Clouvas A, Leontaris F, Xanthos S, Hadjileontiadis L
Department of Electrical and Computer Engineering, Aristotle University of Thessaloniki, GR-54124 Thessaloniki, Greece
Department of Electrical and Computer Engineering, Aristotle University of Thessaloniki, GR-54124 Thessaloniki, Greece.
Radiat Prot Dosimetry. 2016 Dec;172(4):501-509. doi: 10.1093/rpd/ncv513. Epub 2015 Dec 24.
Gamma radiation measurements were performed during the last 27 y, starting from 1988, with a NaI(Tl)-based Xetex 501A radiation monitor located outside the Nuclear Technology Laboratory of the Aristotle University of Thessaloniki in Northern Greece, and a time series was created. Measurements were also performed in the same place during 1995-98 and 2013-15 with portable high purity germanium (HPGe) detector. The total absorbed dose rate in air decreases exponentially with time. The total absorbed dose rate in air is the sum of the gamma dose rates due to (1) uranium series, (2) thorium series, (3) K and (4) Cs (due to the Chernobyl accident). In addition, a small contribution due to cosmic radiation is measured by the radiation monitor. From the time-dependence measurements with the HPGe detector, it was found that the time dependence of the absorbed gamma dose rate in air due to (1) uranium series, (2) thorium series and (3) K is quite constant. On the contrary, gamma dose rate due to Cs decreases exponentially with an effective half-life (t) of ∼13.5 y, stronger than expected due to the natural decay of Cs. Time series analysis of the mean monthly total absorbed dose rate in air was performed. Fourier analysis reveals several periodicities, and applying Zhao-Atlas-Marks transform unravels the time distribution of those periodicities. There are three main discernible periodicities: 12 ± 0.2, 42.3 ± 2.9 and 53.2 ± 3.2 months. One of them is of a seasonal character (annual cycle) and can be linked to seasonal atmospheric variations and is strongly visible from 1988 to 2002 and 2008 to 2014. The other two (42.3 ± 2.9 and 53.2 ± 3.2 months) were found to be also related to meteorological parameters (air temperature), and they were very intense during the years 2002-4 when the annual periodicity was weak. Apart from the three main periodicities, there are also four others (14.7, 18.6, 21.3 and 27.3 months) with lower magnitudes; of which, three agree well with literature data periodicities in solar activity. Different possible mechanisms that can influence the gamma radiation measurements, due to solar activity, were discussed.
伽马辐射测量始于1988年,在过去27年中持续进行,使用位于希腊北部塞萨洛尼基亚里士多德大学核技术实验室外的基于碘化钠(铊)的Xetex 501A辐射监测器,并创建了一个时间序列。1995 - 1998年以及2013 - 2015年期间,还在同一地点使用便携式高纯锗(HPGe)探测器进行了测量。空气中的总吸收剂量率随时间呈指数下降。空气中的总吸收剂量率是由于(1)铀系、(2)钍系、(3)钾和(4)铯(因切尔诺贝利事故)产生的伽马剂量率之和。此外,辐射监测器测量到宇宙辐射有一小部分贡献。通过使用HPGe探测器进行的时间依赖性测量发现,由于(1)铀系、(2)钍系和(3)钾产生的空气中伽马吸收剂量率的时间依赖性相当稳定。相反,由于铯产生的伽马剂量率以约13.5年的有效半衰期(t)呈指数下降,比铯自然衰变预期的要强。对空气中月平均总吸收剂量率进行了时间序列分析。傅里叶分析揭示了几个周期性,应用赵 - 阿特拉斯 - 马克斯变换揭示了这些周期性的时间分布。有三个主要可辨别的周期性:12 ± 0.2、42.3 ± 2.9和53.2 ± 3.2个月。其中一个具有季节性特征(年周期),可与季节性大气变化相关联,在1988年至2002年以及2008年至2014年期间清晰可见。另外两个(42.3 ± 2.9和53.2 ± 3.2个月)也被发现与气象参数(气温)有关,并且在2002 - 2004年年周期较弱时非常强烈。除了这三个主要周期性外,还有另外四个幅度较小的周期性(14.7、18.6、21.3和27.3个月);其中三个与太阳活动的文献数据周期性吻合良好。讨论了由于太阳活动可能影响伽马辐射测量的不同机制。