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Coupled Analysis and Visualization of High Resolution Astrophysical Simulations

机译:高分辨率天体物理模拟的耦合分析与可视化

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Computational physics has benefited from on-going microproces-sor innovations, which have enabled larger and larger numerical simulations. One consequence of these technological advancements has been an explosion in the amount of data generated. For many modelers, available software tools and computing resources are proving inadequate for investigation of high-resolution numerical outputs. In this paper we discuss the general problems associated with very large data visualization and analysis and our work on a particular solution to those through the development of VAPOR (open source, available at http://www.vapor.ucar.edu): a desktop application that leverages today's powerful CPUs and GPUs to enable visualization and analysis of terascale data sets using only a commodity PC or laptop. We briefly illustrate VAPOR's utility through the exploration of a high-resolution simulation aimed at understanding the effects of hydrogen ionization on convective dynamics in stellar envelopes.
机译:计算物理受益于正在进行的微局 - SOR创新,这使得能够更大,数值模拟。这些技术进步的一种后果一直是生成的数据量的爆炸。对于许多建模者来说,可用的软件工具和计算资源证明了对高分辨率数值输出的调查不足。在本文中,我们讨论了与非常大的数据可视化和分析相关的一般问题,以及通过蒸汽开发的特定解决方案的特定解决方案(在http://www.vapor.ucar.edu提供):a桌面应用程序,利用当今强大的CPU和GPU,只使用商品PC或笔记本电脑实现TeraScale数据集的可视化和分析。通过探索旨在了解氢离子化对恒星信封对流动力学的影响,简要说明蒸气的效用。

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