Fluctuations of the longitudinal development of extensive air showers and the composition of primary cosmic rays with an energy not less than approximately 10 to the 17th eV

Details Fluctuations of the longitudinal development of extensive air showers and the composition of primary cosmic rays with an energy not less than approximately 10 to the 17th eV Fluctuations of the longitudinal development of extensive air showers and the composition of primary cosmic rays with an energy not less than approximately 10 to the 17th eV

Jul 1985

adsabs.harvard.edu/abs/1985izyak..49.1329g

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, July 1984) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskai

Physics

Cosmic Ray Showers, Particle Flux Density, Primary Cosmic Rays, Spatial Distribution, Approximation, Cerenkov Radiation, Muons

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