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DOI | 10.1029/2019GL083283 |
Whistler Waves Driven by Field-Aligned Streaming Electrons in the Near-Earth Magnetotail Reconnection | |
Ren, Y.1; Dai, L.1; Li, W.2; Tao, X.3; Wang, C.1; Tang, B.1; Lavraud, B.4; Wu, Y.3; Burch, J. L.5; Giles, B. L.6; Le Contel, O.7; Torbert, R. B.8; Russell, C. T.9; Strangeway, R. J.9; Ergun, R. E.1,10; Lindqvist, P-A1,11 | |
2019-05-28 | |
发表期刊 | GEOPHYSICAL RESEARCH LETTERS |
ISSN | 0094-8276 |
EISSN | 1944-8007 |
出版年 | 2019 |
卷号 | 46期号:10页码:5045-5054 |
文章类型 | Article |
语种 | 英语 |
国家 | Peoples R China; USA; France; Sweden |
英文摘要 | We analyze Magnetospheric Multiscale Mission observations of whistler waves and associated electron field-aligned crescent distribution in the vicinity of the magnetotail near-Earth X-line. The whistler waves propagate outward from the X-line in the neutral sheet. The associated field-aligned streaming electrons exhibit a crescent-like shape, with an inverse slope (df/d vertical bar v(parallel to)vertical bar > 0) at 1-5 keV. The parallel phase velocity of the waves is in the range (1-5 keV) of the inverse slope of the field-aligned crescents in the velocity space. We demonstrate that the observed whistler waves are driven by the electron field-aligned crescents through Landau resonance. The cyclotron resonance is at the high-energy tail with negligible free energy of pitch angle anisotropy in these events. |
领域 | 气候变化 |
收录类别 | SCI-E |
WOS记录号 | WOS:000471237500005 |
WOS关键词 | MAGNETIC RECONNECTION ; DAYSIDE MAGNETOPAUSE ; SEPARATRIX REGIONS ; HALL FIELDS ; MODE WAVES ; MMS |
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/183368 |
专题 | 气候变化 |
作者单位 | 1.Chinese Acad Sci, Natl Space Sci Ctr, State Key Lab Space Weather, Beijing, Peoples R China; 2.Boston Univ, Ctr Space Phys, Boston, MA 02215 USA; 3.Univ Sci & Technol China, Dept Geophys & Planetary Sci, CAS Key Lab Geospace Environm, Hefei, Anhui, Peoples R China; 4.Univ Toulouse, Inst Rech Astrophys & Planetol, CNRS, UPS,CNES, Toulouse, France; 5.Southwest Res Inst, San Antonio, TX USA; 6.NASA, Goddard Space Flight Ctr, Greenbelt, MD USA; 7.Univ Paris Sud, Sorbonne Univ, Observ Paris, Lab Phys Plasmas,CNRS,Ecole Polytech, Paris, France; 8.Univ New Hampshire, Dept Phys, Durham, NH 03824 USA; 9.Univ Calif Los Angeles, Earth & Planetary Sci, Los Angeles, CA USA; 10.Univ Colorado, Dept Astrophys & Planetary Sci, Boulder, CO 80309 USA; 11.Roya Inst Technol, Space & Plasma Grp, Stockholm, Sweden |
推荐引用方式 GB/T 7714 | Ren, Y.,Dai, L.,Li, W.,et al. Whistler Waves Driven by Field-Aligned Streaming Electrons in the Near-Earth Magnetotail Reconnection[J]. GEOPHYSICAL RESEARCH LETTERS,2019,46(10):5045-5054. |
APA | Ren, Y..,Dai, L..,Li, W..,Tao, X..,Wang, C..,...&Lindqvist, P-A.(2019).Whistler Waves Driven by Field-Aligned Streaming Electrons in the Near-Earth Magnetotail Reconnection.GEOPHYSICAL RESEARCH LETTERS,46(10),5045-5054. |
MLA | Ren, Y.,et al."Whistler Waves Driven by Field-Aligned Streaming Electrons in the Near-Earth Magnetotail Reconnection".GEOPHYSICAL RESEARCH LETTERS 46.10(2019):5045-5054. |
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