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Comparison of near-background concentrations of Argon-37 and Xenon-133 in the atmosphere
Journal of Environmental Radioactivity ( IF 2.3 ) Pub Date : 2021-03-30 , DOI: 10.1016/j.jenvrad.2021.106590
B.G. Fritz , ThomasR. Alexander , TheodoreW. Bowyer , JamesC. Hayes , EmilyK. Mace , VincentT. Woods

Radioisotopes of the noble gases xenon and argon can be important indicators of underground nuclear explosions. The Comprehensive Nuclear-Test-Ban Treaty (CTBT) includes monitoring capabilities to identify potential nuclear explosions conducted in violation of the CTBT. This monitoring currently focuses on measurement of the xenon isotopes 131mXe, 133Xe, 133mXe, and 135Xe. However, it is predicted that within 100 days of an underground nuclear explosion (UNE) 37Ar would be released to the atmosphere at higher concentrations than xenon and with a higher signal to background ratio, depending on the radioxenon background levels. Therefore, inclusion of 37Ar measurement capabilities at atmospheric International Monitoring System (IMS) stations may represent an improvement in the capability to detect a nuclear explosion.

At an IMS station location, an understanding of the expected range of background 37Ar activity concentrations is critical to determining what levels would constitute an elevated concentration. This work describes our analysis of atmospheric samples for 37Ar to evaluate the range of background concentrations. Samples were collected at multiple locations withing the United States, with approximately half coming from a sampler co-located with an IMS xenon monitoring station (RN75). The range of 37Ar concentrations measured in atmospheric air samples was relatively narrow; for samples considered detectable, the minimum and maximum measured concentrations were 0.56 and 2.3 mBq/m3, respectively. Comparison of 37Ar and 133Xe concentrations measured at the IMS station indicated some correlation between the measured concentrations. The results presented here demonstrate the capability to detect background concentrations of 37Ar in atmospheric air and provide a basis for potential implementation of 37Ar monitoring at IMS stations.



中文翻译:

大气中Ar-37和Xenon-133的近本底浓度比较

稀有气体氙和氩的放射性同位素可能是地下核爆炸的重要指标。《全面禁止核试验条约》(CTBT)包括监测能力,以查明违反《全面禁试条约》进行的潜在核爆炸。该监视当前集中在氙同位素131m Xe,133 Xe,133m Xe和135 Xe的测量上。但是,据预测,在地下核爆炸(UNE)的100天之内,根据放射性氙的本底水平,会以比氙更高的浓度和更高的信噪比将37 Ar释放到大气中。因此,列入37大气国际监测系统(IMS)站的Ar测量能力可能代表了探测核爆炸能力的提高。

在IMS站位置,了解背景37 Ar活度浓度的预期范围对于确定什么水平会构成升高的浓度至关重要。这项工作描述了我们对37 Ar大气样品的分析,以评估背景浓度的范围。在美国附近的​​多个地方收集了样品,其中大约一半来自与IMS氙气监测站(RN75)并置的采样器。在大气样品中测得的37 Ar浓度范围相对较窄。对于认为可检测的样品,最小和最大测量浓度分别为0.56和2.3 mBq / m 3。比较37在IMS站测得的Ar和133 Xe浓度表明测得的浓度之间存在一定的相关性。此处显示的结果证明了检测大气中37 Ar的背景浓度的能力,并为在IMS站进行37 Ar监测的潜在实施提供了基础。

更新日期:2021-03-31
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