Effect of statistical acceleration in the interplanetary medium on the propagation of particles from a solar flare

Details Effect of statistical acceleration in the interplanetary medium on the propagation of particles from a solar flare Effect of statistical acceleration in the interplanetary medium on the propagation of particles from a solar flare

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ge%26ae..32...13b&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 32, no. 2, Mar.-Apr. 1992, p. 13-18. In Russian.

Physics

Interplanetary Medium, Particle Acceleration, Particle Trajectories, Relativistic Particles, Solar Flares, Adiabatic Conditions, Convection-Diffusion Equation, Statistical Distributions, Time Lag, Transport Properties

Scientific paper

Existing analytical solutions of the nonstationarty transport equation including convection, diffusion, and adiabatic time delay of particles in the case of their instantaneous injection from a spherical shell of given radius r0 are generalized to the relativistic case, with allowance made for the statistical turbulent acceleration of the particles. The effects of acceleration and of changes of r0 on the time profiles of particle intensity are investigated.

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