S. E. Pyatovsky - Lebedev Physical Institute, Russian Academy of Sciences

S. K. Shinbulatov, N. O. Saduev, O. A. Kalikulov, Y. S. Mukhamejanov, Sh. Utey, A. I. Zhumabayev, N. O. Yerezhep, D. Beznosko, J. K. Jhanceitova, R. A. Nam, V. V. Piskal, A. V. Stepanov, L. I. Vildanova, V. V. Zhukov, K. V. Cherdyntceva, V. G. Denisova, E. Kanevskay,N. M. Nesterova,V. S. Puchkov,S. E. Pyatovsky,V. A. Ryabov, A. L. Schepetov, M. D. Smirnova, S. B. Shaulov

36TH INTERNATIONAL COSMIC RAY CONFERENCE, ICRC2019 (2021)

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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

Puchkov V. S.,Pyatovsky S. E.

Physics of atomic nucleino. 2 (2020): 237-246

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Estimation of the p plus He Fraction in the Mass Composition of Primary Cosmic Radiation the Energy Range of E₀=1-100 PeV according to Gamma-Ray Families Featuring Halo

V. S. Puchkov,S. E. Pyatovsky

PHYSICS OF ATOMIC NUCLEIno. 2 (2020): 237-246

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The fraction of light nuclei in the mass composition of primary cosmic radiation at E0=1-100 PeV

Pyatovsky S. E.