EUV Wave Detection and Characterization Using Deep Learning
文献类型:期刊论文
作者 | Xu, Long2![]() ![]() |
刊名 | SOLAR PHYSICS
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出版日期 | 2020-03-19 |
卷号 | 295期号:3页码:14 |
关键词 | Coronal Mass Ejection (CME) Extreme Ultraviolet (EUV) waves Solar burst Deep neural network |
ISSN号 | 0038-0938 |
DOI | 10.1007/s11207-020-01612-4 |
英文摘要 | Coronal Mass Ejections (CMEs) are the most violent solar bursts. They cause severe disturbances in the solar-terrestrial space and affect human activities in many aspects, especially causing damage to high-tech infrastructure. It usually takes few hours for a CME to arrive at the Earth after eruption. Therefore, many efforts have been devoted to CME arrival time prediction, so that we have enough time to take action before a CME arrives at the Earth. For predicting CME arrival time, it is vital to detect the CME origin, arrival and departure speed in a coronagraph. It has been widely accepted that Extreme Ultraviolet (EUV) waves are associated with CMEs, so EUV waves are the signatures of CMEs as CMEs originate and traverse the solar disk, specifically for front-side CMEs. In this paper, two deep neural networks are developed to first detect EUV waves and then outline their wavefronts, giving early signatures of CMEs. Usually, CMEs are recorded by coronagraphs as they transit the corona, so our proposed method can obtain a certain time ahead compared with conventional CME forecasting. In addition, the parameters for describing EUV waves can be more easily deduced, benefiting the subsequent statistical analysis of CMEs. The experimental results demonstrate the effectiveness of the proposed model for detecting EUV waves and generating their outlines. |
WOS关键词 | EIT WAVES ; CORONAL WAVE |
资助项目 | National Natural Science Foundation of China (NSFC)[61572461] ; National Natural Science Foundation of China (NSFC)[61811530282] ; National Natural Science Foundation of China (NSFC)[61872429] ; National Natural Science Foundation of China (NSFC)[11790301] ; National Natural Science Foundation of China (NSFC)[11790305] ; Specialized Research Fund for State Key Laboratories[2018-026F-04] |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:000522137100002 |
出版者 | SPRINGER |
资助机构 | National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Specialized Research Fund for State Key Laboratories ; Specialized Research Fund for State Key Laboratories ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Specialized Research Fund for State Key Laboratories ; Specialized Research Fund for State Key Laboratories ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Specialized Research Fund for State Key Laboratories ; Specialized Research Fund for State Key Laboratories ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Specialized Research Fund for State Key Laboratories ; Specialized Research Fund for State Key Laboratories |
源URL | [http://ir.bao.ac.cn/handle/114a11/55324] ![]() |
专题 | 中国科学院国家天文台 |
通讯作者 | Xu, Long |
作者单位 | 1.Shenzhen Univ, Coll Math & Stat, Shenzhen 518060, Peoples R China 2.Chinese Acad Sci, Natl Astron Observ, Key Lab Solar Act, Beijing 100101, Peoples R China 3.Univ Chinese Acad Sci, Beijing 100049, Peoples R China |
推荐引用方式 GB/T 7714 | Xu, Long,Liu, Sixuan,Yan, Yihua,et al. EUV Wave Detection and Characterization Using Deep Learning[J]. SOLAR PHYSICS,2020,295(3):14. |
APA | Xu, Long,Liu, Sixuan,Yan, Yihua,&Zhang, Weiqiang.(2020).EUV Wave Detection and Characterization Using Deep Learning.SOLAR PHYSICS,295(3),14. |
MLA | Xu, Long,et al."EUV Wave Detection and Characterization Using Deep Learning".SOLAR PHYSICS 295.3(2020):14. |
入库方式: OAI收割
来源:国家天文台
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