Transition-region explosive events produced by plasmoid instability | |
Li, Dong1,2 | |
刊名 | RESEARCH IN ASTRONOMY AND ASTROPHYSICS |
2019-05-01 | |
卷号 | 19期号:5页码:10 |
关键词 | Sun: transition region line: profiles methods: numerical magnetohydrodynamics (MHD) |
ISSN号 | 1674-4527 |
DOI | 10.1088/1674-4527/19/5/67 |
英文摘要 | Magnetic reconnection is thought to be a key process in most solar eruptions. Thanks to high-resolution observations and simulations, the studied scale of the reconnection process has become smaller and smaller. Spectroscopic observations show that the reconnection site can be very small, which always exhibits a bright core and two extended wings with fast speeds, i.e., transition-region explosive events. In this paper, using the PLUTO code, we perform a 2-D magnetohydrodynamic simulation to investigate small-scale reconnection in double current sheets. Based on our simulation results, such as the line-of-sight velocity, number density and plasma temperature, we can synthesize the line profile of Si IV 1402.77 angstrom which is a well known emission line used to study transition-region explosive events on the Sun. The synthetic line profile of Si IV 1402.77 angstrom is complex with a bright core and two broad wings which can extend to nearly 200 kms(-1). Our simulation results suggest that the transition-region explosive events on the Sun are produced by plasmoid instability during small-scale magnetic reconnection. |
资助项目 | National Natural Science Foundation of China[11603077] ; National Natural Science Foundation of China[11573072] ; National Natural Science Foundation of China[11790302] ; National Natural Science Foundation of China[11333009] ; National Natural Science Foundation of China[U1731241] ; National Natural Science Foundation of China[KLSA201708] ; Youth Fund of Jiangsu[BK20161095] ; Youth Fund of Jiangsu[BK20171108] ; Strategic Priority Research Program on Space Science, CAS[XDA15052200] ; Strategic Priority Research Program on Space Science, CAS[XDA15320301] ; Strategic Priority Research Program on Space Science, CAS[2010DP173032] |
WOS关键词 | MAGNETIC RECONNECTION ; SOLAR CHROMOSPHERE ; QUIET SUN ; PARTICLE-ACCELERATION ; BRIGHT POINTS ; PLUTO CODE ; ERUPTION ; FLARE ; JETS ; ENERGETICS |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES |
WOS记录号 | WOS:000467595300005 |
资助机构 | National Natural Science Foundation of China ; National Natural Science Foundation of China ; Youth Fund of Jiangsu ; Youth Fund of Jiangsu ; Strategic Priority Research Program on Space Science, CAS ; Strategic Priority Research Program on Space Science, CAS ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Youth Fund of Jiangsu ; Youth Fund of Jiangsu ; Strategic Priority Research Program on Space Science, CAS ; Strategic Priority Research Program on Space Science, CAS ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Youth Fund of Jiangsu ; Youth Fund of Jiangsu ; Strategic Priority Research Program on Space Science, CAS ; Strategic Priority Research Program on Space Science, CAS ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Youth Fund of Jiangsu ; Youth Fund of Jiangsu ; Strategic Priority Research Program on Space Science, CAS ; Strategic Priority Research Program on Space Science, CAS |
内容类型 | 期刊论文 |
源URL | [http://ir.bao.ac.cn/handle/114a11/26183] |
专题 | 中国科学院国家天文台 |
通讯作者 | Li, Dong |
作者单位 | 1.Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210034, Jiangsu, Peoples R China 2.Chinese Acad Sci, Natl Astron Observ, Key Lab Solar Act, Beijing 100101, Peoples R China |
推荐引用方式 GB/T 7714 | Li, Dong. Transition-region explosive events produced by plasmoid instability[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2019,19(5):10. |
APA | Li, Dong.(2019).Transition-region explosive events produced by plasmoid instability.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,19(5),10. |
MLA | Li, Dong."Transition-region explosive events produced by plasmoid instability".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 19.5(2019):10. |
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