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Estimation of composition of cosmic rays with E sub zero approximately equals 10(17) - 10(18) eVFluctuations 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 E sub 0 = 5.10 to the 17th power eV is received. Estimation of gamma-quanta flux with E sub 0 10 to the 17th power eV is given on the poor-muon showers.
Document ID
19850025742
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Glushkov, A. V. (Academy of Sciences (USSR) Yakutsk, Ussr)
Efimov, N. N. (Academy of Sciences (USSR) Yakutsk, Ussr)
Efremov, N. N. (Academy of Sciences (USSR) Yakutsk, Ussr)
Makarov, I. T. (Academy of Sciences (USSR) Yakutsk, Ussr)
Pravdin, M. I. (Academy of Sciences (USSR) Yakutsk, Ussr)
Dedenko, L. I. (Moscow State Univ.)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 2
Subject Category
Space Radiation
Report/Patent Number
OG-5.1-14
Accession Number
85N34055
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19850025693Collected WorksNinteenth International Cosmic Ray Conference. OG Sessions, Volume 2
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