Current Status of the High-Energy Ray Observatory

D. M. Podorozhny; D. E. Karmanov; A. D. Panov; L. G. Tkachev; A. N. Turundaevskiy

doi:10.3103/S1062873819050307

Current Status of the High-Energy Ray Observatory

作者: Podorozhny D.M.¹, Karmanov D.E.¹, Panov A.D.¹, Tkachev L.G.², Turundaevskiy A.N.¹
隶属关系:
1. Skobeltsyn Institute of Nuclear Physics, Moscow State University
2. Joint Institute for Nuclear Research
期: 卷 83, 编号 5 (2019)
页面: 637-639
栏目: Article
URL: https://journals.rcsi.science/1062-8738/article/view/187393
DOI: https://doi.org/10.3103/S1062873819050307
ID: 187393

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详细

The aims and scientific tasks of the space High-Energy Ray Observatory experiment are determined. The design of the scientific equipment is described. It is characterized by an unprecedently high geometric factor (~20 m² sr) and fairly high accuracy of measurement. The performance of the equipment allows precise study of cosmic rays in a wide range of energies, including the completely unstudied region of 10¹⁵–10¹⁶ eV. The current status of the space experiment is determined.