Title of article
Primary proton spectrum around the knee deduced from the emulsion-chamber data obtained at Mts. Fuji and Kanbala
Author/Authors
Huang، نويسنده , , J and Hotta، نويسنده , , N and Kasahara، نويسنده , , K and Ohta، نويسنده , , I and Ozawa، نويسنده , , S and Saito، نويسنده , , T and Shibata، نويسنده , , M and Xu، نويسنده , , X.W and Yuda، نويسنده , , T، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2003
Pages
12
From page
637
To page
648
Abstract
We have done extensive Monte Carlo simulations using the new simulation codes of CORSIKA and COSMOS to compare with the gamma-family data obtained at Mts. Fuji (3750 m above sea level) and Kanbala (5500 m above sea level). Then, we estimated the primary proton and helium spectra around the knee energy region using a multiple-layered feed-forward neural network as a classifier of primary particle kind. The selection efficiency of proton-induced family events is estimated to be 82%. The flux value of protons at 2×1015 eV is (5.5±1.5)×10−14 (m−2 s−1 sr−1 GeV−1). The result suggests heavy-enriched primary composition around the knee region.
Keywords
Cosmic ray , Emulsion chamber , Gamma-family , neural network , Monte Carlo simulation , proton , Knee region
Journal title
Astroparticle Physics
Serial Year
2003
Journal title
Astroparticle Physics
Record number
1328945
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