A phenomenological study of cosmic ray propagation - A corrected diffusion model

Details A phenomenological study of cosmic ray propagation - A corrected diffusion model A phenomenological study of cosmic ray propagation - A corrected diffusion model

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974a%26a....35..165l&link_type=abstract

Astronomy and Astrophysics, vol. 35, no. 2, Oct. 1974, p. 165-169.

Physics

Nuclear Physics

6

Cosmic Rays, Interstellar Space, Nuclei (Nuclear Physics), Transport Theory, Astronomical Models, Density Distribution, Galactic Structure, Mathematical Models, Phenomenology, Primary Cosmic Rays

Scientific paper

We show that the mathematical solution of the transfer equation given by
Le Guet and Pacheco (1973) for the propagation of cosmic nuclei is
incorrect. We give the correction and find that in certain cases the
diffusion coefficient can differ by about an order of magnitude from
that obtained previously.

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