Automatic Tracking Algorithm of Solar G-band Bright Points | |
Yang, YF1,2,3; Lin, JB2; Deng LH(邓林华)4 | |
2013 | |
会议名称 | 6th International Conference on Intelligent Networks and Intelligent Systems (ICINIS) |
会议日期 | 2013-11-01 |
会议地点 | Shenyang Inst Engn, Shenyang, PEOPLES R CHINA |
关键词 | tracking G-band bright points three dimensional space-time cube evolution |
页码 | 304-307 |
通讯作者 | Yang, YF (reprint author), Kunming Univ Sci & Technol, Fac Informat Engn & Automat, Yunnan Comp Technol Applicat Key Lab, Kunming, Peoples R China. |
英文摘要 | In this paper, we present an automatic tracking algorithm to study the evolution of G-band bright points (GBPs) in the solar photosphere. A data set of 142 G-band speckled images obtained with the Dutch Open Telescope (DOT) on October 19, 2005 is used. The LMD algorithm is used to identify the GBPS in every image of the sequence. A three dimensional space-time cube is adopted to track the isolated and nonisolated GBPs. The three dimensional cylindrical tubes stand for the isolated GBPs and the three dimensional coral-like structures stand for the nonisolated GBPs. They are labeled with 26-adjacent method. The algorithm is useful and efficient for observing the whole evolution process of GBPs. The lifetime distribution of GBPs is fitted with exponential function well. The maximum lifetime of isolated GBPs is only 20 minutes, but that of nonisolated GBPs can reach 70 minutes through the whole image sequence. |
收录类别 | EI ; CPCI |
产权排序 | 第四完成单位 |
会议网址 | http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6754734 |
会议录 | Proceedings - 2013 6th International Conference on Intelligent Networks and Intelligent Systems, ICINIS 2013 |
会议录出版者 | IEEE |
会议录出版地 | 345 E 47TH ST, NEW YORK, NY 10017 USA |
学科主题 | Computer Science |
语种 | 英语 |
ISBN号 | 978-1-4799-2808-8 |
WOS记录号 | WOS:000345841800079 |
研究领域[WOS] | Computer Science |
内容类型 | 会议论文 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/4862] |
专题 | 云南天文台_抚仙湖太阳观测站 |
作者单位 | 1.Yunnan Computer Technology Application Key Lab / Faculty of Information Engineering and Automation, Kunming University of Science and Technology, Kunming, China 2.Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China 3.Key Laboratory of Modern Astronomy and Astrophysics, Nanjing UniversityˈMinistry of Education, Nanjing, China 4.Yunnan Astronomical Observatory, National Astronomical Observatories, Chinese Academy of Sciences, Kunming, China |
推荐引用方式 GB/T 7714 | Yang, YF,Lin, JB,Deng LH. Automatic Tracking Algorithm of Solar G-band Bright Points[C]. 见:6th International Conference on Intelligent Networks and Intelligent Systems (ICINIS). Shenyang Inst Engn, Shenyang, PEOPLES R CHINA. 2013-11-01.http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6754734. |
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