A New Comprehensive Data Set of Solar Filaments of 100 yr Interval. I.
文献类型：期刊论文
| 作者 | Lin,GangHua2 ; Zhu,GaoFei2,3,4; Yang,Xiao2; Song,YongLiang2; Zhang,Mei2,3; Liu,Suo2,3; Wang,XiaoFan2; Su,JiangTao2,3; Zheng,Sheng5; Zhang,JiaFeng4,5
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| 刊名 | The Astrophysical Journal Supplement Series
 |
| 出版日期 | 2020-07-01 |
| 卷号 | 249期号:1 |
| ISSN号 | 0067-0049 |
| 关键词 | Solar filaments Solar chromosphere Astronomy data analysis Astronomy databases Astronomy data visualization |
| DOI | 10.3847/1538-4365/ab92a5 |
| 英文摘要 | Abstract Filaments are very common physical phenomena on the Sun and are often taken as important proxies of solar magnetic activities. The study of filaments has become a hot topic in the space weather research. For a more comprehensive understanding of filaments, especially for an understanding of solar activities of multiple solar cycles, it is necessary to perform a combined multifeature analysis by constructing a data set of multiple solar cycle data. To achieve this goal, we constructed a centennial data set that covers the Hα data from five observatories around the world. During the data set construction, we encountered varieties of problems, such as data fusion, accurate determination of the solar edge, classifying data by quality, dynamic threshold, and so on, which arose mainly due to multiple sources and a large time span of data. But fortunately, these problems were well solved. The data set includes seven types of data products and eight types of feature parameters with which we can implement the functions of data searching and statistical analyses. It has the characteristics of better continuity and highly complementary to space observation data, especially in the wavelengths not covered by space observations, and covers many solar cycles (including more than 60 yr of high-cadence data). We expect that this new comprehensive data set as well as the tools will help researchers to significantly speed up their search for features or events of interest, for either statistical or case study purposes, and possibly help them get a better and more comprehensive understanding of solar filament mechanisms. |
| 语种 | 英语 |
| 出版者 | The American Astronomical Society |
| WOS记录号 | IOP:0067-0049-249-1-AB92A5 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/63311]  |
| 专题 | 中国科学院国家天文台 |
| 作者单位 | 1.Institute for Space Weather Sciences, New Jersey Institute of Technology, Newark, NJ 07102-1982, USA 2.CAS Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People's Republic of China; lgh@nao.cas.cn 3.School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China 4.University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China 5.College of Science, China Three Gorges University, Yichang 443002, People's Republic of China |
| 推荐引用方式 GB/T 7714 | Lin,GangHua,Zhu,GaoFei,Yang,Xiao,et al. A New Comprehensive Data Set of Solar Filaments of 100 yr Interval. I.[J]. The Astrophysical Journal Supplement Series,2020,249(1). |
| APA | Lin,GangHua.,Zhu,GaoFei.,Yang,Xiao.,Song,YongLiang.,Zhang,Mei.,...&Xu,Yan.(2020).A New Comprehensive Data Set of Solar Filaments of 100 yr Interval. I..The Astrophysical Journal Supplement Series,249(1). |
| MLA | Lin,GangHua,et al."A New Comprehensive Data Set of Solar Filaments of 100 yr Interval. I.".The Astrophysical Journal Supplement Series 249.1(2020). |
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来源：国家天文台
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