Development and structure of extensive air showers at energies above 1 million TeV

Details Development and structure of extensive air showers at energies above 1 million TeV Development and structure of extensive air showers at energies above 1 million TeV

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975izssr..39q1215w&link_type=abstract

(Mezhdunarodnyi Seminar po Izucheniiu Shirokikh Atmosfernykh Livnei Kosmicheskikh Luchei, Moscow, USSR, Oct. 21-23, 1974.) Akade

Physics

Cosmic Ray Showers, Energy Spectra, Primary Cosmic Rays, Spatial Distribution, Cerenkov Radiation, Distribution Functions, Muons, Nuclear Interactions, Proton Energy

Scientific paper

A review of data on extensive air showers generated at particle energies higher than 1 million TeV provides evidence for a faster attenuation of the showers than predicted by models where multiple muon production by nucleon/nucleus interaction varies proportionally to E with an exponent of 1/4. The fluctuations in the showers are found to be greater than expected.

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