Physics
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....4.1933p&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
2
Scientific paper
The random nature of cosmic ray (CR) sources leads to the fluctuations of CR intensity in space and time. We calculate the expected fluctuations in a flathalo diffusion model for particles with energies from 1 to 103 TeV. The data on CR spectrum and anisotropy, and the astronomical data on supernova remnants, the potential sources of CRs, can be used to constrain the value of CR diffusion coefficient and its dependence on energy.
Jones Frank C.
Ptuskin Vladimir S.
Seo Eun-Suk
Sina Ramin
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