YNAO OpenIR  > 抚仙湖太阳观测和研究基地
The Formation of a Multifilament System Driven by Photospheric Converging Motions in a Bipolar Sunspot
Li, Haitang1; Guo, Jinhan2,3; Cheng, Xin2,3; Zhou, Chang2,3; Yan XL(闫晓理)4; Chen, Jun5; Guo, Yang2,3; Oloketuyi, Jacob1; Ding, Mingde2,3; Liu, Yu1
发表期刊ASTROPHYSICAL JOURNAL LETTERS
2025-02-01
卷号979期号:2
DOI10.3847/2041-8213/ada893
产权排序第4完成单位
收录类别SCI
摘要Solar filaments are believed to be a clump of cold plasma accumulated in the magnetic dips. However, the magnetic configuration of filaments and the key factors for their formation remains elusive. In this Letter, we present a detailed study of the formation and eruption of a multifilament system with observations and simulations. Before the filament appeared visible, the chromospheric fibrils gradually gathered together, evolving from a diffuse distribution into threadlike structures that were nearly parallel to the polarity inversion lines. On 2022 March 20, an arch filament first appeared showing high dynamics, and subsequently two reserved S-shaped filaments were visibly observed. These two filament segments further reconnected, forming a long coherent filament and resulting in a double-decker configuration. In addition, continuous converging motion and magnetic flux cancellation were found in the photosphere during the evolution. Simultaneously, more bald patch structures appeared at the polarities' collision position. Through a data-driven numerical simulation, we further reconstructed the coronal magnetic field, which is composed of two twisted magnetic flux ropes (MFRs) with their bottom touching the photosphere, along with a group of sheared arcades forming an X-shaped configuration. These findings suggest that the magnetic configuration of the filament is in a highly dynamic state, evolving from a hybrid to a coherent MFR. Moreover, we propose that the formation and eruption of the multifilament system are closely related to magnetic reconnection taking place on the photosphere and in the lower corona, respectively, both mainly driven by the photospheric converging motion.
资助项目Sichuan Science and Technology Program[2025ZNSFSC0877]; National Natural Science Foundations of China (NSFC)[12373063]; China National Postdoctoral Program for Innovative Talents[BX20240159]
项目资助者Sichuan Science and Technology Program[2025ZNSFSC0877] ; National Natural Science Foundations of China (NSFC)[12373063] ; China National Postdoctoral Program for Innovative Talents[BX20240159]
语种英语
学科领域天文学 ; 太阳与太阳系
文章类型Article
出版者IOP Publishing Ltd
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN2041-8205
URL查看原文
WOS记录号WOS:001408853100001
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]MAGNETIC-FLUX ROPE ; FILAMENT CHANNELS ; SOLAR FILAMENT ; CANCELLATION ; FIELD ; EVOLUTION ; ORIGIN ; STABILITY ; ERUPTION ; FLOWS
引用统计
文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/28068
专题抚仙湖太阳观测和研究基地
作者单位1.School of Physical Science and Technology, Southwest Jiaotong University, Chengdu 611756, People's Republic of China; [email protected], [email protected];
2.School of Astronomy and Space Science, Nanjing University, Nanjing 210023, People's Republic of China;
3.Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing 210023, People's Republic of China;
4.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, People's Republic of China;
5.Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023, People's Republic of China
推荐引用方式
GB/T 7714
Li, Haitang,Guo, Jinhan,Cheng, Xin,et al. The Formation of a Multifilament System Driven by Photospheric Converging Motions in a Bipolar Sunspot[J]. ASTROPHYSICAL JOURNAL LETTERS,2025,979(2).
APA Li, Haitang.,Guo, Jinhan.,Cheng, Xin.,Zhou, Chang.,闫晓理.,...&Liu, Yu.(2025).The Formation of a Multifilament System Driven by Photospheric Converging Motions in a Bipolar Sunspot.ASTROPHYSICAL JOURNAL LETTERS,979(2).
MLA Li, Haitang,et al."The Formation of a Multifilament System Driven by Photospheric Converging Motions in a Bipolar Sunspot".ASTROPHYSICAL JOURNAL LETTERS 979.2(2025).
条目包含的文件
文件名称/大小 文献类型 版本类型 开放类型 使用许可
The Formation of a M(1925KB)期刊论文出版稿开放获取CC BY-NC-SA浏览 请求全文
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[Li, Haitang]的文章
[Guo, Jinhan]的文章
[Cheng, Xin]的文章
百度学术
百度学术中相似的文章
[Li, Haitang]的文章
[Guo, Jinhan]的文章
[Cheng, Xin]的文章
必应学术
必应学术中相似的文章
[Li, Haitang]的文章
[Guo, Jinhan]的文章
[Cheng, Xin]的文章
相关权益政策
暂无数据
收藏/分享
文件名: The Formation of a Multifilament System Driven by Photospheric Converging Motions in a Bipolar Sunspot.pdf
格式: Adobe PDF
所有评论 (0)
暂无评论
 

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。