Two-sided Loop Solar Jet Driven by the Eruption of a Small Filament in a Big Filament Channel

doi:10.3847/1538-4357/ad23e5

YNAO OpenIR > 太阳物理研究组

	Two-sided Loop Solar Jet Driven by the Eruption of a Small Filament in a Big Filament Channel
	Yang JY(杨家艳)1 ; Chen, Hechao 2; Hong JC(洪俊超)1 ; Yang B(杨波)1,3 ; Bi Y(毕以)1,3
发表期刊	ASTROPHYSICAL JOURNAL
	2024-03-01
卷号	964 期号:1
DOI	10.3847/1538-4357/ad23e5
产权排序	第1完成单位
收录类别	SCI
摘要	Similar to the cases of anemone jets, two-sided loop solar jets can also be produced by either flux emergence from the solar interior or small-scale filament eruptions. Using high-quality data from the Solar Dynamics Observatory, we have analyzed a two-sided loop solar jet triggered by the eruption of a small filament. The jet occurred in a pre-existing big filament channel. The detailed processes involved in the eruption of the small filament, the interaction between the erupted filament and the big filament channel, and the launch of the two-sided loop jet are presented. The observations further revealed notable asymmetry between the two branches of the jet spire: the northeastern branch is narrow and short, while the southern branch is wide and long and accompanied by discernible untwisting motions. We explored the unique appearance of the jet by employing the method of local potential field extrapolation to calculate the coronal magnetic field configuration around the jet. The photospheric magnetic flux below the small filament underwent cancellation for approximately 7 hr before the filament eruption, and the negative flux near the southern footpoint of the filament decreased by about 56% during this interval. Therefore, we propose that the primary photospheric driver of the filament eruption and the associated two-sided loop jet in this event is flux cancellation rather than flux emergence.
资助项目	B-type Strategic Priority Program - Chinese Academy of Sciences[XDB41000000]; B-type Strategic Priority Program - Chinese Academy of Sciences[XDB0560000]; National Key R&D Program of China[2019YFA0405000]; National Natural Science Foundation of China[12273108]; National Natural Science Foundation of China[11933009]; National Natural Science Foundation of China[12173084]; National Natural Science Foundation of China[12073072]; National Natural Science Foundation of China[12273106]; Yunnan Revitalization Talent Support Program Innovation Team Project[202405AS350012]
项目资助者	B-type Strategic Priority Program - Chinese Academy of Sciences[XDB41000000, XDB0560000] ; National Key R&D Program of China[2019YFA0405000] ; National Natural Science Foundation of China[12273108, 11933009, 12173084, 12073072, 12273106] ; Yunnan Revitalization Talent Support Program Innovation Team Project[202405AS350012]
语种	英语
学科领域	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
ISSN	0004-637X
URL	查看原文
WOS记录号	WOS:001184852200001
WOS研究方向	Astronomy & Astrophysics
WOS类目	Astronomy & Astrophysics
关键词[WOS]	X-RAY JETS ; CORONAL MASS EJECTION ; H-ALPHA SURGES ; MAGNETIC-FLUX CANCELLATION ; ACTIVE-REGION ; BLOWOUT SURGE ; RECONNECTION ; DYNAMICS ; EVOLUTION ; STANDARD
引用统计	被引频次：2[WOS] [WOS记录] [WOS相关记录]
文献类型	期刊论文
版本	出版稿
条目标识符	http://ir.ynao.ac.cn/handle/114a53/26473
专题	太阳物理研究组抚仙湖太阳观测和研究基地
作者单位	1.Yunnan Observatory, Chinese Academy of Sciences, P.O. Box 110, Kunming 650011, People's Republic of China; 2.School of Physics and Astronomy, Yunnan University, Kunming 650500, People's Republic of China; 3.Yunnan Key Laboratory of Solar Physics and Space Science, Kunming 650011, People's Republic of China
第一作者单位	中国科学院云南天文台
推荐引用方式 GB/T 7714	Yang JY,Chen, Hechao,Hong JC,et al. Two-sided Loop Solar Jet Driven by the Eruption of a Small Filament in a Big Filament Channel[J]. ASTROPHYSICAL JOURNAL,2024,964(1).
APA	杨家艳,Chen, Hechao,洪俊超,杨波,&毕以.(2024).Two-sided Loop Solar Jet Driven by the Eruption of a Small Filament in a Big Filament Channel.ASTROPHYSICAL JOURNAL,964(1).
MLA	杨家艳,et al."Two-sided Loop Solar Jet Driven by the Eruption of a Small Filament in a Big Filament Channel".ASTROPHYSICAL JOURNAL 964.1(2024).

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