Cosmic-Ray Propagation and the Energy Spectra Observed on Earth

Details Cosmic-Ray Propagation and the Energy Spectra Observed on Earth Cosmic-Ray Propagation and the Energy Spectra Observed on Earth

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....4.1941h&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

Scientific paper

We assume that our Galaxy is boundaryless, and both the diffusion coefficient and the gas density depend on the spatial coordinate r(r, z ) in the form of the exponential type, and we take the rigidity dependence of the diffusion coefficient into account, having a form D0 (R) ∝ v Rα . We assume further that the source spectrum has a power-like form in rigidity, ∝ R-γ , and the spatial distribution is also of the exponential type. We present an analytical solution, and compare it with recent data obtained by BESS, RUNJOB and others.

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