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Characteristics of anomalously high multiplicity cosmic ray interactionsSix events with the number of secondaries ranging from 250 to several thousands were registered by an installation consisting of a thin graphite target, above and under which are placed photolayers followed by the usual lead X-ray film and emulsion chambers. Data concerning the number of secondaries and their angular distribution are given. The variance of the angular distribution is compared with data obtained at accelerator energies.
Document ID
19850027607
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Chasnikov, I. Y. (Academy of Sciences (USSR) Alma-Ata, Ussr)
Eremenko, Y. A. (Academy of Sciences (USSR) Alma-Ata, Ussr)
Madigozhin, D. T. (Academy of Sciences (USSR) Alma-Ata, Ussr)
Sadykov, T. K. (Academy of Sciences (USSR) Alma-Ata, Ussr)
Voinov, V. G. (Academy of Sciences (USSR) Alma-Ata, Ussr)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 6
Subject Category
Space Radiation
Report/Patent Number
HE-3.3-1
Accession Number
85N35920
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19850027535Collected WorksNineteenth International Cosmic Ray Conference. HE Sessions, Volume 6
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