一个失败的突起喷发与另一个突起的质量流失之间的联系

IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Solar Physics Pub Date : 2024-06-20 DOI:10.1007/s11207-024-02336-5
Jian-chao Xue, Li Feng, Hui Li, Ping Zhang, Jun Chen, Guang-lu Shi, Kai-fan Ji, Ye Qiu, Chuan Li, Lei Lu, Bei-li Ying, Ying Li, Yu Huang, You-ping Li, Jing-wei Li, Jie Zhao, De-chao Song, Shu-ting Li, Zheng-yuan Tian, Ying-na Su, Qing-min Zhang, Yun-yi Ge, Jia-hui Shan, Qiao Li, Gen Li, Yue Zhou, Jun Tian, Xiao-feng Liu, Zhi-chen Jing, Bo Chen, Ke-fei Song, Ling-ping He, Shi-jun Lei, Wei-qun Gan
{"title":"一个失败的突起喷发与另一个突起的质量流失之间的联系","authors":"Jian-chao Xue,&nbsp;Li Feng,&nbsp;Hui Li,&nbsp;Ping Zhang,&nbsp;Jun Chen,&nbsp;Guang-lu Shi,&nbsp;Kai-fan Ji,&nbsp;Ye Qiu,&nbsp;Chuan Li,&nbsp;Lei Lu,&nbsp;Bei-li Ying,&nbsp;Ying Li,&nbsp;Yu Huang,&nbsp;You-ping Li,&nbsp;Jing-wei Li,&nbsp;Jie Zhao,&nbsp;De-chao Song,&nbsp;Shu-ting Li,&nbsp;Zheng-yuan Tian,&nbsp;Ying-na Su,&nbsp;Qing-min Zhang,&nbsp;Yun-yi Ge,&nbsp;Jia-hui Shan,&nbsp;Qiao Li,&nbsp;Gen Li,&nbsp;Yue Zhou,&nbsp;Jun Tian,&nbsp;Xiao-feng Liu,&nbsp;Zhi-chen Jing,&nbsp;Bo Chen,&nbsp;Ke-fei Song,&nbsp;Ling-ping He,&nbsp;Shi-jun Lei,&nbsp;Wei-qun Gan","doi":"10.1007/s11207-024-02336-5","DOIUrl":null,"url":null,"abstract":"<div><p>Sympathetic eruptions of solar prominences have been studied for decades, however, it is usually difficult to identify their causal links. Here, we present two failed prominence eruptions on 26 October 2022 and explore their connections. Using stereoscopic observations, the South prominence (PRO-S) erupts with untwisting motions, flare ribbons occur underneath, and new connections are formed during the eruption. The North prominence (PRO-N) rises up along with PRO-S, and its upper part disappears due to catastrophic mass draining along an elongated structure after PRO-S failed eruption. We suggest that the eruption of PRO-S initiates due to a kink instability, and fails to erupt due to reconnection with surrounding fields. The elongated structure connecting PRO-N overlies PRO-S, which causes the rising up of PRO-N along with PRO-S and mass drainage after PRO-S eruption. This study suggests that a prominence may end its life through mass drainage forced by an eruption underneath.</p></div>","PeriodicalId":777,"journal":{"name":"Solar Physics","volume":"299 6","pages":""},"PeriodicalIF":2.7000,"publicationDate":"2024-06-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s11207-024-02336-5.pdf","citationCount":"0","resultStr":"{\"title\":\"Association Between a Failed Prominence Eruption and the Drainage of Mass from Another Prominence\",\"authors\":\"Jian-chao Xue,&nbsp;Li Feng,&nbsp;Hui Li,&nbsp;Ping Zhang,&nbsp;Jun Chen,&nbsp;Guang-lu Shi,&nbsp;Kai-fan Ji,&nbsp;Ye Qiu,&nbsp;Chuan Li,&nbsp;Lei Lu,&nbsp;Bei-li Ying,&nbsp;Ying Li,&nbsp;Yu Huang,&nbsp;You-ping Li,&nbsp;Jing-wei Li,&nbsp;Jie Zhao,&nbsp;De-chao Song,&nbsp;Shu-ting Li,&nbsp;Zheng-yuan Tian,&nbsp;Ying-na Su,&nbsp;Qing-min Zhang,&nbsp;Yun-yi Ge,&nbsp;Jia-hui Shan,&nbsp;Qiao Li,&nbsp;Gen Li,&nbsp;Yue Zhou,&nbsp;Jun Tian,&nbsp;Xiao-feng Liu,&nbsp;Zhi-chen Jing,&nbsp;Bo Chen,&nbsp;Ke-fei Song,&nbsp;Ling-ping He,&nbsp;Shi-jun Lei,&nbsp;Wei-qun Gan\",\"doi\":\"10.1007/s11207-024-02336-5\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>Sympathetic eruptions of solar prominences have been studied for decades, however, it is usually difficult to identify their causal links. Here, we present two failed prominence eruptions on 26 October 2022 and explore their connections. Using stereoscopic observations, the South prominence (PRO-S) erupts with untwisting motions, flare ribbons occur underneath, and new connections are formed during the eruption. The North prominence (PRO-N) rises up along with PRO-S, and its upper part disappears due to catastrophic mass draining along an elongated structure after PRO-S failed eruption. We suggest that the eruption of PRO-S initiates due to a kink instability, and fails to erupt due to reconnection with surrounding fields. The elongated structure connecting PRO-N overlies PRO-S, which causes the rising up of PRO-N along with PRO-S and mass drainage after PRO-S eruption. This study suggests that a prominence may end its life through mass drainage forced by an eruption underneath.</p></div>\",\"PeriodicalId\":777,\"journal\":{\"name\":\"Solar Physics\",\"volume\":\"299 6\",\"pages\":\"\"},\"PeriodicalIF\":2.7000,\"publicationDate\":\"2024-06-20\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://link.springer.com/content/pdf/10.1007/s11207-024-02336-5.pdf\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Solar Physics\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://link.springer.com/article/10.1007/s11207-024-02336-5\",\"RegionNum\":3,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Solar Physics","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1007/s11207-024-02336-5","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

