_type=abstract
In: Proceedings of Kofu Symposium, Kofu, Japan, Sept. 6-10, 1993, p.251-254.
Physics
Scientific paper
A nonsteady model of magnetic field reconnection is proposed to examine an effective mechanism for the acceleration of particles to very high energy. Under the frozen-in state of the magnetic field in plasma, a time-dependent electromagnetic field configuration is exactly derived. Accordingly, it is possible to investigate dynamics of accelerated particles in the relativistic regime analytically and numerically. Due to the colliding of two plasmas, the magnetic neutral sheet is generated and the magnetic energy is converted into kinetic and internal energy of plasmas. The model will be a plausible candidate of the solar flare.
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