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Magnetospheric chorus wave instability induced by relativistic Kappa-type distributions

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成果类型:
期刊论文
作者:
Yang QiWu;Yang Chang;He YiHua;Liu Si;Zhou QingHua;...
通讯作者:
Xiao FuLiang
作者机构:
[Xiao FuLiang; Yang QiWu; Yang Chang; Liu Si; Zhou QingHua; He YiHua] Changsha Univ Sci & Technol, Sch Phys & Elect Sci, Changsha 410004, Hunan, Peoples R China.
通讯机构:
[Xiao FuLiang] C
Changsha Univ Sci & Technol, Sch Phys & Elect Sci, Changsha 410004, Hunan, Peoples R China.
语种:
英文
关键词:
Kappa-type distribution;energetic electrons;wave-particle interaction;chorus wave instability
期刊:
中国科学:技术科学(英文版)
ISSN:
1674-7321
年:
2016
卷:
59
期:
11
页码:
1739-1745
基金类别:
National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC) [41531072, 41274165, 41404130, 41204114, 41504125]
机构署名:
本校为第一且通讯机构
院系归属:
物理与电子科学学院
摘要:
We study the field-aligned propagating magnetospheric chorus wave instability using a fully relativistic wave growth formula, the previously developed relativistic Kappa-type (KT) distribution and the regular Kappa distribution of energetic electrons. We demonstrate that the peak growth rate using the nonrelativistic Kappa simulation is higher than that using either the relativistic KT or the Kappa simulation at/above 100 keV, because the significant relativistic effect yields a reduction in the relativistic anisotropy. The relativistic anisotr...

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