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.

doi:10.1134/s1063778820010111

Phys. Atom. Nuclei

2020

DOI: 10.1134/s1063778820010111

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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

V. S. Puchkov

S. E. Pyatovsky

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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

Cited by 1 publication

References 22 publications

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

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

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