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Change in the Mass Composition of Primary Cosmic Radiation at Energies in the Range of $${E_{0}=1}$$–100 PeV According to Data of the KASCADE-Grande Experiment
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
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
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
R. A. Mukhamedshin, V. S. Puchkov, S. E. Pyatovsky and S. B. Shaulov Bulletin of the Lebedev Physics Institute 44(12) 380 (2017) https://doi.org/10.3103/S1068335617120090
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