Advective Diffusion Propagation Model for Galactic Cosmic Rays above 1012 eV

Details Advective Diffusion Propagation Model for Galactic Cosmic Rays above 1012 eV Advective Diffusion Propagation Model for Galactic Cosmic Rays above 1012 eV

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....1..315o&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

5

Scientific paper

Based on the detailed research for the diffusive motions of protons and nuclei with energies more than 1012 eV in the galactic turbulent magnetic fields, we calculated the residence times of cosmic rays in the galactic disk with solving an one dimensional advective-diffusion equation. Consequently, this simple model predicts the observed features including energy dependences of the flux for the all-particle and the components, the knee in the energy spectrum, the chemical composition and the anisotropy, with assuming the parameters for the equations such as the magnetic field strength and the galactic wind velocity.

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