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EPJ Web of Conferences 145 19008 (2017)
DOI: 10.1051/epjconf/201614519008
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Estimation of the $$\boldsymbol{p+\textrm{He}}$$ Fraction in the Mass Composition of Primary Cosmic Radiation the Energy Range of $$\boldsymbol{E_{0}=1}$$–100 PeV according to Gamma-Ray Families Featuring Halo

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γ-families with halos observed by X-ray emulsion chamber in EAS and the estimate of the p+He fraction in primary cosmic rays at E0 = 1–100 PeV

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Spectra of Protons and Alpha Particles and Their Comparison in the NUCLEON Experiment Data

D. E. Karmanov, I. M. Kovalev, I. A. Kudryashov, A. A. Kurganov, A. D. Panov, D. M. Podorozhny, A. N. Turundaevskiy and O. A. Vasiliev
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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

A.S. Borisov, V.G. Denisova, Z.M. Guseva, E.A. Kanevskaya, S.E. Pyatovsky, M.G. Kogan, A.E. Morozov, R.A. Mukhamedshin, V.S. Puchkov, S.B. Shaulov, G.P. Shoziyoev, M.D. Smirnova and B. Pattison
EPJ Web of Conferences 145 19008 (2017)
DOI: 10.1051/epjconf/201714519008
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