Visualization of multivariate dark matter halos in cosmology simulations

Jay Takle, D. Silver, E. Kovacs, K. Heitmann
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引用次数: 5

Abstract

In this poster, we present a new approach to visualize multivariate dark matter halos representing the spheroid part of galaxies, the disk part of galaxies, black holes and the halo itself. The data being visualized here is an end result of tracking the evolution of cosmic structures called dark matter halos in cosmological simulation and evaluating the formation and evolution of galaxies within. Cosmologists have traditionally visualized individual galaxies in the form of two dimensional density maps, graphs and parallel coordinates. We introduce a new way of mapping multiple parameters of dark matter halos to a halo-icon. This allows the scientist to view all of the parameters associated with the dark matter halos in one visualization.
宇宙学模拟中多元暗物质晕的可视化
在这张海报中,我们提出了一种新的方法来可视化多元暗物质晕,它代表了星系的球体部分、星系的盘状部分、黑洞和晕本身。这里可视化的数据是在宇宙模拟中跟踪宇宙结构(称为暗物质晕)的演化并评估其中星系的形成和演化的最终结果。宇宙学家传统上以二维密度图、图形和平行坐标的形式将单个星系可视化。我们介绍了一种将暗物质晕的多个参数映射到晕标上的新方法。这使得科学家可以在一个可视化中查看与暗物质晕相关的所有参数。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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