Determination of the mass of primary cosmic radiation from measurements of extensive air showers

Details Determination of the mass of primary cosmic radiation from measurements of extensive air showers Determination of the mass of primary cosmic radiation from measurements of extensive air showers

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975izssr..39q1147w&link_type=abstract

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

Computer Science

Cosmic Ray Showers, Particle Mass, Primary Cosmic Rays, Chemical Composition, Electron Flux Density, Energy Spectra, Muons, Radiation Measurement, Secondary Cosmic Rays

Scientific paper

Some aspects of the application of fragmentation and superposition models to the calculation of the development of extensive air showers are examined. Data on the chemical composition of primary cosmic particles are compared with predictions on the basis of extensive air shower models. A discussion of various shower parameters leads to the conclusion that at least the showers observed at sea level are generated predominantly by protons.

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