Composition of primary cosmic rays above 10 to the 13th eV from the study of time distributions of energetic hadrons near air-shower cores

Details Composition of primary cosmic rays above 10 to the 13th eV from the study of time distributions of energetic hadrons near air-shower cores Composition of primary cosmic rays above 10 to the 13th eV from the study of time distributions of energetic hadrons near air-shower cores

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979phrvl..42..854g&link_type=ejournal

Physical Review Letters, vol. 42, Mar. 26, 1979, p. 854-857.

Physics

Nuclear Physics

36

Cosmic Ray Showers, Elementary Particles, Hadrons, High Energy Interactions, Primary Cosmic Rays, Time Lag, Composition (Property), Ionizing Radiation, Monte Carlo Method, Nuclei (Nuclear Physics)

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