Electron diffusion by chorus waves: effects of latitude-dependent wave power spectrum

被引:1
|
作者
Yu, Jiang [1 ]
Wang, Jing [1 ]
He, Zhaoguo [1 ,2 ,3 ]
Chen, Zuzheng [1 ]
Li, Liuyuan [4 ]
Cui, Jun [1 ,3 ]
Cao, Jinbin [4 ]
机构
[1] Sun Yat Sen Univ, Sch Atmospher Sci, Planetary Environm & Astrobiol Res Lab PEARL, Zhuhai, Peoples R China
[2] Macau Univ Sci & Technol, State Key Lab Lunar & Planetary Sci, Macau, Peoples R China
[3] Chinese Acad Sci, Ctr Excellence Comparat Planetol, Hefei, Peoples R China
[4] Beihang Univ, Sch Space & Environm, Beijing, Peoples R China
基金
中国国家自然科学基金;
关键词
Earth's inner magnetosphere; radiation belt; wave-particle interactions; chorus waves; electron diffusions; WHISTLER-MODE WAVES; VAN ALLEN PROBES; RADIATION-BELT; ACCELERATION; PLASMASPHERE; SCATTERING; DRIVEN; FLUXES;
D O I
10.3389/fspas.2023.1333184
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In the present paper, we investigate the effects of latitude-dependent wave power spectrum on the interactions of chorus with electrons. Great errors in evaluating the electron diffusion coefficients and the resultant electron temporal evolutions are introduced by the widely adopted latitudinally constant model, compared with the latitudinally varying model. The latitudinally constant model tends to overestimate (underestimate) the diffusion coefficients for electrons below (above) 200 keV. The overestimation and underestimation are mainly confined in small to intermediate pitch angles, increase with decreasing pitch angles, and can reach up to several orders of magnitude. The large differences in diffusion coefficients significantly alter the net changes of electron phase space densities and the resultant shapes of electron pitch angle distributions. Our simulations demonstrate that the wave power spectrum distribution along the magnetic field line plays an important role in controlling the dynamics of radiation belt electrons.
引用
收藏
页数:9
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