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 ,
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