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Evaluating models of the neutral, barotropic planetary boundary layer using integral measures: part II. modelling observed conditions

机译:使用积分测度评估中性,正压行星边界层的模型:第二部分。模拟观察条件

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摘要

The steady-state, horizontally homogeneous, neutral, barotropic case forms the foundation of our theoretical understanding of the planetary boundary layer (PBL). While simple analytical models and first-order closure models simulate atmospheric observations of this case well, more sophisticated models, in general, do not. In this paper we examine how well three higher-order closure models, E - #epsilon# - l, E - l, and LRR - l, which have been especially modified for PBL applications, perform in predicting the behaviour of the cross-isobaric angle #alpha#_0, the geostrophic drag coefficient C_g, and the integral of the dissipation rate over the boundary layer, as a function of the surface Rossby number Ro. For comparison we also examine the performance of three first-order closure mixing-length models, two proposed by A. K. Blackadar and one by H. H. Lettau, and the performance of the standard model for second-order closure and a modification of it designed to reduce the overprediction of turbulence in the upper part of the boundary layer.
机译:稳态,水平均匀,中性,正压的情况构成了我们对行星边界层(PBL)的理论理解的基础。虽然简单的分析模型和一阶闭合模型可以很好地模拟这种情况下的大气观测,但一般而言,复杂的模型却不能。在本文中,我们研究了为PBL应用特别修改的三种高阶闭合模型E-#epsilon#-l,E-l和LRR -l在预测交叉等压线的行为方面的表现如何角#alpha#_0,地转阻力系数C_g和边界层上的耗散率的积分,是表面Rossby数Ro的函数。为了进行比较,我们还研究了三个一阶封闭混合长度模型的性能,其中两个由AK Blackadar提出,一个由HH Lettau提出,以及用于二阶封闭的标准模型的性能以及对模型的修改,以减少对边界层上部湍流的过度预测。

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