Features of the zenith-angle dependence of the rho600 and S600 parameters of the Haver Park and Iakutsk EAS facilities

Details Features of the zenith-angle dependence of the rho600 and S600 parameters of the Haver Park and Iakutsk EAS facilities Features of the zenith-angle dependence of the rho600 and S600 parameters of the Haver Park and Iakutsk EAS facilities

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986izssr..50.2172g&link_type=abstract

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

Physics

Angular Distribution, Cosmic Ray Showers, Energy Spectra, Zenith, Cerenkov Counters, Depth, Muons, Scintillation Counters

Scientific paper

An analysis of intense showers in the Catalogue of highest cosmic rays (Watson et al., 1980) shows that, at energies above 10 to the 19th eV, the rho600 parameter has a maximum in the zenith-angle range of 30-35 deg. For this reason, a standard formula for determining rho300 for oblique showers is inapplicable. The utilization of this formula leads to an overly high value of rho600.

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