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首页> 外文期刊>Journal of Geophysical Research, D. Atmospheres: JGR >Development of empirical angular distribution models for smoke aerosols: Methods
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Development of empirical angular distribution models for smoke aerosols: Methods

机译:发展经验角分布烟雾气溶胶:方法的模型

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Using broadband shortwave radiance measurements from the Clouds and Earth Radiant Energy System (CERES) sensors onboard the Terra and Aqua satellites, empirical angular distribution models (EADM) are constructed for smoke aerosols. These EADMs are constructed for smoke aerosols emitted during the biomass burning season (August-October), in South America. All available years (2000-2008) of both rotating azimuth plane and cross-track radiance data from CERES have been utilized. Aerosol scenes are identified using coincident aerosol optical thickness retrievals from the Moderate Resolution Imaging Spectroradiometer (MODIS). The new EADMs are used to estimate top-of-atmosphere (TOA) shortwave flux for cloud free scenes. The CERES clearly shows the angular dependence of shortwave radiance on smoke aerosol optical thickness. A comparison of TOA shortwave fluxes estimated from the new smoke EADM with the existing CERES TOA shortwave fluxes shows that the CERES fluxes are higher (lower) for aerosol optical thickness less (greater) than 0.3, largely due to the use of aerosol optical thickness in characterizing the new EADMs developed in this study. Empirical ADMs for smoke aerosols over land are developed for the first time in this study, and our results demonstrate that large amounts of aerosols emitted during biomass burning activities contribute to the anisotropy of the radiance distribution at the TOA. Therefore, it is imperative to include aerosol information in the angular distribution models, especially now that more than a 10 year record of Terra data is available
机译:使用宽带短波辐射测量从云层和地球辐射能量系统泰拉和阿卡上(CERES)传感器卫星,经验角分布模型(EADM)构造烟雾气溶胶。构造EADMs烟雾气溶胶排放在生物质燃烧的季节(10月间vix指数),在南美洲。年(2000 - 2008)的旋转方位平面从谷神星和航迹辐射数据被利用。使用一致的气溶胶光学厚度检索中分辨率成像光谱仪(MODIS)。估计top-of-atmosphere短波(TOA)通量云免费的场景。显示了短波角的依赖关系光芒在烟雾气溶胶光学厚度。比较TOA短波通量估计新与现有谷神星TOA EADM抽烟短波通量显示谷神星通量高(低)气溶胶光学厚度(更大的)比0.3,很大程度上是由于使用气溶胶光学厚度的描述本研究的新EADMs发达。对烟雾气溶胶对土地开发在这项研究中,第一次和我们的结果证明大量的气溶胶生物质燃烧时所产生的活动为各向异性的光辉在TOA分布。必须包括气溶胶中的信息角分布模型,特别是现在10年以上的记录数据可用

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