首页> 外文期刊>International Journal of High Performance Computing Applications >HIGH-RESOLUTION MESH CONVERGENCE PROPERTIES AND PARALLEL EFFICIENCY OF A SPECTRAL ELEMENT ATMOSPHERIC DYNAMICAL CORE
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HIGH-RESOLUTION MESH CONVERGENCE PROPERTIES AND PARALLEL EFFICIENCY OF A SPECTRAL ELEMENT ATMOSPHERIC DYNAMICAL CORE

机译:光谱元素大气动力学核的高分辨率网格收敛特性和并行效率

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We first demonstrate the parallel performance of the dynamical core of a spectral element atmospheric model. The model uses continuous Galerkin spectral elements to dis-cretize the surface of the Earth, coupled with finite differences in the radial direction. Results are presented from two distributed memory, mesh interconnect supercomputers (ASCI Red and BlueGene/L), using a two-dimensional space filling curve domain decomposition. Better than 80% parallel efficiency is obtained for fixed grids on up to 8938 processors. These runs represent the largest processor counts ever achieved for a geophysical application. They show that the upcoming Red Storm and BlueGene/L supercomputers are well suited for performing global atmospheric simulations with a 10 km average grid spacing. We then demonstrate the accuracy of the method by performing a full three-dimensional mesh refinement convergence study, using the primitive equations to model breaking Rossby waves on the polar vortex. Due to the excellent parallel performance, the model is run at several resolutions up to 36 km with 200 levels using only modest computing resources. Isosurfaces of scaled potential vorticity exhibit complex dynamical features, e.g. a primary potential vorticity tongue, and a secondary instability causing roll-up into a ring of five smaller subvortices. As the resolution is increased, these features are shown to converge while potential vorticity gradients steepen.
机译:我们首先展示光谱元素大气模型动力核心的并行性能。该模型使用连续的Galerkin光谱元素来离散化地球表面,并在径向上施加有限的差异。使用二维空间填充曲线域分解,从两个分布式内存,网格互连超级计算机(ASCI Red和BlueGene / L)中给出了结果。对于多达8938个处理器的固定网格,可获得高于80%的并行效率。这些运行代表了地球物理应用有史以来最大的处理器数量。他们表明即将推出的Red Storm和BlueGene / L超级计算机非常适合于以10 km的平均网格间距执行全球大气模拟。然后,我们通过执行完整的三维网格细化收敛性研究来证明该方法的准确性,该研究使用原始方程式对极涡上的破碎Rossby波建模。由于出色的并行性能,该模型仅使用少量的计算资源就可以在200 km的水平下以高达36 km的多种分辨率运行。等比例的潜在涡度等值面表现出复杂的动力学特征,例如主要的潜在涡旋性舌状物,以及次要的不稳定性会导致卷成五个较小的子涡流环。随着分辨率的提高,这些特征会收敛,而潜在的涡度梯度会变陡。

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