摘要

几十年来,人们一直在研究太阳突出部的共振爆发,但通常很难确定它们之间的因果联系。在这里,我们介绍了2022年10月26日两次失败的日珥爆发,并探讨了它们之间的联系。通过立体观测,南突出(PRO-S)在爆发时出现了解旋运动,其下方出现了耀斑带,并在爆发过程中形成了新的连接。北突出部(PRO-N)与南突出部一起升起,在南突出部喷发失败后,其上部由于灾难性质量沿拉长结构排出而消失。我们认为,PRO-S 的喷发是由扭结不稳定性引起的,由于与周围场的重新连接而导致喷发失败。连接 PRO-N 的拉长结构覆盖在 PRO-S 上,导致 PRO-N 与 PRO-S 一起上升,PRO-S 喷发后出现大量排水。这项研究表明,一个突出部可能会因下面的喷发迫使大量排水而结束其生命。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

摘要图片

查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
Association Between a Failed Prominence Eruption and the Drainage of Mass from Another Prominence

Sympathetic eruptions of solar prominences have been studied for decades, however, it is usually difficult to identify their causal links. Here, we present two failed prominence eruptions on 26 October 2022 and explore their connections. Using stereoscopic observations, the South prominence (PRO-S) erupts with untwisting motions, flare ribbons occur underneath, and new connections are formed during the eruption. The North prominence (PRO-N) rises up along with PRO-S, and its upper part disappears due to catastrophic mass draining along an elongated structure after PRO-S failed eruption. We suggest that the eruption of PRO-S initiates due to a kink instability, and fails to erupt due to reconnection with surrounding fields. The elongated structure connecting PRO-N overlies PRO-S, which causes the rising up of PRO-N along with PRO-S and mass drainage after PRO-S eruption. This study suggests that a prominence may end its life through mass drainage forced by an eruption underneath.

求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
Solar Physics
Solar Physics 地学天文-天文与天体物理
CiteScore
5.10
自引率
17.90%
发文量
146
审稿时长
1 months
期刊介绍: Solar Physics was founded in 1967 and is the principal journal for the publication of the results of fundamental research on the Sun. The journal treats all aspects of solar physics, ranging from the internal structure of the Sun and its evolution to the outer corona and solar wind in interplanetary space. Papers on solar-terrestrial physics and on stellar research are also published when their results have a direct bearing on our understanding of the Sun.
期刊最新文献
Prediction of Geoeffective CMEs Using SOHO Images and Deep Learning A New Solar Hard X-ray Image Reconstruction Algorithm for ASO-S/HXI Based on Deep Learning Calibration and Performance of the Full-Disk Vector MagnetoGraph (FMG) on Board the Advanced Space-Based Solar Observatory (ASO-S) Evaluation of Sunspot Areas Derived by Automated Sunspot-Detection Methods Helioseismic Constraints: Past, Current, and Future Observations
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术
文献互助 智能选刊 最新文献 互助须知 联系我们:info@booksci.cn
Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。
Copyright © 2023 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1