Interplanetary shock induced intensification of electron cyclotron harmonic waves in the Earth's inner magnetosphere

被引:0
作者
Xie, Yi [1 ,2 ]
Liu, Nigang [1 ,2 ]
Su, Zhenpeng [3 ,4 ,5 ]
Yi, Siyang [1 ,2 ]
He, Zhaoguo [1 ,2 ]
Yu, Jiang [1 ,2 ]
Li, Kun [1 ,2 ]
Chen, Zuzheng [1 ,2 ]
Cui, Jun [1 ,2 ]
机构
[1] Sun Yat Sen Univ, Sch Atmospher Sci, Planetary Environm & Astrobiol Res Lab PEARL, Zhuhai, Peoples R China
[2] Sun Yat Sen Univ, Key Lab Trop Atmosphere Ocean Syst, Minist Educ, Zhuhai, Peoples R China
[3] Univ Sci & Technol China, CAS Ctr Excellence Comparat Planetol, CAS Key Lab Geospace Environm, Mengcheng Natl Geophys Observ, Hefei, Peoples R China
[4] Univ Sci & Technol China, Sch Earth & Space Sci, Deep Space Explorat Lab, Hefei, Peoples R China
[5] Collaborat Innovat Ctr Astronaut Sci & Technol, Hefei, Peoples R China
基金
中国国家自然科学基金;
关键词
interplanetary shock; electron cyclotron harmonic wave; solar wind-magnetosphere-ionosphere coupling; inner magnetosphere; plasma wave instability; MAGNETIC-FIELD; SOLAR-WIND; ENERGETIC PARTICLE; PLASMASPHERIC HISS; PLASMA; DIFFUSION; DISCONTINUITIES; DISAPPEARANCE; GENERATION; STEADY;
D O I
10.3389/fphy.2024.1334531
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Electron cyclotron harmonic (ECH) waves are electrostatic emissions frequently observed in the Earth's magnetosphere. By precipitating magnetospheric hot electrons into the ionosphere, ECH waves play a critical role in the formation of diffuse aurora. Previous research has extensively investigated the strong dependence of ECH waves on the geomagnetic activities. In this study, we present the first report of the prompt response of ECH waves to an interplanetary shock on the basis of WIND and Van Allen Probes observations. Our observations and analyses demonstrate that the interplanetary shock compression can increase > 0.1 keV hot electron fluxes in the dayside inner magnetosphere, consequently leading to the prompt intensification of ECH waves by promoting the wave instability. These findings expand our comprehension of the impacts of solar wind disturbances on magnetospheric plasma waves and offer fresh insights into solar wind-magnetosphere-ionosphere coupling.
引用
收藏
页数:11
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