Computer Science
Scientific paper
Aug 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ge%26ae..31..577b&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 31, July-Aug. 1991, p. 577-582. In Russian.
Computer Science
2
Charged Particles, Interplanetary Medium, Particle Diffusion, Solar Flares, Transport Properties, Adiabatic Equations, Diffusion Coefficient, Interplanetary Magnetic Fields, Solar Magnetic Field, Solar Protons
Scientific paper
A general analytical solution is obtained for the nonstationary transport equation, taking into account convection, radial diffusion, adiabatic deceleration and statistical aceleration of particles with a power spectrum with respect to momentum. Under conditions of the instantaneous injection of solar particles, an evaluation is made of the time and radial dependences of the particle intensity, the radial intensity gradient, and the vector of the particle flux anisotropy; and the role of acceleration is investigated. The results obtained are compared with observed temporal profiles of the intensity of nonrelativistic protons from a solar flare.
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