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首页> 外文期刊>Atmospheric Measurement Techniques >Marine boundary layer cloud property retrievals from high-resolution ASTER observations: case studies and comparison with Terra MODIS
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Marine boundary layer cloud property retrievals from high-resolution ASTER observations: case studies and comparison with Terra MODIS

机译:从高分辨率ASTER观测值获取海洋边界层云属性:案例研究和与Terra MODIS的比较

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A research-level retrieval algorithm for cloud optical and microphysical properties is developed for the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) aboard the Terra satellite. It is based on the operational MODIS algorithm. This paper documents the technical details of this algorithm and evaluates the retrievals for selected marine boundary layer cloud scenes through comparisons with the operational MODIS Data Collection 6 (C6) cloud product. The newly developed, ASTER-specific cloud masking algorithm is evaluated through comparison with an independent algorithm reported in Zhao and Di Girolamo (2006). To validate and evaluate the cloud optical thickness (tau) and cloud effective radius (r(eff)) from ASTER, the high-spatial-resolution ASTER observations are first aggregated to the same 1000m resolution as MODIS. Subsequently, tau(aA) and r(eff, aA) retrieved from the aggregated ASTER radiances are compared with the collocated MODIS retrievals. For overcast pixels, the two data sets agree very well with Pearson's product-moment correlation coefficients of R > 0.970. However, for partially cloudy pixels there are significant differences between r(eff, aA) and the MODIS results which can exceed 10 mu m. Moreover, it is shown that the numerous delicate cloud structures in the example marine boundary layer scenes, resolved by the high-resolution ASTER retrievals, are smoothed by the MODIS observations. The overall good agreement between the research-level ASTER results and the operational MODIS C6 products proves the feasibility of MODIS-like retrievals from ASTER reflectance measurements and provides the basis for future studies concerning the scale dependency of satellite observations and three-dimensional radiative effects.
机译:针对Terra卫星上的高级星载热发射和反射辐射计(ASTER),开发了一种研究级的云光学和微物理特性检索算法。它基于可操作的MODIS算法。本文记录了该算法的技术细节,并通过与可操作的MODIS Data Collection 6(C6)云产品进行比较,评估了所选海洋边界层云场景的检索结果。通过与Zhao和Di Girolamo(2006)中报告的独立算法进行比较,评估了新开发的ASTER特定的云屏蔽算法。为了验证和评估来自ASTER的云光学厚度(tau)和云有效半径(r(eff)),首先将高空间分辨率的ASTER观测值汇总为与MODIS相同的1000m分辨率。随后,将从聚合的ASTER辐射度中检索到的tau(aA)和r(eff,aA)与并置的MODIS检索进行比较。对于阴像素,两个数据集与R> 0.970的Pearson乘积矩相关系数非常吻合。但是,对于部分浑浊的像素,r(eff,aA)与MODIS结果之间存在显着差异,可能会超过10μm。此外,还表明,通过高分辨率ASTER检索解决的示例海洋边界层场景中的大量微妙云结构已通过MODIS观测得到了平滑。研究水平的ASTER结果与可操作的MODIS C6产品之间的总体良好一致性证明了从ASTER反射率测量中进行类似MODIS检索的可行性,并为以后有关卫星观测的尺度依赖性和三维辐射效应的研究提供了基础。

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