Computer Science
Scientific paper
Apr 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979izssr..43..793b&link_type=abstract
(Seminar po Iadernoi Kosmicheskoi Fizike, 10th, Leningrad, USSR, Oct. 1978.) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskaia
Computer Science
1
Cosmic Rays, Galactic Radiation, Interplanetary Space, Plasma-Particle Interactions, Solar Wind, Charge Transfer, Energy Spectra, Flux Density, Hydrogen, Kinetic Energy, Mean Free Path, Nonlinear Systems, Solar Protons, Solar Wind Velocity
Scientific paper
The expected decrease in solar-wind velocity due to the effect of the radial galactic-cosmic-ray gradient and the process of charge transfer from solar-wind protons to interplanetary neutral hydrogen is computed. The relative galactic-cosmic-ray modulation is determined in the framework of nonlinear cosmic-ray modulation theory. Numerical solutions are obtained which indicate that the heliocentric distance at which the solar-wind velocity decreases by an order of magnitude is highly dependent on the cosmic-ray kinetic energy density and that the dependence of the transport mean free path for cosmic-ray particle scattering on heliocentric distance also strongly affects the change in solar-wind velocity.
Babaian Kh. V.
Dorman Lev I.
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