The spectrum of superhigh-energy extensive air showers and its irregularity at energies greater than approximately 10 to the 19th eV

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Cosmic Ray Showers, High Energy Interactions, Particle Flux Density, Spectrum Analysis, Cerenkov Radiation, Energy Spectra, Primary Cosmic Rays

Scientific paper

EAS spectra are examined for particle flux densities of rho-600 (at a distance of 600 m from the shower axis), atmospheric Cerenkov light (at a distance of 400 m from the shower axis), and the primary-particle energy spectrum in the range of 3 x 10 to the 17th to 10 to the 20th eV. The study is performed on the basis of a large volume of shower statistics, a method relying on the complete simulation of EAS development and measurements at the Iakutsk station.

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