Computer Science
Scientific paper
Mar 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984p%26ss...32..313z&link_type=abstract
Planetary and Space Science (ISSN 0032-0633), vol. 32, March 1984, p. 313-324.
Computer Science
22
Energetic Particles, Geomagnetic Tail, Magnetic Field Configurations, Particle Acceleration, Protons, Computerized Simulation, Energy Spectra, Equations Of Motion
Scientific paper
The paper considers the energy spectrum of particles accelerated near X-point of the magnetic field in the course of the tearing instability development in the current layer. The time dynamics of the spectrum at the linear and nonlinear stages of the instability is studied. The contribution of the particles inflowing into the vicinity of the magnetic X-point due to drift in the crossed electrical and magnetic fields was also taken into account. The dynamics of particle acceleration are numerically simulated and the results of the simulation are compared with the theoretical model. The analytical and numerical calculations are in reasonable agreement with the results of IMP satellites 7 and 8 energetic proton measurements in a wide energy interval.
Lipatov Alexander S.
Lominadze Dzh. G.
Taktakishvili A. L.
Zelenyi Lev M.
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