中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
A Compact Source for Quasi-periodic Pulsation in an M-class Solar Flare

文献类型:期刊论文

作者Yuan, Ding1,2; Feng, Song3,4; Li, Dong5; Ning, ZongJun5; Tan, Baolin2
刊名ASTROPHYSICAL JOURNAL LETTERS
出版日期2019-12-01
卷号886期号:2页码:6
ISSN号2041-8205
DOI10.3847/2041-8213/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
WOS关键词X-RAY PULSATIONS ; OSCILLATIONS ; RECONNECTION ; SUMER
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]
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.

入库方式: OAI收割

来源:云南天文台

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