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Effects of Wind Shear on Pollution Dispersion

机译:风剪切对污染分散的影响

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Using an accurate numerical method for simulating advection and diffusion of pollution puffs, it is demonstrated that relatively small changes in wind speeds or direction with height induces appreciable horizontal dispersion that cannot be accurately simulated using classical puff diffusion models. Using idealized winds, it is shown that individual puffs of pollution preferentially disperse in the horizontal direction aligned with the mean wind shear vector in the atmospheric planetary boundary layer (PBL). Even if wind directions are constant in the PBL, the speed shear in the lowest constant flux surface layer induces appreciable horizontal dispersion along the mean wind direction. Using a more realistic and typical observed late afternoon PBL wind profile, it is shown that a Lagrangian puff model cannot reasonably simulate the observed transport and dispersion of a puff of pollution for a 3-4 hour period. These results suggest that shear-related dispersion effects are probably the dominant mechanism of horizontal dispersion in the atmosphere. For assessing long-range dispersion of atmospheric pollutants, the common assumption that pollutants disperse as spherical “puffs” is inherently inaccurate since the effects of horizontal dispersion along the direction of ambient wind shear experienced by a dispersing pollution puff are not accurately accounted for. If a puff model is used to assess long range transport and dispersion, it is demonstrated that if peak concentrations are correctly simulated, then the overall area impacted by pollution will be severely skewed, and there will be many areas where concentrations are severely over- or under-estimated. If larger horizontal puff dispersions are assumed so as to encompass the actual impact area, then peak concentrations calculated by Lagrangian puff model are severely underestimated. These results suggest that horizontal dispersion of pollutants should be proportional to the wind shear across the vertical depth of the atmosphere containing pollutants.
机译:使用精确的数值方法来模拟污染粉扑的平流和扩散,证明风速或高度的方向变化相对较小,可以使用经典的PUFF扩散模型准确地模拟可观的水平分散。使用理想化的风,示出了优先分散在与大气行星边界层(PBL)中的平均风剪切载体对准的水平方向上的各个污染的浮气。即使在PBL中的风向是恒定的,最低恒定磁通表面层的速度剪切也沿着平均风向引起可观的水平分散。使用更现实且典型的观察到的下午PBL风轮廓,表明拉格朗日粉扑模型不能合理地模拟3-4小时的污染的观察到的运输和分散。这些结果表明,剪切相关的分散效应可能是大气中水平分散的主导机制。为了评估大气污染物的远程分散,污染物分散为球形“浮搏”的共同假设本质上是不准确的,因为水平分散沿着分散污染粉扑的环境风剪的方向的影响不准确地占据。如果使用PUFF模型来评估长距离传输和分散,则证明如果正确模拟峰值浓度,则污染影响的总面积将严重倾斜,并且将有许多领域,浓度严重过度或估计不足。如果假设较大的水平浮夸分散,以便包含实际的冲击区域,则通过拉格朗日粉扑模型计算的峰值浓度严重低估。这些结果表明,污染物的水平分散应与含有污染物的大气垂直深度的风剪成比例。

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