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The characteristics of chorus waves in the Earth’s inner magnetosphere: the perspective of Gendrin angle
AGU 2024
spa-magnetospheric physics | 13 december 2024
Yun Yan, Chao Yue, Li Li, Qianli Ma, Yoshiharu Omu...
Chorus waves are important for the acceleration and loss processes of radiation belt electrons, and wave normal angle (θ) is an important factor that ...
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Statistical characteristics of the field-aligned currents using AMPERE data
AGU 2024
spa-aeronomy | 12 december 2024
Haobo Fu, Chao Yue, Qiugang Zong, Xuzhi Zhou, Shan...
Field-aligned current (FAC) is a crucial link in the ionosphere and magnetosphere interaction. We used the AMPERE data from 2010 to 2017 to conduct a ...
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Dynamics of Sputtered Neutral Sodium Atoms in the Near-Mercury Space
AGU 2024
spa-magnetospheric physics | 12 december 2024
Jiutong Zhao, Qiugang Zong, Weijie Sun, Xuzhi Zhou...
The solar wind sputtering in the magnetospheric polar cusp is an important source of heavy atoms in Mercurys exosphere and magnetosphere. However, the...
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The Spatio-temporal Variations of Ring Current Ions during Geomagnetic Storms in the Inner Magnetosphere
AGU 2024
spa-magnetospheric physics | 12 december 2024
Yuxuan Li, Chao Yue, Qiugang Zong, Xuzhi Zhou, Sha...
The geomagnetic storm is an intense geomagnetic activity and is closely associated with the ring current particles. In this study, we focus on the rin...
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Observations of cross-scale wave-particle energy transfer in space plasmas
AGU 2024
spa-magnetospheric physics | 10 december 2024
Xuzhi Zhou, jinghuan li, Zhiyang Liu, Shan Wang, Y...
The collisionless plasmas in space and astrophysical environments are intrinsically multiscale in nature, behaving as conducting fluids at macroscales...
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A statistical examination of ion dynamics at 1-Hz whistler waves in the Earth’s foreshock
AGU 2024
spa-solar and heliospheric physics | 10 december 2024
Shan Wang, jinghuan li, Li Li, Xuzhi Zhou, Yoshiha...
The 1-Hz whistler wave precursor attached to shock-like structures are often observed in foreshock. Using observations from the Magnetospheric Multisc...
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Storm-time ring current plasma pressure prediction based on the multi-output convolutional neural network model
AGU 2024
spa-magnetospheric physics | 09 december 2024
Chao Yue, Yun Yan
The terrestrial ring current consists of particles with energy from several keV to 100 s of keV, and its enhancement will result in the depression of ...
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The Excitation of Second Harmonic Poloidal ULF Waves Through Drift‐Bounce Resonance With Protons in the Magnetic Dip
JOURNAL OF GEOPHYSICAL RESEARCH: SPACE PHYSICS
21 november 2024
Yan Zhuang, Haobo Fu, Li Li, Xingyu Li, Ying Liu, ...
The drift‐bounce resonance between ultralow‐frequency (ULF) waves and charged particles is an efficient way to transfer energy. In this...