Very Large Scale Visualization Methods for Astrophysical Data

dc.contributor.authorHanson, Andrew J.en_US
dc.contributor.authorFu, Chi-Wingen_US
dc.contributor.authorWernert, Eric A.en_US
dc.contributor.editorW. de Leeuw and R. van Liereen_US
dc.date.accessioned2014-01-30T06:41:34Z
dc.date.available2014-01-30T06:41:34Z
dc.date.issued2000en_US
dc.description.abstractWe address the problem of interacting with scenes that contain a very large range of scales. Computer graphics environments normally deal with only a limited range of orders of magnitude before numerical error and other anomalies begin to be apparent, and the effects vary widely from environment to environment. Applications such as astrophysics, where a single scene could in principle contain visible objects from the subatomic scale to the intergalactic scale, provide a good proving ground for the multiple scale problem. In this context, we examine methods for interacting continuously with simultaneously active astronomical data sets ranging over 40 or more orders of magnitude. Our approach relies on utilizing a single scale of order 1.0 for the definition of all data sets. Where a single object, like a planet or a galaxy, may require moving in neighborhoods of vastly different scales, we employ multiple scale representations for the single object; normally, these are sparse in all but a few neighborhoods. By keying the changes of scale to the pixel size, we can restrict all data set scaling to roughly four orders of magnitude. Navigation problems are solved by designing constraint spaces that adjust properly to the large scale changes, keeping navigation sensitivity at a relatively constant speed in the user s screen space.en_US
dc.description.seriesinformationEurographics / IEEE VGTC Symposium on Visualizationen_US
dc.identifier.isbn3211835156en_US
dc.identifier.issn1727-5296en_US
dc.identifier.urihttps://doi.org/10.2312/VisSym/VisSym00/115-124en_US
dc.publisherThe Eurographics Associationen_US
dc.titleVery Large Scale Visualization Methods for Astrophysical Dataen_US
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