Plasmoids in reconnecting current sheets: Solar and terrestrial contexts compared
文献类型:期刊论文
作者 | Lin J(林隽)1,2![]() |
刊名 | JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
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出版日期 | 2008-11-29 |
卷号 | 113期号:A11 |
ISSN号 | 0148-0227 |
产权排序 | 第一完成单位 |
通讯作者 | Lin, J (reprint author), Chinese Acad Sci, Natl Astron Observ China, Yunnan Astron Observ, POB 110, Kunming 650011, Yunnan, Peoples R China. |
英文摘要 | Magnetic reconnection plays a crucial role in violent energy conversion occurring in the environments of high electrical conductivity, such as the solar atmosphere, magnetosphere, and fusion devices. We focus on the morphological features of the process in two different environments, the solar atmosphere and the geomagnetic tail. In addition to indirect evidence that indicates reconnection in progress or having just taken place, such as auroral manifestations in the magnetosphere and the flare loop system in the solar atmosphere, more direct evidence of reconnection in the solar and terrestrial environments is being collected. Such evidence includes the reconnection inflow near the reconnecting current sheet and the outflow along the sheet characterized by a sequence of plasmoids. Both turbulent and unsteady Petschek-type reconnection processes could account for the observations. We also discuss other relevant observational consequences of both mechanisms in these two settings. While on face value, these are two completely different physical environments, there emerge many commonalities, for example, an Alfven speed of the same order of magnitude, a key parameter determining the reconnection rate. This comparative study is meant as a contribution to current efforts aimed at isolating similarities in processes occurring in very different contexts in the heliosphere and even in the universe. |
WOS标题词 | Science & Technology ; Physical Sciences |
学科主题 | Astronomy & Astrophysics |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | CORONAL MASS EJECTIONS ; SLOW-MODE SHOCKS ; INTERPLANETARY MAGNETIC CLOUD ; TRAVELING COMPRESSION REGIONS ; PETSCHEK-TYPE RECONNECTION ; 3-DIMENSIONAL FLUX ROPES ; X-LINE RECONNECTION ; 2002 JULY 23 ; MAGNETOHYDRODYNAMIC TURBULENCE ; EARTHS MAGNETOPAUSE |
收录类别 | SCI |
原文出处 | http://onlinelibrary.wiley.com/doi/10.1029/2008JA013409/abstract |
语种 | 英语 |
WOS记录号 | WOS:000261247600003 |
公开日期 | 2016-05-03 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/6118] ![]() |
专题 | 云南天文台_太阳物理研究组 |
作者单位 | 1.Yunnan Astronomical Observatory, National Astronomical Observatories of China, Chinese Academy of Sciences, Kunming, Yunnan, China 2.Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts, USA 3.Institute for the Study of Earth, Ocean, and Space, University of New Hampshire, USA |
推荐引用方式 GB/T 7714 | Lin J,Cranmer, SR,Farrugia, CJ. Plasmoids in reconnecting current sheets: Solar and terrestrial contexts compared[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2008,113(A11). |
APA | Lin J,Cranmer, SR,&Farrugia, CJ.(2008).Plasmoids in reconnecting current sheets: Solar and terrestrial contexts compared.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,113(A11). |
MLA | Lin J,et al."Plasmoids in reconnecting current sheets: Solar and terrestrial contexts compared".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 113.A11(2008). |
入库方式: OAI收割
来源:云南天文台
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