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Primary chemical composition from simultaneous recording of muons induced cascades and accompanying muon group undergroundA new method to estimate the mean atomic number of primary cosmic rays in energy range 10 to the 3rd power to 10 to the 5th power Gev/nucleon is suggested. The Baksan underground scintillation telescope data are used for this analysis. The results of 7500 h run of this experiment are presented.
Document ID
19850027762
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Bakatanov, V. N. (Academy of Sciences (USSR) Moscow, Ussr)
Boziev, S. N. (Academy of Sciences (USSR) Moscow, Ussr)
Chudakov, A. E. (Academy of Sciences (USSR) Moscow, Ussr)
Novoseltsev, Y. F. (Academy of Sciences (USSR) Moscow, Ussr)
Novoseltseva, M. V. (Academy of Sciences (USSR) Moscow, Ussr)
Stenkin, Y. F. (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-5.1-13
Accession Number
85N36075
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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