利用遥感和运输模型对西欧撒哈拉尘羽的调查

Hengheng Zhang, F. Wagner, H. Saathoff, H. Vogel, G. Hoshyaripour, V. Bachmann, J. Förstner, T. Leisner
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引用次数: 1

摘要

摘要2018年4月7日至9日,利用扫描激光雷达(90°,30°)、垂直激光雷达(90°)、太阳光谱仪和传输模型iconart,在德国西南部卡尔斯鲁厄市(8.4298°E, 49.0953°N)附近研究了撒哈拉沙尘羽的演变和特性。激光雷达测量结果表明,尘埃粒子的后向散射系数为0.86±0.14 Mm−1 Sr−1,消光系数为40±0.8 Mm−1,激光雷达比为46±5 Sr,粒子退极化比为0.33±0.07。这些数值与以前在西欧对撒哈拉沙尘羽流的研究中得到的结果非常一致。与遥感测量结果相比,模式模拟对羽流到达时间、层高和结构的预测较好,但对后向散射系数的估计过高。在这篇文章中,我们讨论了不同测量方法的互补性和优势以及模型模拟来预测撒哈拉沙尘羽流。主要结论是:ICON-ART模型可以很好地预测撒哈拉沙尘羽的结构,但在355 nm处的后向散射系数高估了2.2±0.16倍,在340 nm处的气溶胶光学深度(AOD)低估了1.5±0.11倍。采用扫描气溶胶激光雷达可以独立确定白天和夜间的后向散射系数、粒子去极化比,特别是撒哈拉沙尘的激光雷达比。将激光雷达与太阳光度计数据相结合,可以以不同的方式限制气溶胶光学深度,并确定柱集成激光雷达比率。这些综合数据集有助于更好地了解西欧的撒哈拉沙尘羽流。
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Investigation of a Saharan dust plume in Western Europe by remote sensing and transport modelling
Abstract. The evolution and the properties of a Saharan dust plume were studied near the city of Karlsruhe in south-west Germany (8.4298° E, 49.0953° N) from April 7 to 9, 2018 combining a scanning LIDAR (90°, 30°), a vertical LIDAR (90°), a sun photometer, and the transport model ICON-ART. The LIDAR measurements show that the dust particles had backscatter coefficients of 0.86 ± 0.14 Mm−1 Sr−1, an extinction coefficient of 40 ± 0.8 Mm−1, a LIDAR ratio of 46 ± 5 sr, and a particle depolarization ratio of 0.33 ± 0.07. These values are in good agreement with those obtained in previous studies of Saharan dust plumes in Western Europe. Compared to the remote sensing measurements, the model simulation predicts the plume arrival time, its layer height, and structure very well but overestimates the backscatter coefficient. In this manuscript, we discuss the complementarity and advantages of the different measurement methods as well model simulations to predict Saharan dust plumes. Main conclusions are that the ICON-ART model can predict the structure of Saharan dust plumes very well but overestimates the backscatter coefficients by a factor of 2.2 ± 0.16 at 355 nm and underestimates the aerosol optical depth (AOD) by a factor of 1.5 ± 0.11 at 340 nm for this Saharan dust plume event. Employing a scanning aerosol LIDAR allows determining backscatter coefficient, particle depolarization ratio and especially LIDAR ratio of Saharan dust both for daytime and nighttime independently. Combining LIDAR with sun photometer data allows constraining aerosol optical depth in different ways and determining column integrated LIDAR ratios. These comprehensive datasets allow for a better understanding of Saharan dust plumes in Western Europe.
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