首页> 外文期刊>Atmospheric Chemistry and Physics Discussions >Vertical aerosol distribution in the southern hemispheric midlatitudes as observed with lidar in Punta Arenas, Chile (53.2°?S and 70.9°?W), during ALPACA
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Vertical aerosol distribution in the southern hemispheric midlatitudes as observed with lidar in Punta Arenas, Chile (53.2°?S and 70.9°?W), during ALPACA

机译:在ALPACA期间,在智利的蓬塔阿雷纳斯(Punta Arenas)用激光雷达观测到的南半球中纬度的垂直气溶胶分布(53.2°?S和70.9°?W)

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Within this publication, lidar observations of the vertical aerosol distribution above Punta Arenas, Chile (53.2 sup°/sup S and 70.9 sup°/sup W), which have been performed with the Raman lidar Polly supXT/sup from December 2009 to April 2010, are presented. Pristine marine aerosol conditions related to the prevailing westerly circulation dominated the measurements. Lofted aerosol layers could only be observed eight times during the whole measurement period. Two case studies are presented showing long-range transport of smoke from biomass burning in Australia and regionally transported dust from the Patagonian Desert, respectively. The aerosol sources are identified by trajectory analyses with the Hybrid Single-Particle Lagrangian Integrated Trajectory (HYSPLIT) and FLEXible PARTicle dispersion model (FLEXPART). However, seven of the eight analysed cases with lofted layers show an aerosol optical thickness of less than 0.05. From the lidar observations, a?mean planetary boundary layer (PBL) top height of 1150?±?350 m was determined. An analysis of particle backscatter coefficients confirms that the majority of the aerosol is attributed to the PBL, while the free troposphere is characterized by a very low background aerosol concentration. The ground-based lidar observations at 532 and 1064?nm are supplemented by the Aerosol Robotic Network (AERONET) Sun photometers and the space-borne Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP) aboard the Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation (CALIPSO). The averaged aerosol optical thickness (AOT) determined by CALIOP was 0.02?±?0.01 in Punta Arenas from 2009 to 2010.
机译:在此出版物中,对智利蓬塔阿雷纳斯上空的垂直气溶胶分布(53.2 ° S和70.9 ° W)进行了激光雷达观测,这些观测是通过拉曼激光雷达Polly <介绍了从2009年12月到2010年4月的sup> XT 。与普遍的西风环流有关的原始海洋气溶胶条件主导了测量。在整个测量期间,只能观察到八次放气的气溶胶层。提出了两个案例研究,分别显示了澳大利亚生物质燃烧产生的烟尘的远距离运输和巴塔哥尼亚沙漠地区的粉尘。通过混合单颗粒拉格朗日综合轨迹(HYSPLIT)和柔性颗粒弥散模型(FLEXPART)的轨迹分析来识别气溶胶源。但是,在分析的具有放样层的八种情况中,有七种显示的气溶胶光学厚度小于0.05。根据激光雷达的观测,确定了平均行星边界层(PBL)的最高高度为1150±±350 m。对颗粒后向散射系数的分析证实,大多数气溶胶归因于PBL,而自由对流层的特征是背景气溶胶浓度非常低。气溶胶机器人网络(AERONET)太阳光度计和星云云气溶胶激光雷达和红外探路者卫星观测补充了气溶胶机器人网络(AERONET)太阳光度计和带正交偏振的星云气溶胶激光雷达(CALIOP),对地面激光雷达观测提供了补充。 (CALIPSO)。在2009年至2010年期间,由CALIOP确定的蓬塔阿雷纳斯平均气溶胶光学厚度(AOT)为0.02±±0.01。

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