An Unexpected Whistler Wave Generation Around Dipolarization Front

被引:21
作者
Chen, G. [1 ,2 ,3 ,4 ]
Fu, H. S. [5 ]
Zhang, Y. [1 ,2 ,3 ,4 ]
Su, Z. P. [6 ,7 ]
Liu, N. G. [6 ,7 ]
Chen, L. [8 ]
Ge, Y. S. [1 ,2 ,3 ,4 ]
Du, A. M. [1 ,2 ,3 ,4 ]
Liu, C. M. [5 ]
Wang, Z. [5 ]
Chen, F. [5 ]
机构
[1] Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China
[2] Chinese Acad Sci, Innovat Acad Earth Sci, Beijing, Peoples R China
[3] Univ Chinese Acad Sci, Coll Earth & Planetary Sci, Beijing, Peoples R China
[4] China State Shipbldg Corp, Lab Sci & Technol Marine Nav & Control, Tianjin, Peoples R China
[5] Beihang Univ, Sch Space & Environm, Beijing, Peoples R China
[6] Univ Sci & Technol China, Dept Geophys & Planetary Sci, CAS Key Lab Geospace Environm, Hefei, Peoples R China
[7] Univ Sci & Technol China, CAS Ctr Excellence Comparat Planetol, Hefei, Peoples R China
[8] Univ Texas Dallas, Dept Phys, Richardson, TX 75083 USA
基金
中国博士后科学基金;
关键词
dipolarization front; whistler waves; SUPRATHERMAL ELECTRON ACCELERATION; ROLLING-PIN DISTRIBUTION; PARTICLE-ACCELERATION; RECONNECTION ONSET; PLASMA; MAGNETOTAIL; MMS; INSTABILITY; INJECTIONS; EMISSIONS;
D O I
10.1029/2020JA028957
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Dipolarization front (DF)-a sharp boundary separating hot tenuous plasmas from cold dense plasmas-is followed by a strong B-z region, which is termed flux pileup region (FPR) or dipolarizing flux bundle (DFB). Using 9-year (2001-2009) Cluster data, we show that the FPR hosts whistler waves because of the pancake distribution of electrons, whereas the DF boundary hosts lower hybrid drift waves due to the strong density and magnetic gradients statistically. Different from statistical results, we report an unexpected case: whistler waves are generated at the DF boundary rather than inside the FPR. Using Cluster data, we observed strong whistler waves at DF boundaries but no whistlers inside FPRs, although flux tubes inside the FPRs are significantly compressed and suprathermal electrons there are perpendicularly anisotropic. We calculate wave growth rates and successfully explain the generation/damping of these whistlers. We find that 1-4 keV electrons are responsible for generation/damping of these whistlers.
引用
收藏
页数:12
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