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Disaggregation of screen-level variables in a numerical weather prediction model with an explicit simulation of subgrid-scale land-surface heterogeneity

机译:数值天气预报模型中屏幕级变量的分解,并带有次网格规模土地表面异质性的显式模拟

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The earth's surface is characterized by small-scale heterogeneity attributable to variability in land cover, soil characteristics and orography. In atmospheric models, this small-scale variability can be partially accounted for by the so-called mosaic approach, i.e., by computing the land-surface processes on a grid with an explicit higher horizontal resolution than the atmosphere. The mosaic approach does, however, not account for the subgrid-scale variability in the screen-level atmospheric parameters, part of which might be related to land-surface heterogeneity itself. In this study, simulations with the numerical weather prediction model COSMO are shown, employing the mosaic approach together with a spatial disaggregation of the atmospheric forcing by the screen-level variables to the subgrid-scale. The atmospheric model is run with a 2.8 km horizontal grid resolution while the land surface processes are computed on a 400-m horizontal grid. The disaggregation of the driving atmospheric variables at screen-level is achieved by a three-step statistical downscaling with rules learnt from high-resolution fully coupled COSMO simulations, where both, atmosphere and surface, were simulated on a 400-m grid. The steps encompass spline interpolation of the grid scale variables, conditional regression based on the high-resolution runs, and an optional stochastic noise generator which restores the variability of the downscaled variables. Simulations for a number of case studies have been carried out, with or without mosaic surface representation and with or without atmospheric disaggregation, and evaluated with respect to the surface state variables and the turbulent surface exchange fluxes of sensible and latent heat. The results are compared with the high-resolution fully coupled COSMO simulations. The results clearly demonstrate the high importance of accounting for subgrid-scale surface heterogeneity. It is shown that the atmospheric disaggregation leads to clear additional improvements in the structures of the two-dimensional surface state variable fields, but to only marginally impacts on the simulation of the turbulent surface exchange fluxes. A detailed analysis of these results identifies strongly correlated errors in atmospheric and surface variables in the mosaic approach as the main reason for the latter. The effects of these errors largely cancel out in the flux parameterization, and thus explain the comparably good results for the fluxes in the mosaic approach without atmospheric disaggregation despite inferior performance for the surface state variables themselves. Inserting noise in the disaggregation scheme leads to a deterioration of the results.
机译:地球表面的特征是小范围的异质性,这归因于土地覆盖率,土壤特征和地形的变化。在大气模型中,这种小规模的变化可以通过所谓的镶嵌方法部分解决,即通过计算网格上具有明显高于大气水平分辨率的陆地表面过程。然而,镶嵌方法并没有考虑屏幕层大气参数的亚网格尺度变异性,其中一部分可能与地表异质性本身有关。在这项研究中,显示了使用数值天气预报模型COSMO进行的模拟,其中采用了镶嵌方法,并通过屏幕级别的变量对子网格规模对大气强迫进行了空间分解。大气模型以2.8 km的水平网格分辨率运行,而地面过程是在400 m的水平网格上计算的。在屏幕级别上,通过三个步骤进行统计缩小,可以从高分辨率的完全耦合COSMO仿真中获悉规则,从而在屏幕级别上分解驱动大气变量,其中在400 m网格上模拟了大气和地面。这些步骤包括网格比例变量的样条插值,基于高分辨率运行的条件回归以及可选的随机噪声发生器,该随机噪声发生器可恢复缩小比例变量的可变性。在有或没有镶嵌表面表示以及有或没有大气分解的情况下,已经进行了许多案例研究的模拟,并针对表面状态变量以及显热和潜热的湍流表面交换通量进行了评估。将结果与高分辨率的完全耦合COSMO仿真进行比较。结果清楚地表明了考虑亚网格规模表面异质性的高度重要性。结果表明,大气分解导致二维表面状态变量场结构的明显改善,但对湍流表面交换通量的模拟仅产生很小的影响。对这些结果的详细分析确定了镶嵌方法中大气变量和表面变量的高度相关误差,这是后者的主要原因。这些误差的影响在通量参数化中基本抵消了,因此,尽管表面状态变量本身的性能较差,但在没有大气分解的情况下,可以解释镶嵌方法中通量的相对较好结果。在分解方案中插入噪声会导致结果变差。

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