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Overview of aerosol optical properties over southern West Africa from DACCIWA aircraft measurements

机译:来自DACCIWA飞机测量的西非南部非洲气溶胶光学特性概述

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Southern West Africa (SWA) is an African pollution hotspot but a relatively poorly sampled region of the world. We present an overview of in situ aerosol optical measurements collected over SWA in June and July 2016 as part as of the DACCIWA (Dynamics-Aerosol-Chemistry-Clouds Interactions in West Africa) airborne campaign. The aircraft sampled a wide range of air masses, including anthropogenic pollution plumes emitted from the coastal cities, long-range transported biomass burning plumes from central and southern Africa and dust plumes from the Sahara and Sahel region, as well as mixtures of these plumes. The specific objective of this work is to characterize the regional variability of the vertical distribution of aerosol particles and their spectral optical properties (single scattering albedo: SSA, asymmetry parameter, extinction mass efficiency, scattering ?ngstr?m exponent and absorption ?ngstr?m exponent: AAE). The first findings indicate that aerosol optical properties in the planetary boundary layer were dominated by a widespread and persistent biomass burning loading from the Southern Hemisphere. Despite a strong increase in aerosol number concentration in air masses downwind of urban conglomerations, spectral SSA were comparable to the background and showed signatures of the absorption characteristics of biomass burning aerosols. In the free troposphere, moderately to strongly absorbing aerosol layers, dominated by either dust or biomass burning particles, occurred occasionally. In aerosol layers dominated by mineral dust particles, SSA varied from 0.81 to 0.92 at 550nm depending on the variable proportion of anthropogenic pollution particles externally mixed with the dust. For the layers dominated by biomass burning particles, aerosol particles were significantly more light absorbing than those previously measured in other areas (e.g. Amazonia, North America), with SSA ranging from 0.71 to 0.77 at 550nm. The variability of SSA was mainly controlled by variations in aerosol composition rather than in aerosol size distribution. Correspondingly, values of AAE ranged from 0.9 to 1.1, suggesting that lens-coated black carbon particles were the dominant absorber in the visible range for these biomass burning aerosols. Comparison with the literature shows a consistent picture of increasing absorption enhancement of biomass burning aerosol from emission to remote location and underscores that the evolution of SSA occurred a long time after emission. The results presented here build a fundamental basis of knowledge about the aerosol optical properties observed over SWA during the monsoon season and can be used in climate modelling studies and satellite retrievals. In particular and regarding the very high absorbing properties of biomass burning aerosols over SWA, our findings suggest that considering the effect of internal mixing on absorption properties of black carbon particles in climate models should help better assess the direct and semi-direct radiative effects of biomass burning particles.
机译:南部非洲(SWA)是非洲污染热点,但世界上采取了相对较差的地区。我们概述了2016年6月和7月在SWA收集的原位气溶胶光学测量,作为DACCIWA(西非动力学 - 气溶胶化学云互动)空中竞选的一部分。该飞机采样了各种空气群众,包括从沿海城市发出的人为污染羽毛,远程运输的生物量从中央和南部非洲燃烧羽毛,以及来自撒哈拉和萨赫尔地区的尘埃羽毛,以及这些羽毛的混合物。这项工作的具体目标是表征气溶胶颗粒的垂直分布的区域变异性及其光谱光学性质(单散射Albedo:SSA,不对称参数,消光质量效率,散射ΔngΔM指数和吸收?Ngstr?M指数:AAE)。第一个发现表明行星边界层中的气溶胶光学性质由来自南半球的广泛和持续的生物质燃烧负荷来支配。尽管在城市集团的空气群体中的气溶胶数量浓度强烈增加,但光谱SSA与背景相当,并且显示了生物质燃烧气溶胶的吸收特性的签名。在自由的对流层中,适度以强烈吸收气溶胶层,由灰尘或生物质燃烧颗粒占有平,偶尔发生。在由矿物粉尘颗粒主导的气溶胶层中,SSA在550nm下变化0.81至0.92,取决于外部与灰尘外部混合的人为污染颗粒的可变比例。对于由生物质燃烧颗粒支配的层,气溶胶颗粒比以前在其他区域(例如Amazonia,North America)中测量的那些更为光吸收,SSA在550nm处的0.71至0.77。 SSA的可变性主要受气溶胶组成的变化来控制,而不是气溶胶尺寸分布。相应地,AAE的值范围为0.9至1.1,表明镜片​​涂层的黑碳颗粒是这些生物质燃烧气溶胶的可见范围中的显性吸收器。与文献的比较显示了增加生物质吸收的吸收增强从发射到远程位置的吸收增强,并且在排放后SSA的演化发生了很长的时间。此处提出的结果为季风季节在SWA观察到的气溶胶光学特性,并可用于气候建模研究和卫星检索的基础。特别是在SWA上燃烧气溶胶的生物质的非常高的吸收性,我们的研究结果表明,考虑到内部混合对气候模型中黑碳颗粒的吸收性能的影响,应有助于更好地评估生物质的直接和半直接辐射效果燃烧的颗粒。
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