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首页> 外文期刊>Atmospheric chemistry and physics >Measurements of Saharan dust aerosols over the Eastern Mediterranean using elastic backscatter-Raman lidar, spectrophotometric and satellite observations in the frame of the EARLINET project
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Measurements of Saharan dust aerosols over the Eastern Mediterranean using elastic backscatter-Raman lidar, spectrophotometric and satellite observations in the frame of the EARLINET project

机译:使用EARLINET项目框架中的弹性背向散射拉曼激光雷达,分光光度法和卫星观测对地中海东部的撒哈拉尘埃气溶胶进行测量

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We report on the vertical distributions of Saharan dust aerosols over theN.E. Mediterranean region, which were obtained during a typical dustoutbreak on August 2000, by two lidar systems located in Athens andThessaloniki, Greece, in the frame of the European EARLINET project. MODISand ground sun spectrophotometric data, as well as air-mass backwardtrajectories confirmed the existence of Saharan dust in the case examined,which was also successfully forecasted by the DREAM dust model. The lidardata analysis for the period 2000-2002 made possible, for the first time, anestimation of the vertical extent of free tropospheric dust layers [meanvalues of the aerosol backscatter and extinction coefficients and theextinction-to-backscatter ratio (lidar ratio, LR) at 355 nm], as well as aseasonal distribution of Saharan dust outbreaks over Greece, undercloud-free conditions. A mean value of the lidar ratio at 355 nm wasobtained over Athens (53±1 sr) and over Thessaloniki (44±2 sr)during the Saharan dust outbreaks. The corresponding aerosol opticalthickness (AOT) at 355 nm, in the altitude range 0-5 km, was 0.69±0.12and 0.65±0.10 for Athens and Thessaloniki, respectively (within thedust layer the AOT was 0.23 and 0.21, respectively). Air-massback-trajectory analysis performed in the period 2000-2002 for all Saharandust outbreaks over the N.E. Mediterranean indicated the main pathwaysfollowed by the dust aerosols.
机译:我们报告了东北地区撒哈拉粉尘气溶胶的垂直分布。地中海地区是在2000年8月一次典型的尘埃暴发期间获得的,这是由两个位于希腊雅典和塞萨洛尼基的激光雷达系统在欧洲EARLINET项目的框架下获得的。 MODIS和地面太阳分光光度数据以及空气质量向后轨迹证实了该案例中撒哈拉尘埃的存在,这也通过DREAM尘埃模型成功地进行了预测。 2000-2002年的激光雷达数据分析首次使对流层自由尘埃层的垂直范围[气溶胶背向散射和消光系数的平均值以及消退与背向比(激光比,LR)的估算成为可能。 355海里],以及在无云的条件下希腊撒哈拉爆发的季节性分布。在撒哈拉沙漠爆发期间,在雅典(53±1 sr)和塞萨洛尼基(44±2 sr)获得了355 nm激光雷达比的平均值。在0-5 km的海拔范围内,雅典和塞萨洛尼基在355 nm处对应的气溶胶光学厚度(AOT)分别为0.69±0.12和0.65±0.10(在粉尘层内,AOT分别为0.23和0.21)。在2000年至2002年期间,对东北地区的所有Saharandust爆发进行了空气质量轨迹分析。地中海是尘埃尘溶胶跟随的主要途径。

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