Simultaneous observations of a breakout current sheet and a flare current sheet in a coronal jet event

doi:10.1093/mnras/stad3876

	Simultaneous observations of a breakout current sheet and a flare current sheet in a coronal jet event
	Yang LH(杨丽恒)1,5; Yan XL(闫晓理)1,5; Xue ZK(薛志科)1,5; Xu Z(徐喆)1,5; Zhang, Qingmin 4; Hou, Yijun 3; Wang JC(王金成)1,5; Chen, Huadong 3; Li, Qiaoling 2
刊名	Monthly Notices of the Royal Astronomical Society
	2024-02-01
卷号	528 期号:1 页码:1094-1107
关键词	Sun: activity Sun: corona Sun: filaments prominences
ISSN号	0035-8711
DOI	10.1093/mnras/stad3876
产权排序	第1完成单位
文献子类	Journal article (JA)
英文摘要	Previous studies have revealed that solar coronal jets triggered by the eruption of minifilaments (MFs) conform to the famous magnetic-breakout mechanism. In such a scenario, a breakout current sheet (BCS) and a flare current sheet (FCS) should be observed during the jets. With high spatial and temporal resolution data from the SDO, the NVST, the RHESSI, the Wind, and the GOES, we present observational evidence of a BCS and a FCS formation during coronal jets driven by a MF eruption occurring in the active region NOAA 11726 on 2013 April 21. Magnetic field extrapolation shows that the MF was enclosed by a fan-spine magnetic structure. The MF was activated by flux cancellation under it, and then slowly rose. A BCS formed when the magnetic fields wrapping the MF squeezed to antidirectional external open fields. Simultaneously, one thin bright jet and two bidirectional jet-like structures were observed. As the MF erupted as a blowout jet, a FCS was formed when the two distended legs inside the MF field came together. One end of the FCS connected the post-flare loops. The BCS’s peak temperature was calculated to be 2.5 MK. The FCS’s length, width, and peak temperature were calculated to be 4.35–4.93, 1.31–1.45, and 2.5 MK, respectively. The magnetic reconnection rate associated with the FCS was estimated to be from 0.266 to 0.333. This event is also related to a type III radio burst, indicating its influence on interplanetary space. These observations support the scenario of the breakout model as the trigger mechanism of coronal jets, and flux cancellation was the driver of this event. © The Author(s) 2024.
学科主题	天文学
URL标识	查看原文
资助项目	National Natural Science Foundation of China[11973084];National Natural Science Foundation of China[12003064];National Natural Science Foundation of China[12173084];National Natural Science Foundation of China[12203097];National Natural Science Foundation of China[12273060];National Natural Science Foundation of China[12325303];National Natural Science Foundation of China[12373065];Chinese Academy of Sciences[KLSA202101];Chinese Academy of Sciences[XDB0560000];Youth Innovation Promotion Association of the Chinese Academy of Sciences[2019061];Youth Innovation Promotion Association of the Chinese Academy of Sciences[2023063];National Key Research and Development Program of China[2019YFA0405000];National Key Research and Development Program of China[2021YFA1600502];National Key Research and Development Program of China[2022YFF0503800]
语种	英语
资助机构	National Natural Science Foundation of China[11973084, 12003064, 12173084, 12203097, 12273060, 12325303, 12373065] ; Chinese Academy of Sciences[KLSA202101, XDB0560000] ; Youth Innovation Promotion Association of the Chinese Academy of Sciences[2019061, 2023063] ; National Key Research and Development Program of China[2019YFA0405000, 2021YFA1600502, 2022YFF0503800]
内容类型	期刊论文
源URL	[http://ir.ynao.ac.cn/handle/114a53/26492]
专题	云南天文台_抚仙湖太阳观测站
作者单位	1.Yunnan Key Laboratory of the Solar Physics and Space Science, Kunming, 650216, China; 2.Department of Physics, Yunnan University, Yunnan, Kunming, 650091, China 3.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012, China; 4.Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, 210023, China; 5.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, China;
推荐引用方式 GB/T 7714	Yang LH,Yan XL,Xue ZK,et al. Simultaneous observations of a breakout current sheet and a flare current sheet in a coronal jet event[J]. Monthly Notices of the Royal Astronomical Society,2024,528(1):1094-1107.
APA	杨丽恒.,闫晓理.,薛志科.,徐喆.,Zhang, Qingmin.,...&Li, Qiaoling.(2024).Simultaneous observations of a breakout current sheet and a flare current sheet in a coronal jet event.Monthly Notices of the Royal Astronomical Society,528(1),1094-1107.
MLA	杨丽恒,et al."Simultaneous observations of a breakout current sheet and a flare current sheet in a coronal jet event".Monthly Notices of the Royal Astronomical Society 528.1(2024):1094-1107.