中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Observational Study of Chromospheric Jets In and Around a Sunspot Observed by NVST and SDO

文献类型:期刊论文

作者Wu GT(吴国堂)1,2; Yan XL(闫晓理)2,3; Xue ZK(薛志科)2,3; Wang JC(王金成)2,3; Xu Z(徐喆)2,3; Yang LH(杨丽恒)2,3; Zhou YA(周羿安)2; Yang, Liping4; Zhang XS(张鑫生)1,2; Dong QF(董起帆)1,2
刊名ASTROPHYSICAL JOURNAL
出版日期2025-11-10
卷号993期号:2
ISSN号0004-637X
DOI10.3847/1538-4357/ae1198
产权排序第1完成单位
文献子类Article
英文摘要To better understand the characteristics, driving mechanisms, and potential heating contributions of chromospheric jets, we analyze two contrasting types: one originating from within the sunspot penumbra (inside jets) and the other originating from outside the penumbra (outside jets). Statistical analysis of 100 jets (50 inside jets and 50 outside jets) reveals that inside jets have a projected velocity range of 4-14 km s-1, a length range of 1-4 Mm, a width range of 0.2-0.6 Mm, and a lifetime range of 135-450 s, with mean values of 7.90 km s-1, 2.61 Mm, 0.41 Mm, and 260 s, respectively. About 52% of inside jets are associated with brightenings in H alpha blue wing images, and some show high-temperature signatures, suggesting a connection with localized energy release. In contrast, outside jets have higher velocities (8-50 km s-1, average 19.04 km s-1), greater lengths (average 6.26 Mm, up to 27.27 Mm), slightly larger widths (average 0.46 Mm), and longer lifetimes (135-630 s, average 327 s). They typically originate from regions of opposite magnetic polarities and are associated with magnetic flux emergence and extreme-ultraviolet brightenings. Some outside jets correspond to coronal jets with inverted Y-shaped structures and temperatures exceeding one million Kelvin. Our results suggest that both jet types are driven by magnetic reconnection occurring in distinct magnetic field configurations and contribute to chromospheric and coronal heating.
学科主题天文学 ; 太阳与太阳系
URL标识查看原文
出版地No.2 The Distillery, Glassfields, Avon Street, Bristol, ENGLAND
WOS关键词H-ALPHA SURGES ; X-RAY JETS ; PENUMBRAL MICROJETS ; ANEMONE JETS ; SOLAR ; DYNAMICS ; HINODE ; REGION ; TOPOLOGY
资助项目Strategic Priority Research Program of the Chinese Academy of Sciences[XDB0560000]; Yunnan Fundamental Research Projects[202301AT070347]; National Science Foundation of China (NSFC)[12325303]; Yunnan Provincial Department of Education Science Research Fund Project[2025J0945]; Chuxiong Normal University Doctoral Research Initiation Fund Project[BSQD2420]; Yunnan Key Laboratory of Solar Physics and Space Science[202205AG070009]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001605284900001
出版者IOP Publishing Ltd
资助机构Strategic Priority Research Program of the Chinese Academy of Sciences[XDB0560000] ; Yunnan Fundamental Research Projects[202301AT070347] ; National Science Foundation of China (NSFC)[12325303] ; Yunnan Provincial Department of Education Science Research Fund Project[2025J0945] ; Chuxiong Normal University Doctoral Research Initiation Fund Project[BSQD2420] ; Yunnan Key Laboratory of Solar Physics and Space Science[202205AG070009]
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/28699]  
专题云南天文台_抚仙湖太阳观测站
通讯作者Yan XL(闫晓理)
作者单位1.University of Chinese Academy of Sciences, Beijing 100049, People’s Republic of China;
2.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, People’s Republic of China; yanxl@ynao.ac.cn;
3.Yunnan Key Laboratory of Solar Physics and Space Science, Kunming 650216, People’s Republic of China;
4.School of Physics, Electrical and Energy Engineering, Chuxiong Normal University, Chuxiong 675000, People’s Republic of China
推荐引用方式
GB/T 7714
Wu GT,Yan XL,Xue ZK,et al. Observational Study of Chromospheric Jets In and Around a Sunspot Observed by NVST and SDO[J]. ASTROPHYSICAL JOURNAL,2025,993(2).
APA 吴国堂.,闫晓理.,薛志科.,王金成.,徐喆.,...&吴宗银.(2025).Observational Study of Chromospheric Jets In and Around a Sunspot Observed by NVST and SDO.ASTROPHYSICAL JOURNAL,993(2).
MLA 吴国堂,et al."Observational Study of Chromospheric Jets In and Around a Sunspot Observed by NVST and SDO".ASTROPHYSICAL JOURNAL 993.2(2025).

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来源:云南天文台

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