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Электронный каталог: Vaidyanathan, A. - A Combined Study of HiSCORE and TAIGA Scintillation Detector Array for the Identification of EASs
Vaidyanathan, A. - A Combined Study of HiSCORE and TAIGA Scintillation Detector Array for the Identification of EASs
Книга (аналит. описание)
Автор: Vaidyanathan, A.
38th International Cosmic Ray Conference (ICRC2023), Nagoya, Japan, 26 July - 3 August, 2023 [Electronic resource]: A Combined Study of HiSCORE and TAIGA Scintillation Detector Array for the Identification of EASs
б.г.
ISBN отсутствует
Автор: Vaidyanathan, A.
38th International Cosmic Ray Conference (ICRC2023), Nagoya, Japan, 26 July - 3 August, 2023 [Electronic resource]: A Combined Study of HiSCORE and TAIGA Scintillation Detector Array for the Identification of EASs
б.г.
ISBN отсутствует
Книга (аналит. описание)
Vaidyanathan, A.
A Combined Study of HiSCORE and TAIGA Scintillation Detector Array for the Identification of EASs / A.Vaidyanathan, E.Kravchenko, A.Borodin, V.Grebenyuk, A.Grinyuk, M.Lavrova, A.Pan, I.Satyshev, L.Tkachev, [a.o.] // 38th International Cosmic Ray Conference (ICRC2023), Nagoya, Japan, 26 July - 3 August, 2023 [Electronic resource]. – Trieste : SISSA, 2024. – P. 260. – URL: https://doi.org/10.22323/1.444.0260. – Bibliogr.: 10.
The TAIGA experiment in Tunka Valley is expanding the present scintillation detector array with new TAIGA-Muon detector stations. A simulation model was developed to optimise the layout of the new stations and study the identification performance of the array. The extensive air showers (EASs) were simulated with the CORSIKA simulation tool, and the detector response was simulated with the GEANT4 package. The EASs induced by gamma quanta or proton, Helium, Carbon, Nitrogen, Oxygen, Iron in the energy range of 1 PeV and the zenith angle range from 0°to 45°, are used for these studies. For the identification of high-energy extensive air showers, a method based on a neural network was suggested. With this method, the proton identification efficiency is more than 99.9%, while the gamma identification efficiency is not less than 50% – (Proceedings of Science ; Vol. 444) .
ОИЯИ = ОИЯИ (JINR)2024
Спец.(статьи,препринты) = С 347 - Космические лучи
Спец.(статьи,препринты) = С 63 - Астрофизика$
Спец.(статьи,препринты) = С 344.1ж - Сцинтилляционные счетчики, камеры. Сцинтилляционные вещества. Микроканальные умножители
Vaidyanathan, A.
A Combined Study of HiSCORE and TAIGA Scintillation Detector Array for the Identification of EASs / A.Vaidyanathan, E.Kravchenko, A.Borodin, V.Grebenyuk, A.Grinyuk, M.Lavrova, A.Pan, I.Satyshev, L.Tkachev, [a.o.] // 38th International Cosmic Ray Conference (ICRC2023), Nagoya, Japan, 26 July - 3 August, 2023 [Electronic resource]. – Trieste : SISSA, 2024. – P. 260. – URL: https://doi.org/10.22323/1.444.0260. – Bibliogr.: 10.
The TAIGA experiment in Tunka Valley is expanding the present scintillation detector array with new TAIGA-Muon detector stations. A simulation model was developed to optimise the layout of the new stations and study the identification performance of the array. The extensive air showers (EASs) were simulated with the CORSIKA simulation tool, and the detector response was simulated with the GEANT4 package. The EASs induced by gamma quanta or proton, Helium, Carbon, Nitrogen, Oxygen, Iron in the energy range of 1 PeV and the zenith angle range from 0°to 45°, are used for these studies. For the identification of high-energy extensive air showers, a method based on a neural network was suggested. With this method, the proton identification efficiency is more than 99.9%, while the gamma identification efficiency is not less than 50% – (Proceedings of Science ; Vol. 444) .
ОИЯИ = ОИЯИ (JINR)2024
Спец.(статьи,препринты) = С 347 - Космические лучи
Спец.(статьи,препринты) = С 63 - Астрофизика$
Спец.(статьи,препринты) = С 344.1ж - Сцинтилляционные счетчики, камеры. Сцинтилляционные вещества. Микроканальные умножители