Modelling loop-top X-ray source and reconnection outflows in solar flares with intense lasers
文献类型：期刊论文
| 作者 | Zhong, JY ; Li, YT ; Wang, XG ; Wang, JQ ; Dong, QL ; Xiao, CJ ; Wang, SJ ; Liu, X ; Zhang, L ; An, L ; Wang, FL ; Zhu, JQ ; Gu, YA ; He, XT ; Zhao, G ; Zhang, J |
| 刊名 | NATURE PHYSICS
 |
| 出版日期 | 2010 |
| 卷号 | 6期号:12页码:984 |
| 关键词 | MAGNETIC RECONNECTION PLASMAS JETS ASTROPHYSICS FIELDS |
| ISSN号 | 1745-2473 |
| 通讯作者 | Zhao, G: Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China. |
| 中文摘要 | Magnetic reconnection is a process by which oppositely directed magnetic field lines passing through a plasma undergo dramatic rearrangement, converting magnetic potential into kinetic energy and heat(1,2). It is believed to play an important role in many plasma phenomena including solar flares(3,4), star formation(5) and other astrophysical events(6), laser-driven plasma jets(7-9), and fusion plasma instabilities(10). Because of the large differences of scale between laboratory and astrophysical plasmas, it is often difficult to extrapolate the reconnection phenomena studied in one environment to those observed in the other. In some cases, however, scaling laws(11) do permit reliable connections to made, such as the experimental simulation of interactions between the solar wind and the Earth's magnetosphere(12). Here we report well-scaled laboratory experiments that reproduce loop-top-like X-ray source emission by reconnection outflows interacting with a solid target. Our experiments exploit the mega-gauss-scale magnetic field generated by interaction of a high-intensity laser with a plasma to reconstruct a magnetic reconnection topology similar to that which occurs in solar flares. We also identify the separatrix and diffusion regions associated with reconnection in which ions become decoupled from electrons on a scale of the ion inertial length. |
| 收录类别 | SCI |
| 资助信息 | National Basic Research Program of China (973 Program) [2007CB815100, 2009GB105004, 2006CB806300]; National Natural Science Foundation of China [10821061, 10925421, 10734130, 40731056, 40974104, 10975012] |
| 语种 | 英语 |
| 公开日期 | 2013-09-18 |
| 源URL | [http://ir.iphy.ac.cn/handle/311004/42216]  |
| 专题 | 物理研究所_物理所公开发表论文_物理所公开发表论文_期刊论文 |
| 推荐引用方式 GB/T 7714 | Zhong, JY,Li, YT,Wang, XG,et al. Modelling loop-top X-ray source and reconnection outflows in solar flares with intense lasers[J]. NATURE PHYSICS,2010,6(12):984. |
| APA | Zhong, JY.,Li, YT.,Wang, XG.,Wang, JQ.,Dong, QL.,...&Zhang, J.(2010).Modelling loop-top X-ray source and reconnection outflows in solar flares with intense lasers.NATURE PHYSICS,6(12),984. |
| MLA | Zhong, JY,et al."Modelling loop-top X-ray source and reconnection outflows in solar flares with intense lasers".NATURE PHYSICS 6.12(2010):984. |
入库方式： OAI收割
来源：物理研究所
浏览0
下载0
收藏0
其他版本
除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。