Energy characteristics of gamma-quanta families /the Pamir experiment/

Details Energy characteristics of gamma-quanta families /the Pamir experiment/ Energy characteristics of gamma-quanta families /the Pamir experiment/

Mar 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980izyer..44..450b&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yerevan, Armenian SSR, June 5-7, 1979.) Akademiia Nauk SSSR, Izvestiia, Seri

Computer Science

Cosmic Ray Showers, Energy Spectra, Gamma Ray Spectra, High Altitude Nuclear Detection, High Energy Interactions, Electron Photon Cascades, Quantum Theory, Scintillation Counters

Scientific paper

In the Pamir experiment, X-ray scintillation counters stationed 4350 m above sea level are used to detect gamma rays generated in nuclear and electron-photon cascades in the atmosphere; the purpose of the experiment is to examine ultrahigh-energy strong interactions in cosmic ray showers. This paper examines the energy characteristics of gamma quanta investigated in the Pamir experiment. Measured absolute intensities of gamma-quanta families are compared with calculated values.

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