Electrostatic broadband ELF wave emission by Alfven wave breaking

被引:38
作者
Seyler, CE
Clark, AE
Bonnell, J
Wahlund, JE
机构
[1] Cornell Univ, Sch Elect Engn, Ithaca, NY 14853 USA
[2] Swedish Inst Space Phys, IRF, S-98128 Kiruna, Sweden
来源
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS | 1998年 / 103卷 / A4期
关键词
D O I
10.1029/97JA02297
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The linear and nonlinear kinetic properties of electrostatic oblique waves below the lower hybrid frequency are investigated. For propagation angles l = k(parallel to)/k(perpendicular to) < root m(e)/m(i) the waves are damped by either parallel electron Landau or ion cyclotron damping. For T-i/T-e much greater than 1 the waves are only weakly damped and can propagate. These waves are called slow ion cyclotron (SIG) and slow ion acoustic (SIA) waves. A fluid-kinetic model, comprised of hot linear kinetic ions and cold nonlinear fluid electrons, is proposed to describe a nonlinear wave breaking process of small-scale Alfven waves resulting in broadband extremely low-frequency (ELF) wave emission. Numerical solutions of the fluid-kinetic model are compared to the electric and magnetic fields of solitary kinetic Alfven waves and broadband ELF waves observed by the Freja satellite within a hot ion environment. The agreement in waveform morphology and amplitude between the fluid-kinetic simulations and the observed waves provides support for the theory that observed SIA waves are the result of a nonlinear emission process from SIC waves.
引用
收藏
页码:7027 / 7041
页数:15
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