Dependence of the position of the EAS maximum on primary-particle energy

Details Dependence of the position of the EAS maximum on primary-particle energy Dependence of the position of the EAS maximum on primary-particle energy

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985izyak..49.1307a&link_type=abstract

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

Physics

Cosmic Ray Showers, Electron Photon Cascades, Particle Energy, Primary Cosmic Rays, Cerenkov Radiation, Electron Distribution, Maxima

Scientific paper

An improved method for the processing of experimental data is proposed to explain discrepancies in the determination of the maximum depth of the development of extensive air showers as a function of primary-particle energy. This method involves: (1) detailed modeling of the shower-sampling process and (2) an improved calculation of the dependence of the halfwidth of the Cerenkov-radiation pulse on the position of the shower maximum.

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