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arXiv 1104.2157astro-ph.IM
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用于测量地下场所大气μ介子通量的移动探测器

A mobile detector for measurements of the atmospheric muon flux in underground sites

Bogdan Mitrica, Romul Margineanu, Sabin Stoica, Mirel Petcu, Iliana Brancus, Alexandru Jipa, Ionel Lazanu, Octavian Sima, Andreas Haungs, Heinigerd Rebel, Maria… 展开作者

Bogdan Mitrica, Romul Margineanu, Sabin Stoica, Mirel Petcu, Iliana Brancus, Alexandru Jipa, Ionel Lazanu, Octavian Sima, Andreas Haungs, Heinigerd Rebel, Marian Petre, Gabriel Toma, Alexandra Saftoiu, Denis Stanca, Ana Apostu, Claudia Gomoiu

摘要:

μ子是空气中天然辐射剂量的重要组成部分(约为1000)。30 nSv/h),以及在地下场址,即使通量和相对贡献显著降低。在地下观测到的μ介子通量可以作为地下场地深度的估计值,单位为mwe(米水当量)。等效水深是设计物理实验方案的重要依据。布加勒斯特IFIN-HH开发了一个用于测量μ介子通量的移动探测器。由2个闪烁体板组成(约0.9 m2)的同时测量,探测器安装在货车上,这有助于在地面或地下的不同位置进行测量。探测器被用来确定在罗马尼亚不同地点的μ介子通量。特别是,从罗马尼亚Slanic Prahova盐矿的几个地点采集数据并评估了水表水当量值。在Slanic矿不同深度的2个不同坑道中进行了测量。为了检验该方法的稳定性,还进行了不同海拔高度地面μ子通量的测量。结果进行了比较,预测的蒙特卡罗模拟使用CORSIKA和MUSIC代码。

英文摘要:

Muons comprise an important contribution of the natural radiation dose in air (approx. 30 nSv/h of a total dose rate of 65-130 nSv/h), as well as in underground sites even when the flux and relative contribution are significantly reduced. The flux of the muons observed in underground can be used as an estimator for the depth in mwe (meter water equivalent) of the underground site. The water equivalent depth is an important information to devise physics experiments feasible for a specific site. A mobile detector for performing measurements of the muon's flux was developed in IFIN-HH, Bucharest. Consisting of 2 scintillator plates (approx. 0.9 m2) which measure in coincidence, the detector is installed on a van which facilitates measurements at different locations at surface or underground. The detector was used to determine muon fluxes at different sites in Romania. In particular, data were taken and the values of meter water equivalents were assessed for several locations from the salt mine from Slanic Prahova, Romania. The measurements have been performed in 2 different galleries of the Slanic mine at different depths. In order to test the stability of the method, also measure- ments of the muon flux at surface at different elevations were performed. The results were compared with predictions of Monte-Carlo simulations using the CORSIKA and MUSIC codes.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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