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首页> 外文期刊>Journal of Quantitative Spectroscopy & Radiative Transfer >A pilot study of shortwave spectral fingerprints of smoke aerosols above liquid clouds
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A pilot study of shortwave spectral fingerprints of smoke aerosols above liquid clouds

机译:液体云中烟雾气溶胶短波光谱指纹的试验研究

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摘要

Absorbing aerosols like smoke heat the atmosphere by absorbing solar radiation, and such heating is enhanced when aerosols are above liquid clouds. To reduce uncertainty in estimates of the aerosol radiative forcing, it is desirable to characterize the size, index of refraction, optical depth, and altitude of smoke aerosols and underlying cloud droplets. While past work with remotely sensed multi-spectral data have made progress toward such characterization, it remains unclear if those radiatively important parameters can be fully and simultaneously retrieved from shortwave hyperspectral measurements. This issue is studied here first by examining the spectral fingerprints of above-cloud aerosols in the shortwave region (wavelength from 330 nm to 4000 nm) using hyperspectral radiative transfer simulations. These simulations are further explored to analyze the information content for hyperspectral inversion of aerosol and cloud optical depths as well as their microphysical properties over an ocean surface. The analysis shows that the Moderate Resolution Imaging Spectroradiometer (MODIS), with limited spectral bands in the solar spectrum, has partial information required for retrieving the optical depth and the effective radius of smoke and cloud. In contrast, hyperspectral measurements have about 5 extra pieces of information (double the degrees of freedom for signals of MODIS), allowing for the retrieval of additional aerosol and cloud microphysical parameters, including the smoke layer height above cloud, the imaginary part of smoke refractive index, and partially the effective variance of cloud droplet size. Thus, hyperspectral measurements can provide valuable constraints on heating rate estimates of absorbing aerosols above clouds. (C) 2018 Elsevier Ltd. All rights reserved.
机译:吸收烟雾等气雾剂通过吸收太阳辐射而加热气氛,并且当气溶胶高于液体云时,这种加热增强。为了减少气溶胶辐射强制估计的不确定性,希望表征烟雾气雾剂和底层云液滴的尺寸,折射率,光学深度和高度。虽然过去具有远程感测的多光谱数据的工作已经朝着这样的表征进行了进展,但是如果可以从短波高光谱测量中完全和同时检索那些辐射的重要参数,仍然不清楚。这里首先通过检查短波区域(波长从330nm至4000nm)中的云气溶胶的光谱指纹来研究此问题,使用超细辐射传递模拟。进一步探索这些模拟以分析气溶胶和云光学深度的高光谱反转的信息含量以及在海面上的微妙性质。该分析表明,在太阳光谱中,具有有限的光谱带的中等分辨率成像光谱仪(MODIS)具有检索光学深度和有效烟雾半径所需的部分信息。相比之下,高光谱测量有大约5个额外的信息(Modis信号的双倍自由度),允许检索额外的气溶胶和云微物理参数,包括云上方的烟雾层高度,烟雾折射的虚部索引,部分是云液滴尺寸的有效方差。因此,高光谱测量可以为吸收云吸收气溶胶的加热速率估计提供有价值的限制。 (c)2018年elestvier有限公司保留所有权利。

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  • 作者单位

    Univ Iowa Dept Chem &

    Biochem Engn Ctr Global &

    Reg Environm Studies &

    Informat Init Iowa City IA 52242 USA;

    Univ Iowa Dept Chem &

    Biochem Engn Ctr Global &

    Reg Environm Studies &

    Informat Init Iowa City IA 52242 USA;

    Univ Iowa Dept Chem &

    Biochem Engn Ctr Global &

    Reg Environm Studies &

    Informat Init Iowa City IA 52242 USA;

    Univ Iowa Dept Chem &

    Biochem Engn Ctr Global &

    Reg Environm Studies &

    Informat Init Iowa City IA 52242 USA;

    NASA Goddard Space Flight Ctr Climate &

    Radiat Lab Greenbelt MD USA;

    NASA Goddard Space Flight Ctr Climate &

    Radiat Lab Greenbelt MD USA;

    Desert Res Inst Reno NV USA;

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  • 正文语种 eng
  • 中图分类 光学;
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