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Peculiarities of gamma-quanta distribution at 20 TeV energyThe angular distribution of protons from the fragmentational region is analyzed. The gamma-quanta families are generated in a dense target by cosmic ray particles at 20 Tev energy. Families were found which had dense groups (spikes) of gamma-quanta where the rapidity/density is 3 times more than the average value determined for all registered families. The experimental data is compared with the results of artificial families simulation.
Document ID
19850027654
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Ermakov, P. M. (Academy of Sciences (USSR) Alma-Ata, Ussr)
Loktionov, A. A. (Academy of Sciences (USSR) Alma-Ata, Ussr)
Lukin, Y. T. (Academy of Sciences (USSR) Alma-Ata, Ussr)
Sadykov, T. K. (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-3.7-10
Accession Number
85N35967
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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