Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
Optimisation studies of the TAIGA-Muon scintillation detector array. / TAIGA Collaboration.
в: Journal of Instrumentation, Том 17, № 6, P06022, 01.06.2022.Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
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TY - JOUR
T1 - Optimisation studies of the TAIGA-Muon scintillation detector array
AU - the TAIGA Collaboration
AU - Astapov, I.
AU - Bezyazeekov, P.
AU - Blank, M.
AU - Bonvech, E.
AU - Borodin, A.
AU - Brueckner, M.
AU - Budnev, N.
AU - Bulan, A.
AU - Chernov, D.
AU - Chiavassa, A.
AU - Dyachok, A.
AU - Gafarov, A.
AU - Garmash, A.
AU - Grebenyuk, V.
AU - Gress, E.
AU - Gress, O.
AU - Gress, T.
AU - Grinyuk, A.
AU - Grishin, O.
AU - Horns, D.
AU - Igoshin, A.
AU - Ivanova, A. D.
AU - Ivanova, A. L.
AU - Kalmykov, N.
AU - Kindin, V.
AU - Kiryuhin, S.
AU - Kokoulin, R.
AU - Kompaniets, K.
AU - Korosteleva, E.
AU - Kozhin, V.
AU - Kravchenko, E.
AU - Kryukov, A.
AU - Kuzmichev, L.
AU - Lagutin, A.
AU - Lavrova, M.
AU - Lemeshev, Y.
AU - Lubsandorzhiev, B.
AU - Lubsandorzhiev, N.
AU - Lukanov, A.
AU - Lukyantsev, D.
AU - Malakhov, S.
AU - Mirgazov, R.
AU - Mirzoyan, R.
AU - Monkhoev, R.
AU - Osipova, E.
AU - Pakhorukov, A.
AU - Pan, A.
AU - Pankov, L.
AU - Sokolov, A.
AU - Vaidyanathan, A.
N1 - Publisher Copyright: © 2022 IOP Publishing Ltd and Sissa Medialab.
PY - 2022/6/1
Y1 - 2022/6/1
N2 - The TAIGA astroparticle observatory is progressing with the deployment of new detector stations. The Tunka-Grande - scintillation counter array of the observatory expands with the new TAIGA-Muon stations. Several simulation studies were conducted for optimisation of the new station positioning and performance. Extensive air showers induced by gamma quanta or a proton in the range from 100 TeV to 1 PeV at a zenith angle of 0° were used for these studies. Based on the developed simulation, the capabilities of identification of high energy extensive air showers were studied. The soil thickness, the detector and station positions, the lowest measurable energy range of the cosmic rays, and different methods of air shower identification were investigated.
AB - The TAIGA astroparticle observatory is progressing with the deployment of new detector stations. The Tunka-Grande - scintillation counter array of the observatory expands with the new TAIGA-Muon stations. Several simulation studies were conducted for optimisation of the new station positioning and performance. Extensive air showers induced by gamma quanta or a proton in the range from 100 TeV to 1 PeV at a zenith angle of 0° were used for these studies. Based on the developed simulation, the capabilities of identification of high energy extensive air showers were studied. The soil thickness, the detector and station positions, the lowest measurable energy range of the cosmic rays, and different methods of air shower identification were investigated.
KW - Detector modelling and simulations I (interaction of radiation with matter, interaction of photons with matter, interaction of hadrons with matter, etc)
KW - Particle detectors
KW - Particle identification methods
KW - Scintillators, scintillation and light emission processes (solid, gas and liquid scintillators)
UR - http://www.scopus.com/inward/record.url?scp=85133009847&partnerID=8YFLogxK
U2 - 10.1088/1748-0221/17/06/P06022
DO - 10.1088/1748-0221/17/06/P06022
M3 - Article
AN - SCOPUS:85133009847
VL - 17
JO - Journal of Instrumentation
JF - Journal of Instrumentation
SN - 1748-0221
IS - 6
M1 - P06022
ER -
ID: 36495958