Visualizing the Universe

M. Geller, E. E. Flaco, D. Fabricant, B. Estus
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引用次数: 3

Abstract

A Universe mapping project at the Harvard-Smithsonian Center for Astrophysics (CfA), called the CfA Redshift Survey, is described. The line-of-sight recession velocities of galaxies are measured by identifying absorption and emission lines in their spectra. With the two angular positions of a galaxy on the sky and a measurement of its red-shift, each galaxy can be placed in a three-dimensional (3-D) map of the Universe. It is shown that visualization techniques are important for exploring and analyzing the data, for comparing the data with models, and for designing the future. Computer animation of the data is a way of bringing the maps before the public.<>
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可视化宇宙
描述了哈佛-史密森天体物理中心(CfA)的一个宇宙测绘项目,称为CfA红移调查。星系的视距衰退速度是通过识别其光谱中的吸收线和发射线来测量的。有了星系在天空中的两个角度位置和对其红移的测量,每个星系都可以被放置在三维(3-D)宇宙地图中。研究表明,可视化技术对于探索和分析数据、将数据与模型进行比较以及设计未来具有重要意义。数据的电脑动画是将地图呈现在公众面前的一种方式
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