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Angular distribution of muons produced by cosmic ray neutrinos in rockMeasurement of the upgoing muons flux, produced by cosmic ray neutrinos is aiming at: (1) search for neutrino oscillation; (2); search for extraterrestrial neutrinos from local sources; and (3); search for any hypothetical neutral penetrating radiation different from neutrinos. Experimental data of the Baksan underground telescope on intensity of upward muons for three years of living time, was analyzed having in mind mainly neutrino oscillation.
Document ID
19850027802
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Boliev, M. M. (Academy of Sciences (USSR) Moscow, Ussr)
Buckevich, A. V. (Academy of Sciences (USSR) Moscow, Ussr)
Chudakov, A. E. (Academy of Sciences (USSR) Moscow, Ussr)
Leonov-Vendrovsky, A. V. (Academy of Sciences (USSR) Moscow, Ussr)
Mikheyev, S. P. (Academy of Sciences (USSR) Moscow, Ussr)
Zakidyshev, V. N. (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-5.3-24
Accession Number
85N36115
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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