Mass Composition of the Primary Cosmic Rays in the Energy Region 10^{14}-10^{20} eV in Anomalous Diffusion Model

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dc.creatorLagutin, A. A.
dc.creatorRaikin, R. I.
dc.creatorStanovkina, N. V.
dc.creatorTyumentsev, A. G.
dc.creatorMisaki, A.
dc.date2003-06-10
dc.date.accessioned2026-07-07T02:08:44Z
dc.date.available2026-07-07T02:08:44Z
dc.descriptionWe discuss the problem of cosmic ray mass composition variation in wide energy region 10^{14}-10^{20} eV. The mass composition predicted in the framework of recently developed anomalous diffusion model is tested using the results of CORSIKA calculations and experimental data on the depth of maximum of extensive air showers. We show that the model predictions for the mass composition are consistent with observations of different experiments.
dc.description6 pages, 3 figures, 2 tables
dc.identifierhttps://arxiv.org/abs/astro-ph/0306187
dc.identifierhttp://arxiv.org/abs/astro-ph/0306187
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6170
dc.subjectAstrophysics
dc.titleMass Composition of the Primary Cosmic Rays in the Energy Region 10^{14}-10^{20} eV in Anomalous Diffusion Model
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