Gamma-ray families with halos: Main characteristics and possibilities of using them to estimate the p+He fraction in the mass composition of cosmic rays at energies 1–100 PeV

Gamma-ray families with halos: Main characteristics and possibilities of using them to estimate the p+He fraction in the mass composition of cosmic rays at energies 1–100 PeV

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Characteristics of γ-ray families with halos (XREC, Pamir) and data of experiments with EAS are analyzed to estimate the proton and helium (p+He) fractions in the primary cosmic radiation at E0 = 1–100 PeV. It is shown that at energies E0 ∼ 1–100 PeV the fraction of p+He remains significant, namely,...

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Bibliographic Details
Main Authors: Borisov A.S., Denisova V.G., Guseva Z.M., Kanevskaya E.A., Pyatovsky S.E., Kogan M.G., Morozov A.E., Mukhamedshin R.A., Puchkov V.S., Shaulov S.B., Shoziyoev G.P., Smirnova M.D.
Format: Article
Language:English
Published: EDP Sciences 2017-01-01
Series:EPJ Web of Conferences
Online Access:https://doi.org/10.1051/epjconf/201714519008

Internet

https://doi.org/10.1051/epjconf/201714519008

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