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Pis'ma v Zhurnal Èksperimental'noi i Teoreticheskoi Fiziki, 2023, Volume 118, Issue 3, Pages 159–165
DOI: https://doi.org/10.31857/S123456782315003X (Mi jetpl7001) 		 
FIELDS, PARTICLES, AND NUCLEI

Effect of meteorological parameters on the cosmic muon flux studied using the effective generation level method with the DANSS detector data

I. G. Alekseevab, V. V. Belovc, M. V. Danilovb, I. V. Zhitnikovc, D. R. Zinatulinacd, S. V. Kazartsevc, A. S. Kobyakinaeb, A. S. Kuzntesovc, I. V. Machikhilyanf, D. V. Medvedevc, V. M. Nesterova, D. V. Ponomarevc, I. E. Rozovac, N. S. Rumyantsevacg, V. Yu. Rusinova, E. I. Samigullinab, D. N. Sviridaab, N. A. Skrobovaab, E. I. Tarkovskya, D. V. Filosofovc, M. V. Fominac, E. A. Shevchikc, M. V. Shirchenkoc, Yu. A. Shitovc, A. E. Yakovlevab, E. A. Yakushevc

a National Research Center Kurchatov Institute, Moscow, 123182 Russia
b Lebedev Physical Institute, Moscow, 119991 Russia
c Joint Institute for Nuclear Research, Dubna, Moscow region, 141980 Russia
d Voronezh State University, Voronezh, 394018 Russia
e Moscow Institute of Physics and Technology (National Research University), Dolgoprudnyi, Moscow region, 141701 Russia
f Dukhov All-Russia Research Institute of Automatics, Moscow, 127055 Russia
g Dubna State University, Dubna, Moscow region, 141982 Russia
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DOI: https://doi.org/10.31857/S123456782315003X
Abstract: The DANSS detector is located directly under the nuclear reactor at the Kalinin nuclear power plant. Such a position ensures about 50 m.w.e. shielding from cosmic rays in the vertical direction; as a result, the detector occupies an intermediate position between surface and underground detectors in the shielding from cosmic rays. The sensitive volume of the detector consisting of a 1-m$^3$ plastic scintillator is surrounded by the multilayer passive shielding and muon veto. The main aim of the DANSS experiment is to measure the antineutrino spectrum at various distances from the source. To this end, the detector is placed on a lifting platform in order to record data at three positions of 10.9, 11.9, and 12.9 m from the reactor core. The detector can reconstruct muon tracks passing through its sensitive volume. The pressure, temperature, and decay coefficients for muons in various regions of the zenith angle $\theta $ have been determined from the muon data collected during four years using the effective generation level method.
Funding agency Grant number
State Atomic Energy Corporation ROSATOM Н.4х.44.90.13.1119
Н.4х.44.9Б.16.1006
Russian Science Foundation 17-12-01145
23-12-00085
This work was supported by the State Atomic Energy Corporation Rosatom (state contract nos. N.4x.44.90.13.1119 and N.4x.44.9B.16.1006 for the construction of the DANSS setup in 2013-2016) and by the Russian Science Foundation (project no. 17-12-01145, the long-term operation of the detector, the acquisition and processing of experimental data in 2017-021, and project no. 23-12-00085, the analysis of the data).
Received: 04.07.2023
Revised: 04.07.2023
Accepted: 06.07.2023
English version:
Journal of Experimental and Theoretical Physics Letters, 2023, Volume 118, Issue 3, Pages 165–171
DOI: https://doi.org/10.1134/S0021364023602166
Bibliographic databases:
Document Type: Article
Language: Russian
Citation: I. G. Alekseev, V. V. Belov, M. V. Danilov, I. V. Zhitnikov, D. R. Zinatulina, S. V. Kazartsev, A. S. Kobyakin, A. S. Kuzntesov, I. V. Machikhilyan, D. V. Medvedev, V. M. Nesterov, D. V. Ponomarev, I. E. Rozova, N. S. Rumyantseva, V. Yu. Rusinov, E. I. Samigullin, D. N. Svirida, N. A. Skrobova, E. I. Tarkovsky, D. V. Filosofov, M. V. Fomina, E. A. Shevchik, M. V. Shirchenko, Yu. A. Shitov, A. E. Yakovleva, E. A. Yakushev, “Effect of meteorological parameters on the cosmic muon flux studied using the effective generation level method with the DANSS detector data”, Pis'ma v Zh. Èksper. Teoret. Fiz., 118:3 (2023), 159–165; JETP Letters, 118:3 (2023), 165–171
Citation in format AMSBIB
\Bibitem{AleBelDan23}
\by I.~G.~Alekseev, V.~V.~Belov, M.~V.~Danilov, I.~V.~Zhitnikov, D.~R.~Zinatulina, S.~V.~Kazartsev, A.~S.~Kobyakin, A.~S.~Kuzntesov, I.~V.~Machikhilyan, D.~V.~Medvedev, V.~M.~Nesterov, D.~V.~Ponomarev, I.~E.~Rozova, N.~S.~Rumyantseva, V.~Yu.~Rusinov, E.~I.~Samigullin, D.~N.~Svirida, N.~A.~Skrobova, E.~I.~Tarkovsky, D.~V.~Filosofov, M.~V.~Fomina, E.~A.~Shevchik, M.~V.~Shirchenko, Yu.~A.~Shitov, A.~E.~Yakovleva, E.~A.~Yakushev
\paper Effect of meteorological parameters on the cosmic muon flux studied using the effective generation level method with the DANSS detector data
\jour Pis'ma v Zh. \`Eksper. Teoret. Fiz.
\yr 2023
\vol 118
\issue 3
\pages 159--165
\mathnet{http://mi.mathnet.ru/jetpl7001}
\crossref{https://doi.org/10.31857/S123456782315003X}
\edn{https://elibrary.ru/hwoixw}
\transl
\jour JETP Letters
\yr 2023
\vol 118
\issue 3
\pages 165--171
\crossref{https://doi.org/10.1134/S0021364023602166}
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