| Coronal Wave Trains and Plasma Heating Triggered by Turbulence in the Wake of a CME | |
Ye J(叶景)1,2 ; Cai, Qiangwei3; Shen, Chengcai4; Raymond, John C.4; Mei ZX(梅志星)1,2; Li Y(李燕)1,2; Lin J(林隽)1,2,5
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| 发表期刊 | ASTROPHYSICAL JOURNAL
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| 2021-03-01 | |
| 卷号 | 909期号:1页码:11 |
| DOI | 10.3847/1538-4357/abdeb5 |
| 产权排序 | 第1完成单位 |
| 收录类别 | SCI |
| 关键词 | Magnetohydrodynamical simulations Solar coronal mass ejections Termination shock Solar extreme ultraviolet emission |
| 摘要 | Magnetohydrodynamic (MHD) turbulence plays an important role for the fast energy release and wave structures related to coronal mass ejections (CMEs). The CME plasma has been observed to be strongly heated during solar eruptions, but the heating mechanism is not understood. In this paper, we focus on the hot, dense region at the bottom of the CME and the generation of coronal wave trains therein using a high-resolution 2.5D MHD simulation. Our results show that the interaction between the tearing current sheet and the turbulence, including the termination shocks (TSs) at the bottom of the CME, can make a significant contribution to heating the CME, and the heating rate in this region is found to be greater than the kinetic energy transfer rate. Also, the turbulence can be somewhat amplified by the TSs. The compression ratio of the TS under the CME can exceed 4 due to thermal conduction, but such a strong TS is hardly detectable in all Solar Dynamics Observatory/Atmospheric Imaging Assembly bands. And turbulence is an indispensable source for the periodic generation of coronal wave trains around the CME. |
| 资助项目 | Strategic Priority Research Program of CAS[XDA17040507] ; National Natural Science Foundation of China (NSFC)[12073073] ; National Natural Science Foundation of China (NSFC)[11933009] ; Yunling Scholar Project of the Yunnan Province ; Natural Science Foundation of Henan Province[212300410210] ; NSFC[U2031141] ; Applied Basic Research of Yunnan Province[2019FB005] ; Yunnan Province Scientist Workshop of Jun Lin |
| 项目资助者 | Strategic Priority Research Program of CAS[XDA17040507] ; National Natural Science Foundation of China (NSFC)[12073073, 11933009] ; Yunling Scholar Project of the Yunnan Province ; Natural Science Foundation of Henan Province[212300410210] ; NSFC[U2031141] ; Applied Basic Research of Yunnan Province[2019FB005] ; Yunnan Province Scientist Workshop of Jun Lin |
| 语种 | 英语 |
| 学科领域 | 天文学 ; 太阳与太阳系 ; 太阳物理学 |
| 文章类型 | Article |
| 出版者 | IOP PUBLISHING LTD |
| 出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
| ISSN | 0004-637X |
| URL | 查看原文 |
| WOS记录号 | WOS:000625785300001 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 引用统计 | |
| 文献类型 | 期刊论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/24195 |
| 专题 | 太阳物理研究组 |
| 通讯作者 | Ye J(叶景) |
| 作者单位 | 1.Coronal Wave Trains and Plasma Heating Triggered by Turbulence in the Wake of a CME 2.Center for Astronomical Mega-Science, Chinese Academy of Sciences, Beijing 100012, People's Republic of China 3.Institute of Space Physics, Luoyang Normal University, Luoyang, Henan 471934, People's Republic of China 4.Smithsonian Astrophysical Observatory, 60 Garden Street, MS 15, Cambridge, MA 02138, USA 5.University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China |
| 推荐引用方式 GB/T 7714 | Ye J,Cai, Qiangwei,Shen, Chengcai,et al. Coronal Wave Trains and Plasma Heating Triggered by Turbulence in the Wake of a CME[J]. ASTROPHYSICAL JOURNAL,2021,909(1):11. |
| APA | Ye J.,Cai, Qiangwei.,Shen, Chengcai.,Raymond, John C..,Mei ZX.,...&Lin J.(2021).Coronal Wave Trains and Plasma Heating Triggered by Turbulence in the Wake of a CME.ASTROPHYSICAL JOURNAL,909(1),11. |
| MLA | Ye J,et al."Coronal Wave Trains and Plasma Heating Triggered by Turbulence in the Wake of a CME".ASTROPHYSICAL JOURNAL 909.1(2021):11. |
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| Coronal Wave Trains （4827KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | |
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