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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
2019-12-01
卷号886期号:2页码:6
DOI10.3847/2041-8213/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
学科门类理学 ; 理学::天文学
文章类型Article
出版者IOP PUBLISHING LTD
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN2041-8205
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
被引频次:26[WOS]   [WOS记录]     [WOS相关记录]
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
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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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