论文标题

纠正使用暮光作为校准器的衰老效果的天空质量计测量

Correcting Sky Quality Meter measurements for aging effects using twilight as calibrator

论文作者

Puschnig, Johannes, Näslund, Magnus, Schwope, Axel, Wallner, Stefan

论文摘要

在过去的十年中,全球安装了许多天空质量仪(SQM),旨在评估夜空亮度(NSB)的时间变化,从而评估光污染的变化。但是,很明显,SQM读数可能会受到衰老效应的影响,例如传感器敏感性和/或光学组件(滤镜,外壳窗口)的传播率丧失。迄今为止,尚未以系统的方式评估黑暗的大小。我们首次报告了SQM衰老效应的定量,并描述了应用方法。我们结合了2011年至2019年之间在Potsdam-Babelsberg(距柏林中心西南23公里),维也纳和斯德哥尔摩的长期SQM测量以及随时可用的经验暮光模型,该模型是校准器。通过以下斜率进行校准的暮光平方英尺的观察,用于变化的太阳高度,显示了测量系统(平方米 +外壳窗口)的线性退化:34 $ \ pm $ \ pm $ 4,46 $ \ pm $ \ pm $ 2和53 $ 2和53 $ \ pm $ 2毫米2毫米2毫米2毫米$ _ {\ rm _ {\ rm _ { yr $^{ - 1} $用于斯德哥尔摩,波茨坦 - 巴贝尔斯伯格和维也纳。在维也纳(Latitude $ \ sim $ 48 $^\ circ $)中发现的最高坡度和在斯德哥尔摩发现的最低坡度(纬度$ \ sim $ 59 $^\ circ $),我们找到了趋势依赖太阳辐照的指示(这是地理纬度的功能)。

In the last decade numerous Sky Quality Meters (SQMs) were installed throughout the globe, aiming to assess the temporal change of the night sky brightness (NSB), and thus the change in light pollution. However, it has become clear that SQM readings may be affected by aging effects such as degradation of the sensor sensitivity and/or loss of transmissivity of optical components (filter, housing window). To date, the magnitude of the darkening has not been assessed in a systematic way. We report for the first time on the quantification of the SQM aging effect and describe the applied method. We combine long-term SQM measurements obtained between 2011 and 2019 in Potsdam-Babelsberg (23 km to the southwest of the center of Berlin), Vienna and Stockholm with a readily available empirical twilight model, which serves as calibrator. Twilight SQM observations, calibrated for changing sun altitudes, reveal a linear degradation of the measurement systems (SQM + housing window) with the following slopes: 34$\pm$4, 46$\pm$2 and 53$\pm$2 milli-mag$_{\rm SQM}$ arcsec$^{-2}$ yr$^{-1}$ for Stockholm, Potsdam-Babelsberg and Vienna. With the highest slope found in Vienna (latitude $\sim$48$^\circ$) and the lowest one found in Stockholm (latitude $\sim$59$^\circ$), we find an indication for the dependence of the trend on solar irradiance (which is a function of geographic latitude).

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