IBM-SP系统上可压缩湍流的高分辨率模拟

A. Mirin, R. Cohen, B. C. Curtis, W. Dannevik, A. Dimits, M. A. Duchauneau, D. Eliason, D. Schikore, S. E. Anderson, D. Porter, P. Woodward, L. Shieh, Steven W. White
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引用次数: 92

摘要

了解可压缩流中的湍流和混合对于化学燃烧和超新星演化等现实应用具有重要意义。在三维和非常高的分辨率下运行的能力是模拟准确地表示各种长度尺度的相互作用所必需的,因此,混合物种的反应性。为此,我们在位于劳伦斯利弗莫尔国家实验室的IBM持续管理TeraOp (SST)系统上进行了非常高分辨率(超过80亿个区域)的richmyer - meshkov不稳定性和湍流混合的三维模拟,该系统是在能源部(DOE)加速战略计算计划(ASCI)的支持下开发的。我们还在IBM系统的5832个处理器上进行了更高分辨率的原理证明计算(超过240亿个区域),该计算以1.05 Tflop/s的持续速率执行了一个多小时,以及使用改进算法实现了1.18Tflop/s的持续速率的简短计算。完整的生产科学模拟,使用进一步修改的算法,使用IBM系统的3840个处理器,在一周多一点的时间内运行27,000个时间步,获得大约每秒0.6 teraflop(32位算术)的持续吞吐量。制作和后期处理了近30万个图形文件,其中包含超过3tb的数据。高分辨率的三维运行能力使我们能够获得更准确和详细的流体流动结构图像-特别是,通过长波长和短波长的相互作用模拟精细尺度结构的发展,阐明二维和三维湍流之间的差异,探索关于从不稳定流动到随着雷诺数增加而充分发展的湍流的猜想。并确定计算解相对于网格分辨率的收敛性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Very High Resolution Simulation of Compressible Turbulence on the IBM-SP System
Understanding turbulence and mix in compressible flows is of fundamental importance to real-world applications such as chemical combustion and supernova evolution. The ability to run in three dimensions and at very high resolution is required for the simulation to accurately represent the interaction of the various length scales, and consequently, the reactivity of the intermixin species. Toward this end, we have carried out a very high resolution (over 8 billion zones) 3-D simulation of the Richtmyer-Meshkov instability and turbulent mixing on the IBM Sustained Stewardship TeraOp (SST) system, developed under the auspices of the Department of Energy (DOE) Accelerated Strategic Computing Initiative (ASCI) and located at Lawrence Livermore National Laboratory. We have also undertaken an even higher resolution proof-of-principle calculation (over 24 billion zones) on 5832 processors of the IBM system, which executed for over an hour at a sustained rate of 1.05 Tflop/s, as well as a short calculation with a modified algorithm that achieved a sustained rate of 1.18Tflop/s. The full production scientific simulation, using a further modified algorithm, ran for 27,000 timesteps in slightly over a week of wall time using 3840 processors of the IBM system, clockin a sustained throughput of roughly 0.6 teraflop per second (32-bit arithmetic). Nearly 300,000 graphics files comprising over three terabytes of data were produced and post-processed. The capability of running in 3-D at high resolution enabled us to get a more accurate and detailed picture of the fluid-flow structure - in particular, to simulate the development of fine scale structures from the interactions of long-and short-wavelength phenomena, to elucidate differences between two-dimensional and three-dimensional turbulence, to explore a conjecture regarding the transition from unstable flow to fully developed turbulence with increasing Reynolds number, and to ascertain convergence of the computed solution with respect to mesh resolution.
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