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首页> 外文期刊>Boundary-layer Meteorology >Vertical Structure of the Urban Boundary Layer over Marseille UnderSea-Breeze Conditions
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Vertical Structure of the Urban Boundary Layer over Marseille UnderSea-Breeze Conditions

机译:海风条件下马赛市区边界层的垂直结构

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摘要

During the UBL-ESCOMPTE program (June-July 2001), intensive observations were performed in Marseille (France). In particular, a Doppler lidar, located in the north of the city, provided radial velocity measurements on a 6-km radius area in the lowest 3 km of the troposphere. Thus, it is well adapted to document the vertical structure of the atmosphere above complex terrain, notably in Marseille, which is bordered by the Mediterranean sea and framed by numerous massifs. The present study focuses on the last day of the intensive observation period 2 (26 June 2001), which is characterized by a weak synoptic pressure gradient favouring the development of thermal circulations. Under such conditions, a complex stratification of the atmosphere is observed. Three-dimensional numerical simulations, with the Meso-NH atmospheric model including the town energy balance (TEB) urban parameterization, are conducted over south-eastern France. A complete evaluation of the model outputs was already performed at both regional and city scales. Here, the 250-m resolution outputs describing the vertical structure of the atmosphere above the Marseille area are compared to the Doppler lidar data, for which the spatial resolution is comparable. This joint analysis underscores the consistency between the atmospheric boundary layer (ABL) observed by the Doppler lidar and that modelled by Meso-NH. The observations and simulations reveal the presence of a shallow sea breeze (SSB) superimposed on a deep sea breeze (DSB) above Marseille during daytime. Because of the step-like shape of the Marseille coastline, the SSB is organized in two branches of different directions, which converge above the city centre. The analysis of the 250-m wind fields shows evidence of the role of the local topography on the local dynamics. Indeed, the topography tends to reinforce the SSB while it weakens the DSB. The ABL is directly affected by the different sea-breeze circulations, while the urban effects appear to be negligible.
机译:在UBL-ESCOMPTE计划(2001年6月至7月)期间,在马赛(法国)进行了密集的观测。特别是,位于城市北部的多普勒激光雷达在对流层最低3 km的6 km半径区域提供了径向速度测量。因此,它非常适合用来记录复杂地形上方的大气的垂直结构,特别是在马赛地区,该地区以地中海为边界,并由众多地块围绕。本研究的重点是密集观测期2的最后一天(2001年6月26日),其特征是天气压力梯度弱,有利于热循环的发展。在这样的条件下,观察到大气的复杂分层。在法国东南部进行了三维数值模拟,其中包括Meso-NH大气模型,包括城镇能源平衡(TEB)城市参数化。已经在区域和城市范围内对模型输出进行了完整的评估。在这里,将描述马赛地区上方大气垂直结构的250米分辨率输出与多普勒激光雷达数据进行比较,多普勒激光雷达数据的空间分辨率可比。这项联合分析强调了多普勒激光雷达观测到的大气边界层(ABL)与Meso-NH模拟的边界层之间的一致性。观测和模拟显示白天白天在马赛上方的深海风(DSB)上叠加了浅海风(SSB)。由于马赛海岸线呈阶梯状,因此,SSB分为两个不同方向的分支机构,它们汇聚在市中心上方。对250米风场的分析显示了当地地形对当地动力的作用的证据。实际上,地形往往会增强SSB,同时削弱DSB。 ABL受到不同海风环流的直接影响,而城市影响似乎可以忽略不计。

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