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Analysis of influential factors for the relationship between PM2.5 and AOD in Beijing

机译:北京市PM2.5与AOD关系的影响因素分析。

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摘要

The relationship between aerosol optical depth (AOD) and PM isoften investigated in order to obtain surface PM from satelliteobservation of AOD with a broad area coverage. However, various factors couldaffect the AOD–PM regressions. Using both ground and satelliteobservations in Beijing from 2011 to 2015, this study analyzes theinfluential factors including the aerosol type, relative humidity (RH),planetary boundary layer height (PBLH), wind speed and direction, and thevertical structure of aerosol distribution. The ratio of PM to AOD,which is defined as , and the square of their correlation coefficient() have been examined. It shows that varies from 54.32 to183.14, 87.32 to 104.79, 95.13 to 163.52, and 1.23 to 235.08 µg mwith aerosol type in spring, summer, fall, and winter, respectively. issmaller for scattering-dominant aerosols than for absorbing-dominantaerosols, and smaller for coarse-mode aerosols than for fine-mode aerosols.Both RH and PBLH affect the value significantly. The higher the RH,the smaller the , and the higher the PBLH, the smaller the .For AOD and PM data with the correction of RH and PBLH compared tothose without, of monthly averaged PM and AOD at 14:00 LTincreases from 0.63 to 0.76, and of multi-year averaged PMand AOD by time of day increases from 0.01 to 0.93, 0.24 to 0.84, 0.85 to0.91, and 0.84 to 0.93 in four seasons respectively. Wind direction is a keyfactor for the transport and spatial–temporal distribution of aerosolsoriginated from different sources with distinctive physicochemicalcharacteristics. Similar to the variation in AOD and PM, alsodecreases with the increasing surface wind speed, indicating that thecontribution of surface PM concentrations to AOD decreases withsurface wind speed. The vertical structure of aerosol exhibits a remarkablechange with seasons, with most particles concentrated within about 500 m insummer and within 150 m in winter. Compared to the AOD of the wholeatmosphere, AOD below 500 m has a better correlation with PM, forwhich is 0.77. This study suggests that all the above influentialfactors should be considered when we investigate the AOD–PMrelationships.
机译:经常研究气溶胶光学深度(AOD)和PM之间的关系,以便从AOD的卫星观测获得大面积的表面PM。但是,各种因素都可能影响AOD-PM回归。利用2011年至2015年北京的地面和卫星观测资料,分析了气溶胶类型,相对湿度(RH),行星边界层高度(PBLH),风速和风向以及气溶胶分布的垂直结构等影响因素。已经检查了PM与AOD的比(定义为)以及它们的相关系数()的平方。结果表明,在春季,夏季,秋季和冬季,气溶胶类型分别从54.32至183.14、87.32至104.79、95.13至163.52和1.23至235.08μg/ g。散射占优势的气溶胶比吸收占优势的气溶胶小,而粗模式的气溶胶比精细的气溶胶小.RH和PBLH都显着影响该值。 RH越高,PBLH越小,PBLH越高。对于经过RH和PBLH校正的AOD和PM数据,与没有校正的情况相比,每月平均PM和AOD在14:00 LT的值从0.63增加到0.76和的平均年度平均PM和AOD值在四个季节中分别从0.01增至0.93、0.24增至0.84、0.85增至0.91和0.84至0.93。风向是源于具有独特理化特性的不同来源的气溶胶的运输和时空分布的关键因素。类似于AOD和PM的变化,也随着表面风速的增加而减小,这表明表面PM浓度对AOD的贡献随表面风速而降低。气溶胶的垂直结构随季节呈现出显着变化,大多数颗粒集中在夏季约500μm内,冬季约150μm内。与整个大气层的AOD相比,低于500μm的AOD与PM的相关性更好,为0.77。这项研究表明,当我们调查AOD-PM关系时,应考虑所有上述影响因素。

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