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Theory of fluctuations of extended air showersThe Monte Carlo method was used to calculate the probability distribution functions of shower characteristics for primary protons at sea level. The calculation was based on the following model of the elementary event: the interaction paths are 90 g/sq cm for nucleons and 120 g/sq cm for pions. The nonelasticity coefficient for nucleons is uniformly distributed between 0.1 and 0.9, and for pions it is equal to 1. Isobaric pions are taken into account. The spectra of secondary particles were determined using Cocconi's approximation formula. The calculation for the nuclei was carried out on the assumption of a breakup of the nucleus into component nucleons. The mean number of particles and the variances of the distributions for electrons when the number of muons was fixed, and for muons when the number of electrons was fixed, were calculated.
Document ID
19750008427
Acquisition Source
Legacy CDMS
Document Type
Book
Authors
Dedenko, L. G.
(Kanner (Leo) Associates Redwood City, CA, United States)
Date Acquired
August 8, 2013
Publication Date
January 1, 1975
Publication Information
Publication: Cosmic Rays (NASA-TT-F-807)
Subject Category
Space Radiation
Accession Number
75N16499
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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