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A new formulation of #sigma# _y and #sigma# _z for air quality dispersion models

机译:用于空气质量扩散模型的#sigma#_y和#sigma#_z的新公式

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A general formulation for estimating dispersion parameters #sigma# _y and #sigma# _z in the Planetary Boundary Layer (PBL) is proposed. These parmeterizations can be utilised in Gaussian air quality dispersion models for regulatory applications. They are based on the classical Taylor's statistical diffusion theory and on the modelled turbulent kinetic energy spectra and represents an extension of previous models (Degrazia et al.~(1,2)) which were mainly focused on dispersion in a purely convective or in a purely mechanic boundary layer. The sigmas proposed here allow to treat the dispersion in a boundary layer where both buoyancy and shear are important forcing mechanisms. The improved parameterization, inserted in a Gaussian model, has been validated using SF_6 tracer data taken from dispersion experiments.
机译:提出了用于估计行星边界层(PBL)中的色散参数#sigma#_y和#sigma#_z的一般公式。这些参数化可以在高斯空气质量扩散模型中用于监管应用。它们基于经典的泰勒统计扩散理论和建模的湍动能谱,并且代表了先前模型(Degrazia等人,(1,2))的扩展,这些模型主要集中于纯对流或纯对流中的弥散。纯机械边界层。此处提出的sigma可以处理边界层中的分散,其中浮力和剪切力都是重要的强迫机制。使用从色散实验中获得的SF_6示踪剂数据验证了插入高斯模型中的改进参数设置。

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