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Electrons, muons and hadrons in extensive air showers and how do they depend on nuclear interaction model, part 1Monte Carlo simulations of extensive air showers were performed using a couple of different nuclear interaction models and obtaining a variety of shower characteristics. The discussion of these shows that the sensitivity of observables to the primary mass spectrum is significantly stronger than to the interaction model, the latter being quite weak.
Document ID
19850027659
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Wrotniak, J. A.
(Maryland Univ. College Park, MD, United States)
Yodh, G. B.
(Maryland Univ. College Park, MD, United States)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 7
Subject Category
Space Radiation
Accession Number
85N35972
Funding Number(s)
CONTRACT_GRANT: NSF PHY-82-07425
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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