Analysis of the interaction between low-frequency waves and ions in the high-altitude cusp region observed by satellite cluster

被引:0
|
作者
Duan Su-Ping [1 ]
Liu Zhen-Xing
Cao Jin-Bin
Shi Jian-Kui
Lu Li
Li Zhong-Yuan
Zong, Q. G.
Reme, H.
Cornilleau-Wehrlin, N.
Balogh, A.
Andre, M.
机构
[1] Chinese Acad Sci, Ctr Space Sci & Appl Res, Key Lab Space Weather, Beijing 100080, Peoples R China
[2] Univ Sci & Technol China, Sch Earth & Space Sci, Hefei 230026, Peoples R China
[3] Boston Univ, Ctr Space Phys, Boston, MA 02215 USA
[4] CNRS, CESR, F-31028 Toulouse 4, France
[5] CETP, F-78140 Velizy Villacoublay, France
[6] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Space & Atmospher Phys Grp, London SW7 2BZ, England
[7] Swedish Inst Space Phys, Uppsala Div, SE-75121 Uppsala, Sweden
关键词
D O I
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中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The energy transfer between ions (protons) and low frequency waves (LFWs) in the frequency range f(1) from 0.3 to 10 Hz is observed by Cluster crossing the high-altitude polar cusp. The energy transfer between low frequency waves and ions has two means. One is that the energy is transferred from low frequency waves to ions and ions energy increases. The other is that the energy is transferred from ions to low frequency waves and the ion energy decreases. Ion gyratory motion plays an important role in the energy transfer processes. The electromagnetic field of f(1) LFWs can accelerate or decelerate protons along the direction of ambient magnetic field and warm or refrigerate protons in the parallel and perpendicular directions of ambient magnetic field. The peak values of proton number densities have the corresponding peak values of electromagnetic energy of low-frequency waves. This implies that the kinetic Alfven waves and solitary kinetic Alfven waves possibly exist in the high-altitude cusp region.
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页码:1351 / 1354
页数:4
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