| A Compact Source for Quasi-periodic Pulsation in an M-class Solar Flare | |
| Yuan, Ding1,2; Feng, Song3,4; Li, Dong5; Ning, ZongJun5; Tan, Baolin2 | |
| 发表期刊 | ASTROPHYSICAL JOURNAL LETTERS
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| 2019-12-01 | |
| 卷号 | 886期号:2页码:6 |
| DOI | 10.3847/2041-8213/ab5648 |
| 产权排序 | 第3完成单位 |
| 收录类别 | SCI |
| 摘要 | Quasi-periodic pulsations (QPPs) are usually found in the light curves of solar and stellar flares; they carry the features of time characteristics and plasma emission of the flaring core, and could be used to diagnose the coronas of the Sun and remote stars. In this study, we combined the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory and the Nobeyama Radioheliograph (NoRH) to observe an M7.7 class flare that occurred at active region 11520 on 2012 July 19. A QPP was detected both in the AIA 131 |
| 资助项目 | National Natural Science Foundation of China (NSFC)[11803005] ; National Natural Science Foundation of China (NSFC)[11911530690] ; Shenzhen Technology Project[JCYJ20180306172239618] ; Open Research Program of Key Laboratory of Solar Activity of National Astronomical Observatory of China[KLSA201814] ; NSFC[U1931107] ; NSFC[1197309211603077] ; NSFC[11573072] ; Key Applied Basic Research program of Yunnan Province[2018FA035] ; Youth Fund of Jiangsu[BK20171108] |
| 项目资助者 | National Natural Science Foundation of China (NSFC)[11803005, 11911530690] ; Shenzhen Technology Project[JCYJ20180306172239618] ; Open Research Program of Key Laboratory of Solar Activity of National Astronomical Observatory of China[KLSA201814] ; NSFC[U1931107, 1197309211603077, 11573072] ; Key Applied Basic Research program of Yunnan Province[2018FA035] ; Youth Fund of Jiangsu[BK20171108] |
| 语种 | 英语 |
| 学科领域 | 天文学 ; 太阳与太阳系 ; 太阳物理学 |
| 文章类型 | Article |
| 出版者 | IOP PUBLISHING LTD |
| 出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
| ISSN | 2041-8205 |
| URL | 查看原文 |
| WOS记录号 | WOS:000499342700001 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | X-RAY PULSATIONS ; OSCILLATIONS ; RECONNECTION ; SUMER |
| 引用统计 | |
| 文献类型 | 期刊论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/21747 |
| 专题 | 其他 |
| 通讯作者 | Yuan, Ding |
| 作者单位 | 1.Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen, Guangdong 518055, People's Republic of China 2.Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, People's Republic of China 3.Yunnan Astronomical Observatory, Chinese Academy of Sciences, P.O. Box 110, Kunming 650011, People's Republic of China 4.Yunnan Astronomical Observatory, Chinese Academy of Sciences, P.O. Box 110, Kunming 650011, People's Republic of China 5.Key Laboratory for Dark Matter and Space Science, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210034, People's Republic of China |
| 推荐引用方式 GB/T 7714 | Yuan, Ding,Feng, Song,Li, Dong,et al. A Compact Source for Quasi-periodic Pulsation in an M-class Solar Flare[J]. ASTROPHYSICAL JOURNAL LETTERS,2019,886(2):6. |
| APA | Yuan, Ding,Feng, Song,Li, Dong,Ning, ZongJun,&Tan, Baolin.(2019).A Compact Source for Quasi-periodic Pulsation in an M-class Solar Flare.ASTROPHYSICAL JOURNAL LETTERS,886(2),6. |
| MLA | Yuan, Ding,et al."A Compact Source for Quasi-periodic Pulsation in an M-class Solar Flare".ASTROPHYSICAL JOURNAL LETTERS 886.2(2019):6. |
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