A giant shower with a primary energy of 10 to the 20th eV recorded at the Yakutsk station

Details A giant shower with a primary energy of 10 to the 20th eV recorded at the Yakutsk station A giant shower with a primary energy of 10 to the 20th eV recorded at the Yakutsk station

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991izssr..55..717g&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Dagomys, USSR, Nov. 1-3, 1990) Akademiia Nauk SSSR, Izvestiia, Seriia Fizich

Physics

Cosmic Ray Showers, Particle Energy, Primary Cosmic Rays, Angular Distribution, Energetic Particles, Energy Spectra, Muons

Scientific paper

An extensive air shower with a primary energy of about 10 to the 20th eV
recorded on May 7, 1989 at the Yakutsk station is briefly characterized.
An analysis of muon contents is presented for air showers covering a
wide range of primary energies and zenith angles.

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