Mathematics
Scientific paper
May 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978izyak..42.1047d&link_type=abstract
(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, June 1977.) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheska
Mathematics
Cosmic Rays, Galactic Radiation, Interplanetary Space, Modulation, Anisotropic Media, Deceleration, Mathematical Models, Particle Diffusion, Solar Wind
Scientific paper
Spatial-temporal variations in the three-dimensional anisotropy vector are computed for different models of galactic-cosmic-ray propagation in interplanetary space. The linear theory of cosmic-ray modulation is used to consider a model of anisotropic diffusion in the presence of latitudinal and longitudinal solar-wind asymmetries as well as the spherically symmetric anisotropic-diffusion model. Nonlinear modulation theory is employed to examine a spherically symmetric model of anisotropic diffusion and to evaluate the effect of cosmic-ray focusing in an asymmetric model. The linear theory indicates that the anisotropy vector and cosmic-ray fluxes become more asymmetric with increasing distance from the sun and that the amplitude of 27-day cosmic-ray variations increases for increasing values of the modulation parameter. The nonlinear results show that the nonlinear interaction between the solar wind and cosmic-ray fluxes causes the solar wind to decelerate at large distances from the sun.
Babaian Kh. V.
Debish A. M.
Dorman Lev I.
Ianke V. G.
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