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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.
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页数:11
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