Numerical experiments of fast magnetic reconnection driven by the rapidly expanding plasma
文献类型：期刊论文
| 作者 | Xu SS(许杉杉)3,4 ; Lin J(林隽)1,2,3,4; Mei ZX(梅志星)1,2,4
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| 刊名 | SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
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| 出版日期 | 2025-07-01 |
| 卷号 | 68期号:9 |
| 关键词 | magnetic reconnction shock waves MHD numerical simulation |
| ISSN号 | 1674-7348 |
| DOI | 10.1007/s11433-025-2688-0 |
| 产权排序 | 第1完成单位 |
| 文献子类 | Article |
| 英文摘要 | Three modes of magnetic reconnection, flux pile-up, Sonnerup, and hybrid, are examined in the context of driven magnetic reconnection via 2D and 2.5D magnetohydrodynamic (MHD) numerical simulations. They result from variances in gas pressure and magnetic field strength in the reconnection inflow region. The simulation demonstrates that the Spitzer diffusion region of magnetic reconnection is not just an X-point; instead, it appears as a slim and elongated current sheet that creates two pairs of the slow-mode shock (SS) on either end. These shocks contribute to forming four boundaries that separate the inflow from the outflow. In the regions far from the Spitzer diffusion region, two sets of rotational discontinuity (RD) stand inside the SSs and form the combination of SS and RD structures. The RDs reverse the magnetic field inside the reconnection outflow region, and create a W-shaped magnetic field in that region. The scenario that the rotation of the magnetic field is not caused by an intermediate wave, and the SS is located outside the RD, is consistent with the inference of Priest (Mon. Not. R. Astron. Soc. 159, 389 (1972)), and is contrary to that of Petschek and Thorne (Astrophys. J. 147, 1157 (1967)) and Vasyliunas (Rev. Geophys. Space Phys. 13, 303 (1975)). |
| 学科主题 | 天文学 ; 太阳与太阳系 |
| URL标识 | 查看原文 |
| 出版地 | 16 DONGHUANGCHENGGEN NORTH ST, BEIJING 100717, PEOPLES R CHINA |
| WOS关键词 | CURRENT SHEET ; ENERGY-CONVERSION ; SOLAR ; MODELS ; ENHANCEMENT ; FIELDS ; FLARES |
| 资助项目 | National Key R&D Program of China[2022YFF0503804]; National Natural Science Foundation of China[11933009]; National Natural Science Foundation of China[12273107]; National Natural Science Foundation of China[U2031141]; Applied Basic Research of Yunnan Province[2019FB005]; Yunnan Province Scientist Workshop of Solar Physics; Yunnan Province Yunling Scholar Project |
| WOS研究方向 | Physics |
| 语种 | 英语 |
| WOS记录号 | WOS:001522739300001 |
| 出版者 | SCIENCE PRESS |
| 资助机构 | National Key R&D Program of China[2022YFF0503804] ; National Natural Science Foundation of China[11933009, 12273107, U2031141] ; Applied Basic Research of Yunnan Province[2019FB005] ; Yunnan Province Scientist Workshop of Solar Physics ; Yunnan Province Yunling Scholar Project |
| 版本 | 出版稿 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/28385]  |
| 专题 | 云南天文台_太阳物理研究组 |
| 通讯作者 | Lin J(林隽) |
| 作者单位 | 1.Yunnan Key Laboratory of Solar Physics and Space Science, Kunming, 650216, China 2.Center for Astronomical Mega-Science, Chinese Academy of Sciences, Beijing, 100012, China; 3.University of Chinese Academy of Sciences, Beijing, 100049, China; 4.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, China; |
| 推荐引用方式 GB/T 7714 | Xu SS,Lin J,Mei ZX. Numerical experiments of fast magnetic reconnection driven by the rapidly expanding plasma[J]. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,2025,68(9). |
| APA | 许杉杉,林隽,&梅志星.(2025).Numerical experiments of fast magnetic reconnection driven by the rapidly expanding plasma.SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,68(9). |
| MLA | 许杉杉,et al."Numerical experiments of fast magnetic reconnection driven by the rapidly expanding plasma".SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY 68.9(2025). |
入库方式： OAI收割
来源：云南天文台
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