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A model framework to reduce bias in ground-level PM_(2.5) concentrations inferred from satellite-retrieved AOD

机译:从卫星检索的AOD推断出地面PM_(2.5)浓度的偏倚的模型框架

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摘要

We present a new method to infer ground-level fine particulate matter (PM2.5) from satellite remote sensing observations of aerosol optical depth (AOD). The conventional method generally uses a range of modelling approaches to determine PM2.5:AOD relationships that are subsequently used to infer ground-level PM2.5 concentrations from satellite-retrieved AOD. Here, we use a high-resolution atmospheric chemistry simulation to explore how changes in the vertical distribution of aerosol extinction coefficients affects the PM2.5:AOD relationship and how we can use that information to improve the robustness of inferred estimates of ground-level PM2.5 over eastern China. We define a metric, Gamma AODPBL, that describes the fraction of AOD that resides in the planetary boundary layer compared with the total columnar AOD. We determine physically-meaningful PM2.5: AOD relationships using data for which Gamma AODPBL = 50%, a criterion based on sensitivity analyses on data clusters that we identify using a hierarchical clustering method. We use statistical and machine learning methods to develop independent models that describe these PM2.5:AOD relationships, and use a Monte Carlo approach to quantify the improvement after our selection of more physically relevant data records. Benefiting from the improved representativeness of AOD for ground-level PM2.5, our method effectively reduces bias in inferred estimates of ground-level PM2.5 by 10-15% (9-12%) for space-borne sensors passing over in the morning (afternoon). It also captures more variations in ground-level PM2.5 by up to 8% (5%) for space-borne sensors passing over in the morning (afternoon), particularly over areas dominated by natural aerosols such as dust. Accordingly, our method improves the seasonal ground-level PM2.5 maps, e.g. the bias of the autumn (winter) mean of ground level PM2.5 estimates over Qinghai and Gansu (Shaaxi, Shanxi, and Henan) provinces reduces from-8% to-5% (11%-6%).
机译:我们提出了一种从气溶胶光学深度(AOD)的卫星遥感观察中推断出地层精细颗粒物(PM2.5)的新方法。传统方法通常使用一系列建模方法来确定PM2.5:AOD关系,其随后用于从卫星检索的AOD中推断出地层PM2.5浓度。在这里,我们使用高分辨率大气化学仿真来探讨气溶胶消光系数的垂直分布的变化如何影响PM2.5:AOD关系以及我们如何利用该信息来提高地面PM2推断估计的鲁棒性在中国东部。我们定义了一个公制,Gamma Aodpbl,其描述与总柱状AOD相比地驻留在行星边界层的AOD的分数。我们使用伽马Aodpbl> = 50%的数据确定物理有意义的PM2.5:AOD关系,基于使用分层聚类方法识别的数据集群对敏感性分析的标准。我们使用统计和机器学习方法开发描述这些PM2.5:AOD关系的独立模型,并使用Monte Carlo方法量化我们选择更具物理相关数据记录后的改进。从AOD的AOD的改善代表性受益于地面PM2.5的提高,我们的方法有效地减少了地面PM2.5的推断估计值10-15%(9-12%)用于通过其的空间传感器上午下午)。它还捕获地面PM2.5的更多变化,高达8%(5%)用于在早晨(下午)通过的空间传感器,特别是在由天然气溶胶如灰尘中占主导地位的区域。因此,我们的方法改善了季节性地面PM2.5地图,例如:秋季(冬季)的偏差平均接地水平PM2.5估计青海和甘肃(陕西,山西和河南)省份省份从-8%降至-5%(11%-6%)。

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