Diurnal Valley Winds in a Deep Alpine Valley: Model Results

Juerg Schmidli, Julian Quimbayo-Duarte
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引用次数: 1

Abstract

Thermally driven local winds are ubiquitous in deep Alpine valleys during fair weather conditions resulting in a unique wind climatology for any given valley. The accurate forecasting of these local wind systems is challenging, as they are the result of complex and multi-scale interactions. Even more so, if the aim is an accurate forecast of the winds from the near-surface to the free atmosphere, which can be considered a prerequisite for the accurate prediction of mountain weather. This study combines the evaluation of the simulated surface winds in several Alpine valleys with a more detailed evaluation of the wind evolution for a particular location in the Swiss Rhone valley, at the town of Sion during the month of September 2016. Four numerical simulations using the COSMO model are evaluated, two using a grid spacing of 1.1 km and two with a grid spacing of 550 m. For each resolution, one simulation is initialised with the soil moisture from the COSMO analysis and one with an increased soil moisture (+30%). In a first part, a comparison with observations from the operational measurement network of MeteoSwiss is used to evaluate the model performance, while, in a second part, data from a wind profiler stationed at Sion airport is used for a more detailed evaluation of the valley atmosphere near the town of Sion. The analysis focuses on 18 valley wind days observed in the Sion region in September 2016. Only the combination of an increased soil moisture and a finer grid spacing resulted in a significant improvement of the simulated flow patterns in the Sion region. This includes a stronger and more homogeneous along-valley wind in the Wallis and a more realistic cross-valley wind and temperature profile near the town of Sion. It is shown that the remaining differences between the observed and simulated near-surface wind are likely due to very local topographic features. Small-scale hills, not resolved on even the finer model grid, result in a constriction of the valley cross section and an acceleration of the observed low-level up-valley wind in the region of Sion.
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深阿尔卑斯山谷的日谷风:模式结果
在晴朗的天气条件下,热驱动的当地风在深阿尔卑斯山谷中无处不在,导致任何给定山谷的独特风气候学。由于这些局地风系统是复杂的多尺度相互作用的结果,因此对其进行准确预报具有挑战性。更重要的是,如果目标是准确预测从近地表到自由大气的风,这可以被认为是准确预测山区天气的先决条件。本研究结合了对几个阿尔卑斯山谷的模拟地面风的评估,以及对2016年9月瑞士罗纳河谷锡永镇某一特定地点的风演变的更详细评估。利用COSMO模型进行了4次数值模拟,其中2次栅格间距为1.1 km, 2次栅格间距为550 m。对于每个分辨率,一个模拟初始化为COSMO分析的土壤湿度,另一个模拟初始化为土壤湿度增加(+30%)。在第一部分中,使用与MeteoSwiss业务测量网络的观测结果进行比较来评估模型的性能,而在第二部分中,使用驻扎在锡安机场的风廓线仪的数据对锡安镇附近的山谷大气进行更详细的评估。分析的重点是2016年9月锡安地区观测到的18个山谷风日。只有增加土壤湿度和减小网格间距才能显著改善锡安地区的模拟流态。这包括沃利斯地区更强、更均匀的沿山谷风,以及锡昂镇附近更真实的跨山谷风和温度剖面。结果表明,观测到的和模拟的近地面风之间的剩余差异可能是由于非常局部的地形特征造成的。小规模的丘陵,即使在更精细的模型网格上也无法解决,导致山谷横截面的收缩和锡安地区观测到的低空上山谷风的加速。
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