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Muon groups and primary composition at 10 to the 13th power to 10 to the 15th power eVThe data on muon groups observed at Baksan underground scintillation telescope is analyzed. In this analysis we compare the experimental data with calulations, based on a superposition model in order to obtain the effective atomic number of primary cosmic rays in the energy range 10 to the 13th power to 10 to the 15th power eV.
Document ID
19850027761
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Budko, E. V. (Academy of Sciences (USSR) Moscow, Ussr)
Chudakov, A. E. (Academy of Sciences (USSR) Moscow, Ussr)
Dogujaev, V. A. (Academy of Sciences (USSR) Moscow, Ussr)
Mihelev, A. R. (Academy of Sciences (USSR) Moscow, Ussr)
Padey, V. A. (Academy of Sciences (USSR) Moscow, Ussr)
Petkov, V. A. (Academy of Sciences (USSR) Moscow, Ussr)
Striganov, P. S. (Academy of Sciences (USSR) Moscow, Ussr)
Suvorova, O. V. (Academy of Sciences (USSR) Moscow, Ussr)
Voevodsky, A. V. (Academy of Sciences (USSR) Moscow, Ussr)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 8
Subject Category
Space Radiation
Report/Patent Number
HE-5.1-12
Accession Number
85N36074
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19850027753Collected WorksNineteenth International Cosmic Ray Conference. HE Sessions, Volume 8
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