A Compact Source for Quasi-periodic Pulsation in an M-class Solar Flare

doi:10.3847/2041-8213/ab5648

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	A Compact Source for Quasi-periodic Pulsation in an M-class Solar Flare
	Yuan, Ding 1,2; Feng, Song 3,4; Li, Dong 5; Ning, ZongJun 5; Tan, Baolin 2
刊名	ASTROPHYSICAL JOURNAL LETTERS
	2019-12-01
卷号	886 期号:2 页码:6
ISSN号	2041-8205
DOI	10.3847/2041-8213/ab5648
产权排序	第3完成单位
文献子类	Article
英文摘要	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
学科主题	天文学 ; 太阳与太阳系 ; 太阳物理学
URL标识	查看原文
出版地	TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
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]
WOS关键词	X-RAY PULSATIONS ; OSCILLATIONS ; RECONNECTION ; SUMER
WOS研究方向	Astronomy & Astrophysics
语种	英语
出版者	IOP PUBLISHING LTD
WOS记录号	WOS:000499342700001
资助机构	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]
内容类型	期刊论文
源URL	[http://ir.ynao.ac.cn/handle/114a53/21746]
专题	云南天文台_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.