Akira Takeuchi, Hiromitsu Fujii, A. Yamashita, Masayuki Tanaka, R. Kataoka, Y. Miyoshi, M. Okutomi, H. Asama
{"title":"3D visualization of aurora from optional viewpoint at optional time","authors":"Akira Takeuchi, Hiromitsu Fujii, A. Yamashita, Masayuki Tanaka, R. Kataoka, Y. Miyoshi, M. Okutomi, H. Asama","doi":"10.1145/2820926.2820967","DOIUrl":null,"url":null,"abstract":"Three-dimensional analysis of the aurora is significant because the shape of aurora depends on solar wind which influences electric equipment such as satellites. Our research group set two fish-eye cameras in Alaska, U.S.A and reconstructed the Aurora's shape from a pair of stereo images [Fujii et al. 2014]. However, the method using the feature-based matching cannot detect dense enough feature points accurately since they are hard to detect from the aurora image whose most parts are with low contrast. In this paper, we achieved both increasing the detected feature points and improving accuracy. Applying this method, the 3D shape of aurora from optional view point at optional time can be visualized.","PeriodicalId":432851,"journal":{"name":"SIGGRAPH Asia 2015 Posters","volume":"15 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2015-11-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"SIGGRAPH Asia 2015 Posters","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1145/2820926.2820967","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 1
Abstract
Three-dimensional analysis of the aurora is significant because the shape of aurora depends on solar wind which influences electric equipment such as satellites. Our research group set two fish-eye cameras in Alaska, U.S.A and reconstructed the Aurora's shape from a pair of stereo images [Fujii et al. 2014]. However, the method using the feature-based matching cannot detect dense enough feature points accurately since they are hard to detect from the aurora image whose most parts are with low contrast. In this paper, we achieved both increasing the detected feature points and improving accuracy. Applying this method, the 3D shape of aurora from optional view point at optional time can be visualized.
极光的三维分析很重要,因为极光的形状取决于太阳风,而太阳风会影响卫星等电子设备。我们的研究小组在美国阿拉斯加设置了两台鱼眼相机,并从一对立体图像中重建了极光的形状[Fujii et al. 2014]。然而,基于特征匹配的方法很难从大部分对比度较低的极光图像中检测到足够密集的特征点,因此无法准确检测到这些特征点。在本文中,我们既增加了检测到的特征点,又提高了精度。应用该方法,可以实现任意时间、任意视点上的极光三维形状的可视化。