论文标题
使用教室中的Hubble Ultradeep字段数据的交互式宇宙学可视化
Interactive Cosmology Visualization Using the Hubble UltraDeep Field Data in the Classroom
论文作者
论文摘要
我们已经开发了一种基于Java的教学工具,即“欣赏Hubble在Hyper-Speed上”($ \ textit {ahah} $),该工具旨在在开始的天文学和宇宙学课程中使用学生和讲师,我们已在线提供。该工具使用户可以假设在$ \ sim500 \!\!\!\!10^{12} $ times Light的速度,从Redshifts $ z \!= \!0 $今天到$ z \!\!6 $ aft 1 gyr aft 1 gyr aft y light shift $ \ sim500 \!\!10^{12} $ times the Light的速度,在三个维度上穿越Hubble Ultra Deep Field(HUDF)(HUDF)。用户还可以以各种宇宙学配置和两种不同的几何模式查看宇宙 - 包括宇宙扩展的标准几何形状,以及静态的伪euclidean几何形状进行比较。在本文中,我们详细介绍了该Java应用程序功能的基础数学公式,并为使用这些特定公式提供了理由。其中包括在各种宇宙学中计算物体的角度大小的方式,以及如何在相对扩展的宇宙学中定义应用程序的坐标系。我们还简要讨论了用于选择和准备应用程序中图像的方法,用于测量星系红移的数据以及可视化的定性含义 - 也就是说,当用户在通过模拟中“移动”虚拟望远镜时确切地看到了什么。最后,我们对课堂教学工具的有效性进行了研究,其结果显示了该工具的功效,并以超过$ \ sim的$ \ sim $ 90%获得了学生的认可,并为其在课堂环境中的进一步使用提供了理由。
We have developed a Java-based teaching tool, "Appreciating Hubble at Hyper-speed" ($\textit{AHaH}$), intended for use by students and instructors in beginning astronomy and cosmology courses, which we have made available online. This tool lets the user hypothetically traverse the Hubble Ultra Deep Field (HUDF) in three dimensions at over $\sim500\!\times\!10^{12}$ times the speed of light, from redshifts $z\!=\!0$ today to $z\!=\!6$, about 1 Gyr after the Big Bang. Users may also view the Universe in various cosmology configurations and two different geometry modes - standard geometry that includes expansion of the Universe, and a static pseudo-Euclidean geometry for comparison. In this paper we detail the mathematical formulae underlying the functions of this Java application, and provide justification for the use of these particular formulae. These include the manner in which the angular sizes of objects are calculated in various cosmologies, as well as how the application's coordinate system is defined in relativistically expanding cosmologies. We also briefly discuss the methods used to select and prepare the images in the application, the data used to measure the redshifts of the galaxies, and the qualitative implications of the visualization - that is, what exactly users see when they "move" the virtual telescope through the simulation. Finally, we conduct a study of the effectiveness in this teaching tool in the classroom, the results of which show the efficacy of the tool, with over $\sim$90% approval by students, and provide justification for its further use in a classroom setting.