Energetic spectrum of particles accelerated in the vicinity of the zero line of a magnetic field

Details Energetic spectrum of particles accelerated in the vicinity of the zero line of a magnetic field Energetic spectrum of particles accelerated in the vicinity of the zero line of a magnetic field

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975azh....52..763b&link_type=abstract

Astronomicheskii Zhurnal, vol. 52, July-Aug. 1975, p. 763-771. In Russian.

Astronomy and Astrophysics

Astronomy

15

Cosmic Rays, Current Sheets, Energy Spectra, Particle Acceleration, Stellar Magnetic Fields, Zero Force Curves, Nonuniform Magnetic Fields, Plasma Turbulence, Pulsars

Scientific paper

The acceleration of charged particles (cosmic rays) in the hyperbolic magnetic and uniform electric fields arising during the decay of a neutral current sheet is examined. It is shown that the acceleration process consists of a direct acceleration by the electric field in the nonadiabatic region near the zero line and a betratron acceleration in the drift region. The characteristic energy of charged particles is determined in the nonrelativistic and ultrarelativistic limits. It is found that the energetic spectra have an exponential form in the high-energy range.

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