High-Frequency Electrostatic Waves Driven by Electron Crescents near Electron Diffusion Regions: A Review
编号:159 稿件编号:1203 访问权限:仅限参会人 更新:2021-06-14 09:29:25 浏览:679次 特邀报告

报告开始:2021年07月10日 16:15 (Asia/Shanghai)

报告时间:20min

所在会议:[S9B] 9B、行星科学与空间物理 » [S9B-1] 9B、行星科学与空间物理-1

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摘要
Magnetic reconnection is a fundamental and universal process, which transfers energy stored in the magnetic field to kinetic and thermal energies of charged particles. NASA’s Magnetospheric Multiscale (MMS) mission was designed to investigate the electron diffusion region (EDR), which is the core region of the reconnection where the magnetic field lines break and reconnect. Various types of plasma waves have been reported in and near EDRs. Recent studies reveal that only two types of high-frequency electrostatic waves (upper-hybrid waves and electron Bernstein waves) are driven by the crescent-shaped agyrotropic electron distribution functions in the EDRs. The kinetic interaction between the electrons and the large-amplitude electrostatic waves can thermalize electrons and change the electron pressure tensor. Therefore, those electrostatic waves may modify the reconnection electric field and have feedback on the reconnection process.
关键字
electrostatic waves,electron crescents,MMS,magnetic reconnection
报告人
李文亚
中国科学院国家空间科学中心

稿件作者
李文亚 中国科学院国家空间科学中心
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