Numerical Simulation of Oscillatory Magnetic Reconnection Modulated by Solar Convective Motions
文献类型：期刊论文
| 作者 | Wang YF(王逸夫)3,4 ; Ni L(倪蕾)2,3,4; Cheng GC(程冠冲)3,4; Hu JL(胡佳亮)3,4; Chen YH(陈雨豪)1,3,4; Zafar, Abdullah4
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| 刊名 | ASTROPHYSICAL JOURNAL
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| 出版日期 | 2025-07-10 |
| 卷号 | 987期号:2 |
| ISSN号 | 0004-637X |
| DOI | 10.3847/1538-4357/addd15 |
| 产权排序 | 第1完成单位 |
| 文献子类 | Article |
| 英文摘要 | Oscillatory magnetic reconnection is a periodic magnetic reconnection process, during which the current sheet's orientation and the magnetic connections change periodically. This periodic variation is generally considered to originate from the magnetic reconnection itself rather than from external driving processes. We conduct 2.5D radiative magnetohydrodynamic simulations to investigate the emergence of a magnetic flux tube from the convection zone into the lower corona, where the emerging magnetic fields reconnect with background ones. During the reconnection process, within 5771 s the current sheet's orientation has been reversed 41 times, corresponding to 40 oscillation periods. Notably, the longest period is 30 minutes, which is consistent with the previous observational results. We find that the main factor leading to the reversal of the current sheet's orientation is the quasi-periodic external force provided by the emergence of plasma and magnetic fields from the convection zone. We also find the shifting of the upward outflows from the reconnection region along the horizontal direction due to the alternating changes of the reconnection inflow and outflow regions. In addition to the quasi-periodic change of the current sheet orientation, the reconnection rate at the main X-point also oscillates with a period between 100 and 400 s, which corresponds to the period of p-mode oscillations. |
| 学科主题 | 天文学 ; 太阳与太阳系 |
| URL标识 | 查看原文 |
| 出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
| WOS关键词 | QUASI-PERIODIC PULSATIONS ; EMERGING FLUX ; TRANSITION-REGION ; X-POINT ; DRIVEN ; EMISSION ; DYNAMICS ; SCALE ; JETS ; ERUPTIONS |
| 资助项目 | Basic Research of Yunnan Province in China; NSFC[12373060]; Strategic Priority Research Program of the Chinese Academy of Sciences[XDB0560000]; National Key R&D Program of China[2022YFF0503804]; National Key R&D Program of China[2022YFF0503800]; Youth Innovation Promotion Association CAS[Y2021024]; International Space Science Institute (ISSI) in Bern, through ISSI International Team project[23-586]; 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:001522733400001 |
| 出版者 | IOP Publishing Ltd |
| 资助机构 | Basic Research of Yunnan Province in China ; NSFC[12373060] ; Strategic Priority Research Program of the Chinese Academy of Sciences[XDB0560000] ; National Key R&D Program of China[2022YFF0503804, 2022YFF0503800] ; Youth Innovation Promotion Association CAS[Y2021024] ; International Space Science Institute (ISSI) in Bern, through ISSI International Team project[23-586] ; Yunnan Key Laboratory of Solar Physics and Space Science[202205AG070009] ; [202401AS070044] |
| 版本 | 出版稿 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/28404]  |
| 专题 | 云南天文台_太阳物理研究组 |
| 通讯作者 | Ni L(倪蕾) |
| 作者单位 | 1.Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA 2.Yunnan Key Laboratory of Solar Physics and Space Science, Kunming 650216, People’s Republic of China; 3.University of Chinese Academy of Sciences, Beijing 100049, People’s Republic of China; 4.Yunnan Observatories, Chinese Academy of Sciences, Kunming, Yunnan 650216, People’s Republic of China; leini@ynao.ac.cn, chengguanchong@ynao.ac.cn; |
| 推荐引用方式 GB/T 7714 | Wang YF,Ni L,Cheng GC,et al. Numerical Simulation of Oscillatory Magnetic Reconnection Modulated by Solar Convective Motions[J]. ASTROPHYSICAL JOURNAL,2025,987(2). |
| APA | 王逸夫,倪蕾,程冠冲,胡佳亮,陈雨豪,&Zafar, Abdullah.(2025).Numerical Simulation of Oscillatory Magnetic Reconnection Modulated by Solar Convective Motions.ASTROPHYSICAL JOURNAL,987(2). |
| MLA | 王逸夫,et al."Numerical Simulation of Oscillatory Magnetic Reconnection Modulated by Solar Convective Motions".ASTROPHYSICAL JOURNAL 987.2(2025). |
入库方式： OAI收割
来源：云南天文台
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