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Idealized large-eddy simulations of nocturnal low-level jets over subtropical desert regions and implications for dust-generating winds

机译:亚热带沙漠地区夜间低空急流的理想大涡模拟及其对扬尘风的影响

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摘要

Nocturnal low-level jets (LLJs) are maxima in the wind profile, which often form above the stable nocturnal boundary layer. Over the Sahara, the world's largest source of mineral dust, this phenomenon is of particular importance to the emission and transport of desert aerosol. We present the first ever detailed large-eddy simulations of dust-generating LLJs. Using sensitivity studies with the UK Met Office large-eddy model (LEM), two key controls of the nocturnal LLJ are investigated: surface roughness and the Coriolis force. Functional relationships derived from the LEM results help to identify optimal latitude-roughness configurations for a maximum LLJ enhancement. Ideal conditions are found in regions between 20 and 27°N with roughness lengths >0.0001 m providing long oscillation periods and large jet amplitudes. Typical LLJ enhancements reach up to 3.5 m s for geostrophic winds of 10 m s. The findings are largely consistent with results from a theoretical LLJ model applied for comparison. The results demonstrate the importance of latitude and roughness in creating regional patterns of LLJ influence. Combining the functional relationships with high-resolution roughness data over northern Africa gives good agreement with the location of morning dust uplift in satellite observations. It is shown that shear-induced mixing plays an important role for the LLJ evolution and surface gustiness. With decreasing latitude the LLJ oscillation period is longer and, thus, shear-induced mixing is weaker, allowing a more stable nocturnal stratification to develop. This causes a later and more abrupt LLJ breakdown in the morning with stronger gusts, which can compensate for the slower LLJ evolution that leads to a weaker jet maximum. The findings presented here can serve as the first step towards a parametrization to improve the representation of the effects of nocturnal LLJs on dust emission in coarser-resolution models.
机译:夜间低空急流(LLJs)是风廓线中的最大值,通常在稳定的夜间边界层上方形成。在撒哈拉沙漠(世界上最大的矿物粉尘源)上,这种现象对于沙漠气溶胶的排放和运输尤为重要。我们展示了有史以来第一个详细的产生粉尘低空喷气飞机的大涡模拟。使用UK Met Office大涡模型(LEM)进行的敏感性研究,研究了夜间LLJ的两个关键控制因素:表面粗糙度和科里奥利力。从LEM结果得出的功能关系有助于确定最佳的纬度-粗糙度配置,以实现最大的LLJ增强。在20至27°N之间的区域中找到理想条件,粗糙度长度> 0.0001 m,可提供较长的振荡周期和较大的喷射幅度。对于10 m s的地转风,典型的LLJ增强可达3.5 m s。这些发现与用于比较的理论LLJ模型的结果基本一致。结果表明,纬度和粗糙度对创建LLJ影响的区域模式非常重要。将功能关系与北非的高分辨率粗糙度数据相结合,可以与卫星观测中早晨扬尘的位置很好地吻合。结果表明,剪切诱导的混合对于LLJ的演化和表面的味觉起着重要的作用。随着纬度的减小,LLJ振荡周期会更长,因此,剪切诱导的混合作用会减弱,从而使夜间分层更加稳定。这会导致早晨的LLJ击穿较晚且更突然,且阵风更强,这可以弥补LLJ的缓慢演变,从而导致最大射流变弱。此处介绍的发现可作为朝着参数化迈出的第一步,以提高夜间分辨率的LLJ对粉尘排放的影响。

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