Modulation of Whistler Mode Waves by Ion-Scale Waves Observed in the Distant Magnetotail

被引:3
|
作者
Zhao, Duo [1 ]
Fu, Suiyan [2 ]
Parks, George K. [3 ]
Chen, Lunjin [4 ]
Liu, Xu [4 ]
Tong, Yuguang [3 ]
Li, Jinxing [5 ]
Pu, Zuyin [2 ]
Zong, Qiugang [2 ]
Sun, Weijie [6 ]
Li, Shouxian [1 ]
An, JianZhu [1 ]
机构
[1] Inst Appl Phys & Computat Math, Beijing, Peoples R China
[2] Peking Univ, Sch Earth & Space Sci, Beijing, Peoples R China
[3] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[4] Univ Texas Dallas, William B Hanson Ctr Space Sci, Richardson, TX 75083 USA
[5] Univ Calif Los Angeles, Dept Atmospher & Ocean Sci, Los Angeles, CA USA
[6] Univ Michigan, Dept Climate & Space Sci & Engn, Ann Arbor, MI 48109 USA
关键词
CHORUS EMISSIONS; PLASMA SHEET; PROPAGATION; FLOWS; ACCELERATION; ELECTRONS;
D O I
10.1029/2019JA027278
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Wave activities in tailward flows have been explored in the distant magnetotail at similar to 54 RE, where the coupling between whistler mode waves and ion-scale waves was observed. The whistler mode waves periodically appeared at each cycle of the ion-scale waves, and the electron distribution functions associated with the whistler mode waves showed enhancement in the direction parallel to background magnetic field. Wave analyses show that the field-aligned electron components act as the energy source of the whistler mode waves. The ion-scale waves are generated by the interaction of the hot ion beam with background ions. A likely candidate of the ion-scale wave is the kinetic Alfven wave, which can generate the enhanced field-aligned electron populations by the parallel electric field.
引用
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页数:11
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