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- W2111489984 abstract "A two-dimensional model of the propagation of cosmic-ray (CR) nuclei in galaxies is discussed in which cosmic rays, produced in the galactic plane, diffuse into a halo and are convected outward in a galactic wind. Analytical solutions of the convection-diffusion equation are presented, assuming a linear increase of the convection velocity with distance from the plane, V(z)=3 V 0 z, and allowing for an energy-dependent diffusion coefficient, D(E)=D 0 (E/GeV) α . The differences compared to the classical diffusion model are outlined and constraints on model parameters from CR observations and γ-ray observations of the Milky Way are presented" @default.
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- W2111489984 date "1993-01-01" @default.
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- W2111489984 title "Galactic diffusion and wind models of cosmic-ray transport. I - Insight from CR composition studies and gamma-ray observations" @default.
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