AGASP III期间的光学深度和雾霾颗粒大小

Peter Pilewskie, Francisco P.J. Valero
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引用次数: 8

摘要

作为北极气体气溶胶采样项目第三部分(AGASP III)的一部分,使用全直接漫射辐射计研究了北极雾霾的光学特性。辐射计安装在NOAA WP-3D研究飞机上,测量了可见光和近红外的七个窄带通道的太阳下流辐照度。在AGASP航班310和311中,雾霾光学深度的最大值接近0.1。从311航班消光测量推断出的粒径谱在0.1 μm和0.8 μm附近有两个主要模式。提出了一种反演散射辐射角依赖性的方法,并提出了薄卷云的存在。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Optical depths and haze particle sizes during AGASP III

The optical properties of Arctic Haze were studied using a total-direct-diffuse radiometer as part of the Arctic Gas Aerosol Sampling Project, part III (AGASP III). The radiometer was installed on the NOAA WP-3D research aircraft and measured solar downwelling irradiance in seven narrow-band channels in the visible and near-infra-red. Haze optical depths had maximum values near 0.1 in the mid-visible for AGASP flights 310 and 311. An inferred particle size spectrum from flight 311 extinction measurements showed two dominant modes near 0.1 and 0.8 μm. A method of retrieving the angular dependence of scattered radiation is presented and suggests the presence of thin cirrus.

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