中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Nonlinear bounce resonances between magnetosonic waves and equatorially mirroring electrons

文献类型:期刊论文

作者Chen, Lunjin; Maldonado, Armando; Bortnik, Jacob; Thorne, Richard M.; Li, Jinxing; Dai, Lei; Zhan, Xiaoya
刊名JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
出版日期2015
卷号120期号:8页码:6514-6527
关键词bounce resonance magnetosonic waves equatorial noise radiation belt wave-particle interaction nonlinear
ISSN号2169-9380
通讯作者Chen, LJ (reprint author), Univ Texas Dallas, Dept Phys, Richardson, TX 75083 USA.
英文摘要Equatorially mirroring energetic electrons pose an interesting scientific problem, since they generally cannot resonate with any known plasma waves and hence cannot be scattered down to lower pitch angles. Observationally it is well known that the flux of these equatorial particles does not simply continue to build up indefinitely, and so a mechanism must necessarily exist that transports these particles from an equatorial pitch angle of 90 degrees down to lower values. However, this mechanism has not been uniquely identified yet. Here we investigate the mechanism of bounce resonance with equatorial noise (or fast magnetosonic waves). A test particle simulation is used to examine the effects of monochromatic magnetosonic waves on the equatorially mirroring energetic electrons, with a special interest in characterizing the effectiveness of bounce resonances. Our analysis shows that bounce resonances can occur at the first three harmonics of the bounce frequency (n omega(b), n = 1, 2, and 3) and can effectively reduce the equatorial pitch angle to values where resonant scattering by whistler mode waves becomes possible. We demonstrate that the nature of bounce resonance is nonlinear, and we propose a nonlinear oscillation model for characterizing bounce resonances using two key parameters, effective wave amplitude (A) over tilde and normalized wave number (k) over tilde (z). The threshold for higher harmonic resonance is more strict, favoring higher (A) over tilde and (k) over tilde (z), and the change in equatorial pitch angle is strongly controlled by (k) over tilde (z). We also investigate the dependence of bounce resonance effects on various physical parameters, including wave amplitude, frequency, wave normal angle and initial phase, plasma density, and electron energy. It is found that the effect of bounce resonance is sensitive to the wave normal angle. We suggest that the bounce resonant interaction might lead to an observed pitch angle distribution with a minimum at 90 degrees.
收录类别SCI
语种英语
源URL[http://ir.nssc.ac.cn/handle/122/5089]  
专题国家空间科学中心_空间科学部
推荐引用方式
GB/T 7714
Chen, Lunjin,Maldonado, Armando,Bortnik, Jacob,et al. Nonlinear bounce resonances between magnetosonic waves and equatorially mirroring electrons[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2015,120(8):6514-6527.
APA Chen, Lunjin.,Maldonado, Armando.,Bortnik, Jacob.,Thorne, Richard M..,Li, Jinxing.,...&Zhan, Xiaoya.(2015).Nonlinear bounce resonances between magnetosonic waves and equatorially mirroring electrons.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,120(8),6514-6527.
MLA Chen, Lunjin,et al."Nonlinear bounce resonances between magnetosonic waves and equatorially mirroring electrons".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 120.8(2015):6514-6527.

入库方式: OAI收割

来源:国家空间科学中心

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。