中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Rapid Spatiotemporal Evolution of Vertical Electric Currents during an X-class Flare

文献类型:期刊论文

作者Shen, Jinhua1,2; Yang, Xu5; Li, Jianping4; Liu, Yangyu2,3; Su, Yingna4; Ji, Haisheng4
刊名ASTROPHYSICAL JOURNAL
出版日期2025-06-10
卷号986期号:1页码:102
ISSN号0004-637X
DOI10.3847/1538-4357/add92d
产权排序1
英文摘要In this paper, we present a detailed analysis of the spatiotemporal evolution of photospheric vertical electric currents (VECs) during an X1.1 flare (SOL2013-11-10T05:08). The VEC on the solar surface is calculated using the 135 s high-temporal-resolution vector magnetograms obtained from the Helioseismic and Magnetic Imager on board the Solar Dynamics Observatory. In the region, a highly sheared magnetic channel that is also a polarity inversion line (PIL) divides the region into two parts. The spatial configuration of VEC ribbons is always conjugate footprints, and it takes the form of a sigmoid along two sides of the PIL at the beginning of the flare. The temporal evolution of the VECs shows a rapid enhancement associated with the impulsive phase of the flare, and mean horizontal fields in this region show similar temporal behavior. The most prominent enhancement of VECs not only shows up along the two sides of the enhancement Bh but also spreads outward along the PILs. The VECs in positive and negative fields have an initial separation motion and are followed by an apparent approaching motion. In contrast, the flaring loops and white-light flare ribbons have an initial contraction and later expansion motion. Our results show that the rapid change of magnetic fields related to flares has a predominant role in affecting the spatiotemporal evolution of VECs.
WOS关键词HIGH-RESOLUTION OBSERVATIONS ; SHEARED MAGNETIC-FIELDS ; QUASI-SEPARATRIX LAYERS ; SOLAR ACTIVE REGIONS ; LORENTZ FORCE ; CURRENT NEUTRALIZATION ; STATISTICAL-ANALYSIS ; ERUPTIVE ACTIVITY ; FLUX EMERGENCE ; ENERGY-RELEASE
资助项目MOST divided by National Natural Science Foundation of China (NSFC)https://doi.org/10.13039/501100001809[XDB0560000] ; Strategic Priority Research Program of the Chinese Academy of Sciences[12273101] ; National Natural Science Foundation of China (NSFC)[2024D01E38] ; Natural Science Foundation of Xinjiang Uygur Autonomous Region[YNSPCC202219] ; Specialized Research Fund for State Key Laboratories of Solar Activity and Space Weather and Yunnan Key Laboratory of Solar Physics and Space Science
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001506909500001
出版者IOP Publishing Ltd
资助机构MOST divided by National Natural Science Foundation of China (NSFC)https://doi.org/10.13039/501100001809 ; Strategic Priority Research Program of the Chinese Academy of Sciences ; National Natural Science Foundation of China (NSFC) ; Natural Science Foundation of Xinjiang Uygur Autonomous Region ; Specialized Research Fund for State Key Laboratories of Solar Activity and Space Weather and Yunnan Key Laboratory of Solar Physics and Space Science
源URL[http://ir.xao.ac.cn/handle/45760611-7/7822]  
专题太阳物理研究室_太阳物理研究团组
通讯作者Shen, Jinhua
作者单位1.State Key Lab Solar Act & Space Weather, Beijing 100190, Peoples R China
2.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
3.UCAS, Sch Astron & Space Sci, Beijing 100049, Peoples R China
4.Chinese Acad Sci, Key Lab Dark Matter & Space Astron, Nanjing 210023, Peoples R China
5.Big Bear Solar Observ, 40386 N Shore Ln, Big Bear City, CA 92314 USA
推荐引用方式
GB/T 7714
Shen, Jinhua,Yang, Xu,Li, Jianping,et al. Rapid Spatiotemporal Evolution of Vertical Electric Currents during an X-class Flare[J]. ASTROPHYSICAL JOURNAL,2025,986(1):102.
APA Shen, Jinhua,Yang, Xu,Li, Jianping,Liu, Yangyu,Su, Yingna,&Ji, Haisheng.(2025).Rapid Spatiotemporal Evolution of Vertical Electric Currents during an X-class Flare.ASTROPHYSICAL JOURNAL,986(1),102.
MLA Shen, Jinhua,et al."Rapid Spatiotemporal Evolution of Vertical Electric Currents during an X-class Flare".ASTROPHYSICAL JOURNAL 986.1(2025):102.

入库方式: OAI收割

来源:新疆天文台

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。