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A non-hydrostatic atmospheric model for the simulation of stratospheric mountain waves

机译:用于模拟平流层山浪的非静水大气模型

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摘要

A review of existing solution methodology for non-hydrostatic atmospheric models identified the split-explicit timestepping approach as the preferred solution method for a new non-hydrostatic atmospheric model. The linear advectionequation was used for stability analysis of different combinations of time integration and advection schemes beforethe third order Runge-Kutta (RK3) time integration scheme was chosen. A number of one- and two-dimensional testproblems were then applied to the linear advection equation to study the robustness of the different finite differenceadvection schemes. It was found that the third and fifth order upwind advection schemes have good phase propertiesand are generally robust even in coarse grid resolutions. The RK3 time integration scheme with third and fifth orderupwind advection schemes were then applied to the split explicit formulation for the new non-hydrostatic atmosphericmodel. The model was verified with well known test cases of increasing complexity. The performance of the new modelwas compared with other established non-hydrostatic models. Due to the highly non-linear ow in the test case, therewas some variability in simulation results from the other models. Our new model simulation results were all withinthe average of the majority of the models and was not an outlier.A two-dimensional version of the new model was used to study mountain waves in the middle atmosphere over thesouthern Andes. Using realistic temperatures, winds and topography, the model simulations generate large amplitudelong wavelength breaking mountain waves in the middle atmosphere that compare favourably with satellite measure-ments. Modelled waves have preferred horizontal wavelengths. Spectral analysis reveals correspondences betweenwavelengths and peaks in the spectrum of Andean topographic elevations. The shorter waves reach the stratospherewell before the longer ones, consistent with group velocity arguments, with longer wavelengths ultimately dominating.At later times we find evidence of downward propagating secondary waves produced by upper level breaking of theprimary waves.
机译:对非静压大气模型的现有解决方案方法的回顾确定了采用显式分段时间步长法作为新的非静压大气模型的首选解决方法。在选择三阶Runge-Kutta(RK3)时间积分方案之前,将线性对流方程用于时间积分和对流方案不同组合的稳定性分析。然后将许多一维和二维测试问题应用于线性对流方程,以研究不同有限差分对流方案的鲁棒性。已经发现,三阶和五阶迎风对流方案具有良好的相位特性,即使在粗网格分辨率下也通常很健壮。然后,将具有第三级和第五级迎风对流方案的RK3时间积分方案应用于新的非静水大气模型的拆分显式公式。该模型已通过众所周知的复杂性不断增加的测试案例进行了验证。将新模型的性能与其他已建立的非静液压模型进行了比较。由于测试用例中的高度非线性流,其他模型的仿真结果存在一些差异。我们的新模型模拟结果均在大多数模型的平均值之内,而不是异常值。该模型的二维版本用于研究安第斯山脉南部中层大气中的山浪。使用现实的温度,风和地形,模型模拟在中层大气中产生了大振幅长的波长破碎山波,这与卫星测量结果相比具有优势。建模波具有首选的水平波长。光谱分析揭示了安第斯地形高程光谱中的波长和峰值之间的对应关系。较短的波先到达平流层井,然后到达较长的平流层井,这与群速度论证一致,较长的波长最终占主导地位。后来,我们发现了由初级波的高位破裂产生的向下传播的次级波的证据。

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