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DOI | 10.1029/2018GL081420 |
Effects of Cross-Sheet Density and Temperature Inhomogeneities on Magnetotail Reconnection | |
Lu, San1,2; Artemyev, A. V.1,2,3; Angelopoulos, V.1,2; Pritchett, P. L.4; Runov, A.1,2 | |
2019-01-16 | |
发表期刊 | GEOPHYSICAL RESEARCH LETTERS |
ISSN | 0094-8276 |
EISSN | 1944-8007 |
出版年 | 2019 |
卷号 | 46期号:1页码:28-36 |
文章类型 | Article |
语种 | 英语 |
国家 | USA; Russia |
英文摘要 | Properties of magnetic reconnection in Earth's magnetotail are determined by prereconnection current sheet characteristics. Although spacecraft observations have revealed that the spatial profiles of two important parameters, density and temperature, across the prereconnection magnetotail current sheet are inhomogeneous, the effects of the inhomogeneities on reconnection processes have received insufficient attention. Using Time History of Events and Macroscale Interactions during Substorm (THEMIS) and Acceleration, Reconnection, Turbulence, and Electrodynamics of Moon's Interaction with the Sun (ARTEMIS) observations, we show that the inhomogeneities are ubiquitous throughout the magnetotail. Using particle-in-cell simulations, we demonstrate that strong density inhomogeneity increases magnetotail reconnection rate, and strong temperature inhomogeneity further increases reconnection outflow speed (although reconnection rate does not change significantly). Overall, these inhomogeneities expedite energy conversion efficiency and secondary plasmoid formation during reconnection. As the current sheet density and temperature characteristics vary considerably with geocentric distance and time under different geospace conditions, a large variety of reconnection and postreconnection dynamics results from this dependence. Plain Language Summary Magnetic reconnection, a fundamental plasma process by which magnetic energy is explosively released to accelerate and heat charged particles via topologic change of magnetic field lines, happens in Earth's magnetotail current sheet. This magnetotail current sheet has inhomogeneous density and temperature profiles across it. We demonstrate that these density and temperature inhomogeneities are important because they exist throughout the magnetotail and control properties of magnetotail reconnection in various aspects. |
英文关键词 | magnetic reconnection magnetotail current sheet |
领域 | 气候变化 |
收录类别 | SCI-E |
WOS记录号 | WOS:000456938600004 |
WOS关键词 | MAGNETIC RECONNECTION ; ELECTRON ACCELERATION ; DIPOLARIZATION FRONTS ; ONSET ; THEMIS |
WOS类目 | Geosciences, Multidisciplinary |
WOS研究方向 | Geology |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://119.78.100.173/C666/handle/2XK7JSWQ/26016 |
专题 | 气候变化 |
作者单位 | 1.Univ Calif Los Angeles, Dept Earth Planetary & Space Sci, Los Angeles, CA 90095 USA; 2.Univ Calif Los Angeles, Inst Geophys & Planetary Phys, Los Angeles, CA 90095 USA; 3.RAS, Space Res Inst, Moscow, Russia; 4.Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA USA |
推荐引用方式 GB/T 7714 | Lu, San,Artemyev, A. V.,Angelopoulos, V.,et al. Effects of Cross-Sheet Density and Temperature Inhomogeneities on Magnetotail Reconnection[J]. GEOPHYSICAL RESEARCH LETTERS,2019,46(1):28-36. |
APA | Lu, San,Artemyev, A. V.,Angelopoulos, V.,Pritchett, P. L.,&Runov, A..(2019).Effects of Cross-Sheet Density and Temperature Inhomogeneities on Magnetotail Reconnection.GEOPHYSICAL RESEARCH LETTERS,46(1),28-36. |
MLA | Lu, San,et al."Effects of Cross-Sheet Density and Temperature Inhomogeneities on Magnetotail Reconnection".GEOPHYSICAL RESEARCH LETTERS 46.1(2019):28-36. |
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