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
Author:
Publisher
Allerton Press
Subject
Electronic, Optical and Magnetic Materials
Link
http://link.springer.com/article/10.3103/S1068335617120090/fulltext.html
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Cited by 2 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. 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;Physics of Atomic Nuclei;2021-05
2. 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;Physics of Atomic Nuclei;2020-03
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