Primary Heavy Components Spectra and 2-ry/1-ry Ratio Observed by RUNJOB Collaboration

Details Primary Heavy Components Spectra and 2-ry/1-ry Ratio Observed by RUNJOB Collaboration Primary Heavy Components Spectra and 2-ry/1-ry Ratio Observed by RUNJOB Collaboration

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....4.1877f&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

Using all the data with sum of gamma ray energies greater than 5 TeV, we
report the energy spectra of heavy primary cosmic rays from CNO through
iron. Basing on these observations, we construct energy dependence of
B/C and subFe/Fe ratios and will discuss the propagation of cosmic rays
in the galaxy.

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