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How clear-sky polarization varies with wavelength in the visible-NIR

机译:晴空偏振如何随可见近红外中的波长变化

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摘要

Because of the increasing variety of applications for polarization imaging and sensing, there is a growing need for information about polarization phenomenology in the natural environment, including the spectral distribution of polarization in the atmosphere. A computer model that has been validated in comparisons with measurements from our all-sky polarization imager has been used here to simulate the spectrum of clear-sky polarization at a many locations around the world, with a wide variety of underlying surface-reflectance and aerosol conditions. This study of the skylight polarization spectral variability shows that there is no simple spectrum that can be assumed or predicted without knowledge of the atmospheric aerosol properties and underlying surface reflectance.
机译:由于偏振成像和传感的应用种类越来越多,因此越来越需要有关自然环境中偏振现象的信息,包括大气中偏振的光谱分布。经过验证的计算机模型与全天候偏振成像仪的测量结果进行了比较,这里已使用该计算机模型来模拟世界上许多地方的晴空偏振光谱,并具有各种潜在的表面反射率和气溶胶。条件。对天光偏振光谱变异性的这项研究表明,如果不了解大气气溶胶特性和下面的表面反射率,就无法假设或预测简单的光谱。

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