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Exploring a global multiresolution modeling approach using aquaplanet simulations.

机译:探索使用水上行星模拟的全球多分辨率建模方法。

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Results from aquaplanet experiments performed using the Model for Prediction across Scales (MPAS) hydrostatic dynamical core implemented within the Department of Energy (DOE)-NCAR Community Atmosphere Model (CAM) are presented. MPAS is an unstructured-grid approach to climate system modeling that supports both quasi-uniform and variable-resolution meshing of the sphere based on conforming grids. Using quasi-uniform simulations at resolutions of 30, 60, 120, and 240 km, the authors evaluate the performance of CAM-MPAS via its kinetic energy spectra, general circulation, and precipitation characteristics. By analyzing an additional variable-resolution simulation with grid spacing that varies from 30 km in a spherical, continental-sized equatorial region to 240 km elsewhere, the CAM-MPAS's potential for use as a regional climate simulation tool is explored. Similar to other quasi-uniform aquaplanet simulations, tropical precipitation increases with resolution, indicating the resolution sensitivity of the physical parameterizations. Comparison with the finite volume (FV) dynamical core suggests a weaker tropical circulation in the CAM-MPAS simulations, which is evident in reduced tropical precipitation and a weaker Hadley circulation. In the variable-resolution simulation, the kinetic energy spectrum within the high-resolution region closely resembles the quasi-uniform 30-km simulation, indicating a robust simulation of the fluid dynamics. As suggested by the quasi-uniform simulations, the CAM4 physics behave differently in the high and low resolution regions. A positive precipitation anomaly occurs on the western edge of the high-resolution region, exciting a Gill-type response; this zonal asymmetry represents the errors incurred in a variable resolution setting. When paired with a multiresolution mesh, the aquaplanet test case offers an exceptional opportunity to examine the response of physical parameterizations to grid resolution.
机译:介绍了使用在能源部(DOE)-NCAR社区大气模型(CAM)中实施的跨尺度预测模型(MPAS)静水动力核心进行的滑水行星实验的结果。 MPAS是一种用于气候系统建模的非结构化网格方法,它支持基于一致网格的球体的准均匀和可变分辨率网格划分。使用分辨率分别为30、60、120和240 km的准均匀模拟,作者通过其动能谱,总体环流和降水特征评估了CAM-MPAS的性能。通过分析网格间距从球形,大陆性赤道区域的30 km到其他地方的240 km的网格的可变分辨率模拟,探索了CAM-MPAS用作区域气候模拟工具的潜力。与其他准均匀的水上行星模拟相似,热带降水随着分辨率增加而增加,表明物理参数化的分辨率敏感性。与有限体积(FV)动力核心的比较表明,在CAM-MPAS模拟中,热带环流减弱,这在热带降水减少和Hadley环流减弱中很明显。在可变分辨率模拟中,高分辨率区域内的动能谱与准均匀30公里模拟非常相似,表明流体动力学的鲁棒性模拟。正如准均匀模拟所建议的那样,CAM4物理在高分辨率和低分辨率区域的行为是不同的。在高分辨率区域的西边缘出现正降水异常,激发了吉尔型响应;这种区域不对称性表示可变分辨率设置中产生的误差。当与多分辨率网格配对时,滑水板测试用例提供了一个难得的机会来检查物理参数化对网格分辨率的响应。

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