Analysis of seasonal variations of the cosmic ray muon flux and neutrons produced by muons in the LVD detector

被引：7

作者：

Agafonova N.Yu. ^{[1
]}

Boyarkin V.V. ^{[1
]}

Dadykin V.L. ^{[1
]}

Dobrynina E.A. ^{[1
]}

Enikeev R.I. ^{[1
]}

Zatsepin G.T. ^{[1
]}

Malgin A.S. ^{[1
]}

Ryazhskaya O.G. ^{[1
]}

Ryasny V.G. ^{[1
]}

Shakiryanova I.R. ^{[1
]}

Yakushev V.F. ^{[1
]}

机构：

[1] Institute for Nuclear Research, Russian Academy of Sciences, Moscow 117312

来源：

Bulletin of the Russian Academy of Sciences: Physics | 2011年 / 75卷 / 3期

关键词：

Muon Flux; White Spirit; Cosmic Muon; Large Volume Detector; Neutron Count Rate;

D O I：

10.3103/S1062873811030063

中图分类号：

学科分类号：

摘要：

The Russian-Italian Large Volume Detector (LVD) is located at the Gran Sasso underground laboratory at a depth of 3300 m w.e. To study the seasonal variations of the penetrating component of cosmic rays, the data on cosmic ray muons detected in 2001-2008 was analyzed, along with those associated with neutrons produced by muons since April 2003. One-year periodic variations of muons and neutrons produced by them were found. The maximum intensity is observed in July, in accord with theoretical concepts. © 2011 Allerton Press, Inc.

引用

页码：427 / 430

页数：3

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