Propagation of 10 to the 11th power to 10 to the 14th power eV particles in the galaxy

Details Propagation of 10 to the 11th power to 10 to the 14th power eV particles in the galaxy Propagation of 10 to the 11th power to 10 to the 14th power eV particles in the galaxy

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975icrc....2..690g&link_type=abstract

Presented at the 14th Intern. Cosmic Ray Conf., Munich

Astronomy and Astrophysics

Astronomy

Cosmic Rays, Interstellar Magnetic Fields, Lines Of Force, Astronomical Models, Diffusion Theory, Galaxies, Random Processes

Scientific paper

A semicompound diffusion model is suggested which combines the random separation of galactic field lines with compound diffusion. The diffusion's being one-dimensional is restricted to regions in which the field lines being initially gyroradius apart remain well-correlated. Assuming particle escape at the edges of the galactic disc the mean confinement time is given. Also discussed are the direction and magnitude of the anisotropy as well as its angular structure.

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