Fiedler S, Schepanski K, Heinold B, Knippertz P, Tegen I
School of Earth and Environment, University of Leeds Leeds, UK.
School of Earth and Environment, University of Leeds Leeds, UK ; Now at Leibniz Institute for Tropospheric Research Leipzig, Germany.
J Geophys Res Atmos. 2013 Jun 27;118(12):6100-6121. doi: 10.1002/jgrd.50394. Epub 2013 Jun 21.
[1] This study presents the first climatology for the dust emission amount associated with Nocturnal Low-Level Jets (NLLJs) in North Africa. These wind speed maxima near the top of the nocturnal boundary layer can generate near-surface peak winds due to shear-driven turbulence in the course of the night and the NLLJ breakdown during the following morning. The associated increase in the near-surface wind speed is a driver for mineral dust emission. A new detection algorithm for NLLJs is presented and used for a statistical assessment of NLLJs in 32 years of ERA-Interim reanalysis from the European Centre for Medium-Range Weather Forecasts. NLLJs occur in 29% of the nights in the annual and spatial mean. The NLLJ climatology shows a distinct annual cycle with marked regional differences. Maxima of up to 80% NLLJ frequency are found where low-level baroclinicity and orographic channels cause favorable conditions, e.g., over the Bodélé Depression, Chad, for November-February and along the West Saharan and Mauritanian coast for April-September. Downward mixing of NLLJ momentum to the surface causes 15% of mineral dust emission in the annual and spatial mean and can be associated with up to 60% of the total dust amount in specific areas, e.g., the Bodélé Depression and south of the Hoggar-Tibesti Channel. The sharp diurnal cycle underlines the importance of using wind speed information with high temporal resolution as driving fields for dust emission models. Fiedler, S., K. Schepanski, B. Heinold, P. Knippertz, and I. Tegen (2013), Climatology of nocturnal low-level jets over North Africa and implications for modeling mineral dust emission, J. Geophys. Res. Atmos., 118, 6100-6121, doi:10.1002/jgrd.50394.
[1] 本研究给出了与北非夜间低空急流(NLLJs)相关的沙尘排放量的首个气候学研究成果。夜间边界层顶部附近的这些风速最大值,会因夜间剪切驱动的湍流以及次日早晨NLLJ的崩溃,而产生近地表峰值风。近地表风速的相应增加是矿物沙尘排放的一个驱动因素。本文提出了一种新的NLLJs检测算法,并将其用于对欧洲中期天气预报中心32年的ERA-Interim再分析资料中NLLJs的统计评估。在年平均和空间平均中,NLLJs出现在29%的夜晚。NLLJ气候学呈现出明显的年周期,且存在显著的区域差异。在低空斜压性和地形通道造成有利条件的地方,发现NLLJ频率最高可达80%,例如在11月至2月期间的乍得博德莱洼地,以及4月至9月期间沿西撒哈拉和毛里塔尼亚海岸。NLLJ动量向下混合至地表,在年平均和空间平均中导致15%的矿物沙尘排放,在特定区域,例如博德莱洼地和霍加尔-提贝斯提通道以南,这一比例可高达总沙尘量的60%。急剧的日变化周期凸显了使用具有高时间分辨率的风速信息作为沙尘排放模型驱动场的重要性。菲德勒,S.,K. 舍潘斯基,B. 海诺尔德,P. 克尼珀茨,以及I. 特根(2013年),《北非夜间低空急流的气候学及其对矿物沙尘排放建模的影响》,《地球物理学研究杂志:大气》,118,6100 - 6121,doi:10.1002/jgrd.50394 。