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Modeling non-equilibrium atmospheric turbulence.

机译:模拟非平衡大气湍流。

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摘要

Reynolds-averaged turbulence modeling in meteorology is advanced by developing a new model, better suited than traditional ones for non-equilibrium atmospheric turbulent flows. Traditional models are based on equilibrium, most notably the local equilibrium assumption on the turbulent kinetic energy ( E) equation and/or algebraic equations for turbulence length scale, l, designed for classical quasi-steady, one-dimensional atmospheric boundary layers (1D-ABLs). The validity of these models is therefore questionable for non-equilibrium flows.; The new model is of E-ϵ type, computing eddy viscosities as Kα = cα E2/ϵ (α an arbitrary quantity) with transport equations for E and its dissipation rate, ϵ. The model thus prognostically calculates lE 3/2/ϵ, allowing sensitivity to non-equilibrium. Stability functions, cα, derived from second-order closure equations, are functions of static stability and the deviation of E from its local equilibrium value. The novel element is a modified ϵ-equation, of standard form but with coefficients altered or functions for them introduced to correct predictive failures of the standard equation for neutral and stable 1D-ABLs. The modifications result from mathematical analyses to enforce equation consistency with 1D-ABL theory.; The modified E-ϵ model is applied to the one-dimensional neutral-to-stable transitional ABL to assess its predictive improvements over traditional models for three non-equilibrium flows: the evening transition, residual layer and “very stable” ABL. The new model accurately predicts ABL bulk quantities and turbulence profiles for these cases, outperforming traditional models. This is attributed to its prediction of growing l with time in decaying, stably-stratified turbulence. Although counterintuitive, since l is generally thought limited in strong stability, growth is appropriate for shifting the dominant sink terms in the second-order closure equations basing the model from dissipation and slow pressure redistribution to buoyancy destruction as EN/ϵ approaches infinity in decaying turbulence (N being the Brunt-Vaisala frequency). Traditional models are either inconsistent with decaying turbulence or limit l in stable stratification regardless of turbulence state, leading to their reduced accuracy.; The success of the new model is promising for research on non-equilibrium atmospheric turbulent flows of decaying, stably-stratified turbulence through three-dimensional Reynolds-averaged computation. Investigation of non-equilibrium flows of growing turbulence and incorporation into weather and climate codes necessitate model extension to buoyantly driven flows, a future research task.
机译:通过开发新的模型来改进气象学中的雷诺平均湍流模型,该模型比传统模型更适合于非平衡大气湍流。传统模型基于平衡,最显着的是基于湍流长度尺度的湍动能( E )方程和/或代数方程的局部平衡假设,经典的准稳定一维大气边界层(1D-ABLs)。因此,这些模型的有效性对于非平衡流是值得怀疑的。新模型是 E -&epsiv;类型,计算涡流粘度为 K α = c α E 2 /&epsiv; (α为任意量),其中包含 E 的传输方程及其耗散率&epsiv;。该模型因此预测了 l E 3/2 /&epsiv ;,从而对非平衡敏感。由二阶闭合方程导出的稳定性函数 c α是静态稳定性的函数,也是 E 与其局部平衡值的偏差。该新颖元素是标准形式的修改的等式,但是系数发生了变化或引入了它们的功能,以纠正中性和稳定1D-ABL的标准方程式的预测失效。修改来自数学分析,以使方程与1D-ABL理论保持一致。修改后的 E -&epsiv;将该模型应用于一维中性到稳定的过渡ABL,以评估其相对于传统模型对三种非平衡流的预测性改进:晚过渡,残余层和“非常稳定” ABL。新模型可以准确预测这些情况下的ABL体积和湍流曲线,优于传统模型。这归因于其预测在逐渐稳定分层的湍流中随时间增长的 l 。尽管违反直觉,但由于通常认为 l 在强稳定性方面受到限制,因此增长适合将基于模型从耗散和缓慢的压力再分布到浮力破坏的二阶闭合方程中的主要下沉项转移为< italic> EN /&epsiv;在衰减湍流中接近无穷大( N 是Brunt-Vaisala频率)。传统模型要么与衰减湍流不一致,要么在稳定分层中限制 l ,而不管湍流状态如何,从而导致精度降低。通过三维雷诺平均计算,新模型的成功对于研究衰减的,稳定分层的湍流的非平衡大气湍流是有希望的。对湍流不断增长的非平衡流的研究以及将其纳入天气和气候法规中,需要将模型扩展至浮力驱动的流,这是未来的研究任务。

著录项

  • 作者

    Freedman, Frank Ronald.;

  • 作者单位

    Stanford University.;

  • 授予单位 Stanford University.;
  • 学科 Physics Atmospheric Science.; Geophysics.
  • 学位 Ph.D.
  • 年度 2003
  • 页码 152 p.
  • 总页数 152
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 大气科学(气象学);地球物理学;
  • 关键词

  • 入库时间 2022-08-17 11:44:50

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