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A two Turbulence Kinetic Energy model as a scale-adaptive approach to modeling the planetary boundary layer

机译:两个湍流动能模型,作为尺度自适应方法,用于建模行星边界层

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摘要

A two Turbulence Kinetic Energy (2TKE) model is developed to address the boundary layer “grey zone” problem. The model combines ideas from local and nonlocal models into a single energetically consistent framework. By applying the Reynolds averaging to the large eddy simulation (LES) equations that employ Deardorff's subgrid TKE, we arrive at a system of equations for the boundary layer quantities and two turbulence kinetic energies: one which encapsulates the TKE of large boundary-layer-scale eddies and another which represents the energy of eddies subgrid to the vertical grid size of a typical large-scale model. These two energies are linked via the turbulent cascade of energy from larger to smaller scales and are used to model the mixing in the boundary layer. The model is evaluated for three dry test cases and found to compare favorably to large eddy simulations. The usage of two TKEs for mixing helps reduce the dependency of the model on the vertical grid scale as well as on the free tropospheric stability and facilitates a smoother transition from convective to stable regimes. The usage of two TKEs representing two ranges of scales satisfies the prerequisite for modeling the boundary layer in the “grey zone”: an idea that is explored further in a companion paper.
机译:开发了两个湍流动能(2TKE)模型来解决边界层“灰色区域”问题。该模型将来自本地和非本地模型的思想组合到一个单一的,能量一致的框架中。通过将雷诺平均方法应用于采用Deardorff子网格TKE的大型涡模拟(LES)方程,我们得出了一个关于边界层量和两种湍动能的方程组:一个将大边界层规模的TKE封装起来涡流和另一个代表涡流能量的网格,该能量细分为典型大型模型的垂直网格大小。这两个能量通过湍流级联从较大到较小的比例联系在一起,并用于对边界层中的混合进行建模。对三个干燥测试案例进行了模型评估,发现该模型可与大型涡流仿真进行比较。使用两个TKE进行混合有助于减少模型对垂直网格规模以及对流层自由稳定性的依赖性,并有助于从对流状态到稳定状态的平稳过渡。代表两个比例尺范围的两个TKE的使用满足了在“灰色区域”中对边界层建模的先决条件:这一想法将在随附的论文中进一步探讨。

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