Observation of Two Splitting Processes in a Partial Filament Eruption on the Sun: The Role of Breakout Reconnection

Partial filament eruptions have often been observed; however, the physical mechanisms that lead to filament splitting are not yet fully understood. In this study, we present a unique event of a partial filament eruption that undergoes two distinct splitting processes. The first process involves vert...

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Main Authors: Zheng Sun, Ting Li, Hui Tian, Yijun Hou, Zhenyong Hou, Hechao Chen, Xianyong Bai, Yuanyong Deng
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ace5b1
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author Zheng Sun
Ting Li
Hui Tian
Yijun Hou
Zhenyong Hou
Hechao Chen
Xianyong Bai
Yuanyong Deng
author_facet Zheng Sun
Ting Li
Hui Tian
Yijun Hou
Zhenyong Hou
Hechao Chen
Xianyong Bai
Yuanyong Deng
author_sort Zheng Sun
collection DOAJ
description Partial filament eruptions have often been observed; however, the physical mechanisms that lead to filament splitting are not yet fully understood. In this study, we present a unique event of a partial filament eruption that undergoes two distinct splitting processes. The first process involves vertical splitting and is accompanied by brightenings inside the filament, which may result from internal magnetic reconnection within the filament. Following the first splitting process, the filament is separated into an upper part and a lower part. Subsequently, the upper part undergoes a second splitting, which is accompanied by a coronal blowout jet. An extrapolation of the coronal magnetic field reveals a hyperbolic flux tube structure above the filament, indicating the occurrence of breakout reconnection that reduces the constraining field above. Consequently, the filament is lifted up, but at a nonuniform speed. The high-speed part reaches the breakout current sheet to generate the blowout jet, while the low-speed part falls back to the solar surface, resulting in the second splitting. In addition, continuous brightenings are observed along the flare ribbons, suggesting the occurrence of a slipping reconnection process. This study presents, for the first time, the unambiguous observation of a two-stage filament-splitting process, advancing our understanding of the complex dynamics of solar eruptions.
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spelling doaj.art-03123ad52f214b6c850269d9fe4966f62023-09-03T15:11:49ZengIOP PublishingThe Astrophysical Journal1538-43572023-01-01953214810.3847/1538-4357/ace5b1Observation of Two Splitting Processes in a Partial Filament Eruption on the Sun: The Role of Breakout ReconnectionZheng Sun0https://orcid.org/0000-0001-5657-7587Ting Li1https://orcid.org/0000-0001-6655-1743Hui Tian2https://orcid.org/0000-0002-1369-1758Yijun Hou3https://orcid.org/0000-0002-9534-1638Zhenyong Hou4https://orcid.org/0000-0003-4804-5673Hechao Chen5https://orcid.org/0000-0001-7866-4358Xianyong Bai6https://orcid.org/0000-0003-2686-9153Yuanyong Deng7School of Earth and Space Sciences, Peking University , Beijing 100871, People's Republic of China ; huitian@pku.edu.cnNational Astronomical Observatories, Chinese Academy of Sciences , Beijing 100101, People's Republic of China ; liting@nao.cas.cn; School of Astronomy and Space Science, University of Chinese Academy of Sciences , Beijing 100049, People's Republic of ChinaSchool of Earth and Space Sciences, Peking University , Beijing 100871, People's Republic of China ; huitian@pku.edu.cn; National Astronomical Observatories, Chinese Academy of Sciences , Beijing 100101, People's Republic of China ; liting@nao.cas.cn; National Space Science Center, Chinese Academy of Sciences , Beijing 100190, People's Republic of ChinaNational Astronomical Observatories, Chinese Academy of Sciences , Beijing 100101, People's Republic of China ; liting@nao.cas.cn; School of Astronomy and Space Science, University of Chinese Academy of Sciences , Beijing 100049, People's Republic of ChinaSchool of Earth and Space Sciences, Peking University , Beijing 100871, People's Republic of China ; huitian@pku.edu.cn; Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University) , Ministry of Education, Nanjing 210093, People's Republic of ChinaSchool of Physics and Astronomy, Yunnan University , Kunming 650500, People's Republic of ChinaNational Astronomical Observatories, Chinese Academy of Sciences , Beijing 100101, People's Republic of China ; liting@nao.cas.cnNational Astronomical Observatories, Chinese Academy of Sciences , Beijing 100101, People's Republic of China ; liting@nao.cas.cnPartial filament eruptions have often been observed; however, the physical mechanisms that lead to filament splitting are not yet fully understood. In this study, we present a unique event of a partial filament eruption that undergoes two distinct splitting processes. The first process involves vertical splitting and is accompanied by brightenings inside the filament, which may result from internal magnetic reconnection within the filament. Following the first splitting process, the filament is separated into an upper part and a lower part. Subsequently, the upper part undergoes a second splitting, which is accompanied by a coronal blowout jet. An extrapolation of the coronal magnetic field reveals a hyperbolic flux tube structure above the filament, indicating the occurrence of breakout reconnection that reduces the constraining field above. Consequently, the filament is lifted up, but at a nonuniform speed. The high-speed part reaches the breakout current sheet to generate the blowout jet, while the low-speed part falls back to the solar surface, resulting in the second splitting. In addition, continuous brightenings are observed along the flare ribbons, suggesting the occurrence of a slipping reconnection process. This study presents, for the first time, the unambiguous observation of a two-stage filament-splitting process, advancing our understanding of the complex dynamics of solar eruptions.https://doi.org/10.3847/1538-4357/ace5b1Solar magnetic reconnectionSolar flaresJets
spellingShingle Zheng Sun
Ting Li
Hui Tian
Yijun Hou
Zhenyong Hou
Hechao Chen
Xianyong Bai
Yuanyong Deng
Observation of Two Splitting Processes in a Partial Filament Eruption on the Sun: The Role of Breakout Reconnection
The Astrophysical Journal
Solar magnetic reconnection
Solar flares
Jets
title Observation of Two Splitting Processes in a Partial Filament Eruption on the Sun: The Role of Breakout Reconnection
title_full Observation of Two Splitting Processes in a Partial Filament Eruption on the Sun: The Role of Breakout Reconnection
title_fullStr Observation of Two Splitting Processes in a Partial Filament Eruption on the Sun: The Role of Breakout Reconnection
title_full_unstemmed Observation of Two Splitting Processes in a Partial Filament Eruption on the Sun: The Role of Breakout Reconnection
title_short Observation of Two Splitting Processes in a Partial Filament Eruption on the Sun: The Role of Breakout Reconnection
title_sort observation of two splitting processes in a partial filament eruption on the sun the role of breakout reconnection
topic Solar magnetic reconnection
Solar flares
Jets
url https://doi.org/10.3847/1538-4357/ace5b1
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