Diffusion and nuclear fragmentation of cosmic rays: choice of galactic model

Details Diffusion and nuclear fragmentation of cosmic rays: choice of galactic model Diffusion and nuclear fragmentation of cosmic rays: choice of galactic model

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....5.1947p&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

2

Scientific paper

The problem of cosmic ray transport in the Galaxy is discussed. The analysis of energy spectra of primary and secondary nuclei, surviving fractions of secondary radioactive isotopes, and cosmic ray anisotropy allows one to determine the parameters of the diffusion-convection model of cosmic ray propagation in a turbulent interstellar medium. Particular attention is given to the interpretation of peaks in the secondary to primary ratios at a few GeV/n, the energy dependence of cosmic ray diffusion, and the shape of cosmic ray source spectrum.

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