可视化的黑暗天空IEEE SciVis竞赛2015

Theodoros Christoudias, C. Kallidonis, L. Koutsantonis, Christos Lemesios, Lefteris Markou, Constantinos Sophocleous
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引用次数: 5

摘要

宇宙模拟是我们理解宇宙137亿年历程的基石,从我们在宇宙微波背景中看到的微小波动到今天,我们被星系和星系团包围,这些星系和星系团由一个巨大的宇宙网相互连接。在本文中,我们展示了2015年IEEE科学可视化竞赛的结果,该竞赛涉及来自黑暗天空模拟的数据集[10]。我们摄取、处理和可视化粒子云和晕的位置形成的宇宙学数据,并阐明各种科学兴趣的属性,包括重力势、速度和自旋。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Visualising the dark sky IEEE SciVis contest 2015
Cosmological simulations are a cornerstone of our understanding of the Universe during its 13.7 billion year progression from small fluctuations that we see in the cosmic microwave background to today, where we are surrounded by galaxies and clusters of galaxies interconnected by a vast cosmic web. In this paper, we present our results on the 2015 IEEE Scientific Visualization Contest, which pertains to datasets derived from the Dark Sky Simulations [10]. We ingest, process and visualise cosmological data of particle clouds and halo formations in terms of positions and shed light on various properties of scientific interest including graviational potential, velocity and spin.
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