COMPLEX INSTALLATION HADRON-55 FOR REGISTRATION OF WIDE ATMOSPHERIC SHOWERS
Idrissova T. Sadykov T. Burtebayev N. Ryabov V. Zhukov V.
2021Jagiellonian University
Acta Physica Polonica B, Proceedings Supplement
2021#14Issue 4681 - 686 pp.
Gamma astronomy is the only experimental possibility of local sources specifying high-energy cosmic radiation (1012-1014 eV). In prospect, only neutrino astronomy can supplement the search and study of the galactic and metagalactic objects, where the processes of protons and nuclei acceleration are realized. These processes are accompanied by the generation of gamma quanta and neutrinos, which are not scattered in the magnetic fields of the Universe. Therefore, possibilities of experimental study of the processes and specific stellar objects properties are expanded. Various models and theories of the Universe development are created and tested based on the experimental data obtained in gamma astronomy. Thus, the development of the gamma-astronomical experimental research and observation methods is brought to the fore. The HADRON-55 installation is one of the ground-based gamma-ray detectors that can reliably detect gamma rays with the energies above 1 TeV. In the article, the physical and technical characteristics, the algorithm for registration, and their spatial-energy characteristics of gamma-ray are presented.
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The Institute of Nuclear Physics, Ibragimova 1, Almaty, 050032, Kazakhstan
Satbayev University, Institute of Physics and Technology, Ibragimova 11, Almaty, 050032, Kazakhstan
P.N. Lebedev Physical Institute, The Russian Academy of Sciences, Leninski Prospekt 53, Moscow, Russian Federation
The Institute of Nuclear Physics
Satbayev University
P.N. Lebedev Physical Institute
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