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Monitoring temporal opacity fluctuations of large structures with muon radiography: a calibration experiment using a water tower

机译:用μ子射线照相术监测大型结构的时间不透明性波动:使用水塔的校准实验

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摘要

Usage of secondary cosmic muons to image the geological structures density distribution significantly developed during the past ten years. Recent applications demonstrate the method interest to monitor magma ascent and volcanic gas movements inside volcanoes. Muon radiography could be used to monitor density variations in aquifers and the critical zone in the near surface. However, the time resolution achievable by muon radiography monitoring remains poorly studied. It is biased by fluctuation sources exterior to the target, and statistically affected by the limited number of particles detected during the experiment. The present study documents these two issues within a simple and well constrained experimental context: a water tower. We use the data to discuss the influence of atmospheric variability that perturbs the signal, and propose correction formulas to extract the muon flux variations related to the water level changes. Statistical developments establish the feasibility domain of muon radiography monitoring as a function of target thickness (i.e. opacity). Objects with a thickness comprised between ≈50 ± 30 m water equivalent correspond to the best time resolution. Thinner objects have a degraded time resolution that strongly depends on the zenith angle, whereas thicker objects (like volcanoes) time resolution does not.
机译:在过去的十年中,利用二次宇宙μ子成像地质结构的密度分布有了很大的发展。最近的应用表明,该方法对监测火山内部的岩浆上升和火山气体运动很感兴趣。 Muon射线照相术可用于监测含水层和近地表关键区域的密度变化。然而,通过μ子射线照相监测可实现的时间分辨率仍然研究不足。它受到目标外部波动源的偏见,并且在统计上受到实验过程中检测到的有限数量颗粒的影响。本研究在简单且受严格限制的实验环境中记录了这两个问题:水塔。我们使用这些数据讨论扰动信号的大气变化的影响,并提出校正公式以提取与水位变化有关的μ子通量变化。统计的发展确定了μ子射线照相监测的可行性范围与目标厚度(即不透明度)的函数关系。厚度在约50±30微米水当量之间的物体对应于最佳时间分辨率。较薄的对象的时间分辨率会降低,这在很大程度上取决于天顶角,而较厚的对象(例如火山)的时间分辨率则不会。

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