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EAS accompanied by gamma-families at Mt. Norikura and comparison with Monte Carlo simulationThe experimental data of extensive air showers (EAS) accompanied by gamma-families, with total energy greater than 10 TeV, were compared with a Monte Carlo simulation with a rising cross section proportional to E sup 0.04 for the p-air inelastic cross section. It is found that the absolute intensity of size spectrum of such EAS is strongly affected by the primary protons intensity at 10 to the 15th power approx. 10 to the 16th power eV region and the experimental size spectrum agrees with the simulated spectra for the p-poor primary composition better than the p-rich one.
Document ID
19850027615
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Shima, M.
(Konan Univ. Kobe, Japan)
Saito, T.
(Konan Univ. Kobe, Japan)
Sakata, M.
(Konan Univ. Kobe, Japan)
Yamamoto, Y.
(Konan Univ. Kobe, Japan)
Kasahara, K.
(Tokyo Univ. Tanashi, Japan)
Yuda, T.
(Tokyo Univ. Tanashi, Japan)
Torii, S.
(Kanagawa Univ. Yokohama, United States)
Hotta, N.
(Utsunomiya Univ.)
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-3.3-10
Accession Number
85N35928
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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