Energy characteristics of gamma-quanta families with a total energy above 30 TeV - Experiment Pamir

Details Energy characteristics of gamma-quanta families with a total energy above 30 TeV - Experiment Pamir Energy characteristics of gamma-quanta families with a total energy above 30 TeV - Experiment Pamir

Jul 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978izyak..42.1346b&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, June 1977.) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheska

Physics

Cosmic Ray Showers, Electron Photon Cascades, Energy Spectra, Gamma Rays, Energetic Particles, Mountains, Spectral Energy Distribution

Scientific paper

Several hundred groups of electron-photon cascades (so-called gamma-quanta families) were detected and measured at high-altitude stations in the Pamir mountain range. In the present paper, it is shown that at a constant relative threshold, the energy spectrum of particles in cascades with a total energy above 30 TeV changes with increasing total energy.

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