The energy dependence of the secondary to primary ratio

Details The energy dependence of the secondary to primary ratio The energy dependence of the secondary to primary ratio

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....9..271m&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Late Papers. Volume 9 (A85-22801 0

Physics

Energetic Particles, Galactic Cosmic Rays, Magnetohydrodynamic Waves, Particle Diffusion, Plasma-Particle Interactions, Heavy Nuclei, Radiation Distribution

Scientific paper

The energy dependence of the secondary to primary ratios in the cosmic
rays can be explained by a model accounting for the scattering of the
particles by self-generated Alfvén waves. This model predicts an
energy-dependent truncation of the pathlength distribution.

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