Depth distribution of the shower maximum at E(0) = 10 to the 18th eV

Details Depth distribution of the shower maximum at E(0) = 10 to the 18th eV Depth distribution of the shower maximum at E(0) = 10 to the 18th eV

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986izssr..50.2166g&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Tbilisi, Georgian SSR, Apr. 1986) Akademiia Nauk SSSR, Izvestiia, Seriia Fiz

Computer Science

2

Cosmic Ray Showers, Maxima, Statistical Distributions, Depth, Muons, Primary Cosmic Rays

Scientific paper

Depth fluctuations of the maximum of cosmic rays showers as determined at the Iakutsk facility are equal to sigma(Xm) = 61 + or - 10 g/sq cm. Specifically, measurements were made of fluctuations of the ratio of the number of muons (at energies greater than 1 GeV) to the number of electrons at a distance 300 m from the shower axis. The form of the Xm distribution is in accordance with the hypothesis of an 80-percent proton composition of primary cosmic rays in the above energy range.

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