Association Between a Failed Prominence Eruption and the Drainage of Mass from Another Prominence

IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
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
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Abstract

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.

Abstract Image

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
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。
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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.
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