Other
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....2..234c&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 2 p 234-237 (SEE N85-34006 22-93)
Other
Cosmic Ray Showers, Energy Spectra, Heavy Nuclei, High Energy Interactions, Primary Cosmic Rays, Protons, Comparison, Ferrous Metals, Iron Isotopes, Proton Beams, Simulation
Scientific paper
Estimation of the relative intensities of protons and heavy nuclei in primary cosmic rays in the energy region 10 to the 15th power approx. 10 to the 17th power eV, was done by a systematic comparison between all available observed data on various parameters of extensive air showers (EAS) and the results of simulation. The interaction model used is an extrapolation of scaling violation indicated by recent pp collider results. A composition consisting of various percentages of Fe in an otherwise pure proton beam was assumed. Greatest overall consistency between the data and the simulation is found when the Fe fraction is in the region of 25%.
Cheung Teddy
MacKeown Kevin P.
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