An atmospheric radiation model based on response matrices generated by detailed Monte Carlo Simulations of cosmic ray interactions
Nuclear Science, IEEE Transactions（2004）
摘要
A comprehensive model of the energetic radiation in the atmosphere has been developed. It is based on the use of a dynamic cosmic ray radiation model, an efficient rigidity cutoff calculation tool, and the use of detailed atmospheric response matrices to monochromatic cosmic ray particle incidences. The response matrices were produced by detailed Monte Carlo (MC) simulations of cosmic ray interactions with the atmosphere. This model can predict the secondary particle (proton, neutron, electron, gamma, charged pion, or charged muon) spectrum at any given location and time in the atmosphere.
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关键词
gamma-ray astronomy,secondary particle spectrum,cosmic ray mesons,astronomy computing,cosmic ray electrons,charged muon,Monte Carlo simulations,protons,cosmic ray energy spectra,energetic radiation,atmospheric response matrices,rigidity cutoff calculation tool,cosmic ray protons,electrons,Monte Carlo methods,monochromatic cosmic ray particle incidences,cosmic ray neutrons,atmospheric radiation model,cosmic ray muons,gamma,charged pion,neutrons,dynamic cosmic ray radiation model,cosmic ray interactions
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