Barometric Effect of High-Energy Muons (> 230 GeV)

M. Berkova; V. Yanke; L. Dorman; V. Petkov; M. Kostyuk; R. Novoseltseva; Yu. Novoseltsev; P. Striganov; M. Boliev; V. Volchenko; G. Volchenko; A. Yanin; I. Dzaparova; M. Kochkarov

arXiv · 1402.1183

Barometric Effect of High-Energy Muons (> 230 GeV)

M. Berkova·V. Yanke·L. Dorman·V. Petkov·M. Kostyuk·R. Novoseltseva·Yu. Novoseltsev·P. Striganov·M. Boliev·V. Volchenko·G. Volchenko·A. Yanin·I. Dzaparova·M. Kochkarov

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Abstract

According to the Baksan underground scintillation telescope data the barometric coefficients for six intervals of zenith angles of particle registration were obtained for ten years (2003-2012). The obtained barometric coefficients exceed an order of magnitude the theoretical values. Nevertheless, these results are in good agreement with the data obtained for the barometric effect of high-energy muons in a number papers of other authors. And there is a noticeable increase of the absolute values of the measured barometric coefficients with increase of the threshold energy of muons.

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M. Berkova, V. Yanke, L. Dorman, V. Petkov, M. Kostyuk, R. Novoseltseva, Yu. Novoseltsev, P. Striganov, M. Boliev, V. Volchenko, G. Volchenko, A. Yanin, I. Dzaparova, M. Kochkarov. 2014-02-05. Barometric Effect of High-Energy Muons (> 230 GeV). https://arxiv.org/abs/1402.1183

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