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Dynamical Nighttime Fog/Low Stratus Detection Based on Meteosat SEVIRI Data: A Feasibility Study

机译:基于Meteosat SEVIRI数据的动态夜间雾/低层探测的可行性研究

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Automated detection of fog and low stratus in nighttime satellite data has been implemented on the basis of numerous satellite systems in past decades. Commonly, differences in small-droplet emissivities at 11μm and 3.9μm are utilized. With Meteosat SEVIRI, however, this method cannot be applied with a fixed threshold due to instrument design: The 3.9μm band is exceptionally wide and overlaps with the 4μm CO2 absorption band. Therefore, the emissivity difference varies with the length of the slant atmospheric column between sensor and object. To account for this effect, the new technique presented in this paper is based on the dynamical extraction of emissivity difference thresholds for different satellite viewing zenith angles. In this way, varying concentrations of CO2 and column depths are accounted for. The new scheme is exemplified in a plausibility study and shown to provide reliable results.
机译:在过去的几十年中,已经在众多卫星系统的基础上实现了夜间卫星数据中雾和低层的自动检测。通常,利用11μm和3.9μm处的小液滴发射率的差异。但是,对于Meteosat SEVIRI,由于仪器设计的原因,该方法无法在固定阈值下应用:3.9μm谱带异常宽,与4μmCO2吸收谱带重叠。因此,发射率差随传感器和物体之间的倾斜大气柱的长度而变化。为了解决这个问题,本文提出的新技术基于不同卫星观测天顶角的发射率差异阈值的动态提取。这样,就可以解释不同浓度的CO2 和色谱柱深度。该新方案在真实性研究中得到了例证,并被证明可以提供可靠的结果。

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