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Measurement of cosmic-ray origin neutrons using a scintillation detector at the summit of Mt. Fuji (Conference Paper)

机译:使用山顶的闪烁探测器测量宇宙射线起源的中子。富士(会议论文)

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摘要

Cosmic-ray origin neutrons were measured with a scintillation detector at the summit of Mt. Fuji at an altitude of 3776 m during the summer of 2008. The averaged neutron ambient dose equivalent rate converted from the count rates of the detector was 0.47 ± 0.001 μSv h~(-1), which is approximately four times greater than the calculated value of 0.11 ± 0.01 μSv h~(-1). It is postulated that the discrepancy between the measured and calculated neutron ambient dose equivalent rates is on account of the additional charged particle component of the mixed radiation field. To examine the characteristics of the detector at high altitude, a simple model equation which relates the count rates of the detector to the calculated fluence rates of cosmic radiation has been supposed. Based on the model equation it is estimated that the neutron ambient dose equivalent rate would be 0.14 ± 0.04 μSv h~(-1), and the proton contribution would be 0.28 ± 0.03 μSv h~(-1) converted as neutron ambient dose equivalent rate. The results agree to the values of the measured and calculated neutron dose equivalent rates, and the discrepancy between them within the errors.
机译:宇宙射线起源的中子是在山顶用闪烁探测器测量的。 2008年夏季,富士在3776 m的海拔上。从探测器的计数率转换而来的平均中子环境剂量当量率为0.47±0.001μSvh〜(-1),约为计算值的四倍。 0.11±0.01μSvh〜(-1)。假定测量和计算的中子环境剂量当量率之间的差异是由于混合辐射场的附加带电粒子成分引起的。为了检查探测器在高空的特性,已经提出了一个简单的模型方程,该方程将探测器的计数率与计算出的宇宙辐射通量率相关。根据模型方程,估计中子环境剂量当量率为0.14±0.04μSvh〜(-1),质子贡献为0.28±0.03μSvh〜(-1)换算为中子环境剂量当量率。结果与测量和计算的中子剂量当量率的值以及误差之间的差异相符。

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