Alfven wave scattering and the secondary to primary ratio

Details Alfven wave scattering and the secondary to primary ratio Alfven wave scattering and the secondary to primary ratio

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....3...58b&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 3 p 58-60 (SEE N85-34862 23-93)

Physics

Abundance, Cosmic Ray Showers, Magnetic Fields, Magnetohydrodynamic Waves, Molecular Clouds, Scatter Propagation, Secondary Cosmic Rays, Topology, Diffusion Coefficient, Heavy Nuclei, Interstellar Space, Nonlinearity, Spallation, Steady State

Scientific paper

The cosmic ray abundances have traditionally been used to determine the elemental and isotopic nature of galactic ray sources and average measures of propagation conditions. Detailed studies of the physics of propagation are usually paired with relatively straightforward estimates of the secondary-to-primary (S/P) ratios. In the work reported here, calculations of elemental abundances are paired with a more careful treatment of the propagation process. It is shown that the physics of propagation does indeed leave specific traces of Galactic structure in cosmic ray abundances.

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