Estimation of composition of cosmic rays with Ezero approximately equals 10(17) - 10(18) eV

Details Estimation of composition of cosmic rays with Ezero approximately equals 10(17) - 10(18) eV Estimation of composition of cosmic rays with Ezero approximately equals 10(17) - 10(18) eV

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....2..186g&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 2 p 186-189 (SEE N85-34006 22-93)

Other

Cerenkov Radiation, Cosmic Ray Showers, Depth Measurement, Energy Spectra, Galactic Radiation, Muons, Cerenkov Counters, Cosmic Rays, Electron Distribution, Flux Density, Variations

Scientific paper

Fluctuations of the shower maximum depth obtained from analysis of electron and muon fluctuations and the extensive air showers (EAS) Cerenkov light on the Yakutsk array data and data of other arrays are considered. On the basis of these the estimation of composition of primaries with E0 = 5.10 to the 17th power eV is received. Estimation of gamma-quanta flux with E0 10 to the 17th power eV is given on the poor-muon showers.

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