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Chinese Academy of Sciences Institutional Repositories Grid
Bounce-averaged diffusion coefficients for superluminous wave modes in the magnetosphere

文献类型:期刊论文

作者Xiao, Fuliang; Chen, Liangxu; He, Yihua
刊名JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS
出版日期2011
卷号73期号:1页码:88-94
关键词Wave-particle interaction Superluminous waves Bounce-averaged diffusion coefficients
ISSN号1364-6826
通讯作者Xiao, FL (reprint author), Changsha Univ Sci & Technol, Sch Phys & Elect Sci, Changsha 410004, Hunan, Peoples R China.
中文摘要In this study, we present a first evaluation of bounce-averaged diffusion coefficients of superluminous wave (R-X and L-O) modes at two locations: L = 6.5 and 4.5. We show that, analogous to the local diffusion coefficients, bounce-averaged momentum diffusion coefficients play a dominant role for pitch angles alpha above a critical angle alpha(c), namely, < D(pp)> > vertical bar < D(p alpha)> vertical bar > < D(alpha alpha)>. We also demonstrate that for a Gaussian distribution of wave normal angle theta (X = tan theta). diffusion coefficients are sensitively dependent on the peak X(m). As X(m) increases, < D(pp)> and < D(alpha alpha)> are found to increase in cases of interest: X(m) = tan 25 degrees, tan 45 degrees and tan 65 degrees. We have estimated wave amplitudes for particular stochastic acceleration timescale for 1 MeV electrons and found that the required wave amplitudes B(te) similar to 86 to similar to 170 pT for a timescale tau = 1 day. These results indicate that superluminous wave modes may have a significant potential for both stochastic acceleration of trapped electrons (with higher pitch angles) and loss process of untrapped electrons (with smaller pitch angles). (C) 2009 Elsevier Ltd. All rights reserved.
英文摘要In this study, we present a first evaluation of bounce-averaged diffusion coefficients of superluminous wave (R-X and L-O) modes at two locations: L = 6.5 and 4.5. We show that, analogous to the local diffusion coefficients, bounce-averaged momentum diffusion coefficients play a dominant role for pitch angles alpha above a critical angle alpha(c), namely, < D(pp)> > vertical bar < D(p alpha)> vertical bar > < D(alpha alpha)>. We also demonstrate that for a Gaussian distribution of wave normal angle theta (X = tan theta). diffusion coefficients are sensitively dependent on the peak X(m). As X(m) increases, < D(pp)> and < D(alpha alpha)> are found to increase in cases of interest: X(m) = tan 25 degrees, tan 45 degrees and tan 65 degrees. We have estimated wave amplitudes for particular stochastic acceleration timescale for 1 MeV electrons and found that the required wave amplitudes B(te) similar to 86 to similar to 170 pT for a timescale tau = 1 day. These results indicate that superluminous wave modes may have a significant potential for both stochastic acceleration of trapped electrons (with higher pitch angles) and loss process of untrapped electrons (with smaller pitch angles). (C) 2009 Elsevier Ltd. All rights reserved.
学科主题空间物理
收录类别SCI ; EI
资助信息National Natural Science Foundation of China [40774078, 40874076, 40931053, 40925014]; Special Fund for Public Welfare Industry (meteorology) [GYHY200806024]; Changsha University of Science and Technology; State Key Laboratories for Space Weather, Chinese Academy of Sciences
语种英语
公开日期2014-12-15
源URL[http://ir.nssc.ac.cn/handle/122/3119]  
专题国家空间科学中心_空间科学部
推荐引用方式
GB/T 7714
Xiao, Fuliang,Chen, Liangxu,He, Yihua. Bounce-averaged diffusion coefficients for superluminous wave modes in the magnetosphere[J]. JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS,2011,73(1):88-94.
APA Xiao, Fuliang,Chen, Liangxu,&He, Yihua.(2011).Bounce-averaged diffusion coefficients for superluminous wave modes in the magnetosphere.JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS,73(1),88-94.
MLA Xiao, Fuliang,et al."Bounce-averaged diffusion coefficients for superluminous wave modes in the magnetosphere".JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS 73.1(2011):88-94.

入库方式: OAI收割

来源:国家空间科学中心

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