Whistler-mode waves trapped by density irregularities in the Earth's magnetosphere
编号:153 稿件编号:1473 访问权限:仅限参会人 更新:2021-06-14 09:06:18 浏览:632次 口头报告

报告开始:2021年07月10日 15:30 (Asia/Shanghai)

报告时间:15min

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
Whistler-mode waves are electromagnetic waves pervasively observed in the Earth's and other planetary magnetospheres. They are considered to be mainly responsible for producing the hazardous radiation and diffuse aurora, which heavily relies on their properties. Density irregularities, frequently observed in the Earth’s magnetospheres, are found to change largely the properties of whistler-mode waves. Here we report, using Van Allen Probes measurements, whistler-mode waves strongly modulated by two different density enhancements. With particle-in-cell simulations, we propose wave trapping caused by field-aligned density irregularities (ducts) may account for this phenomenon. Simulation results show that whistler-mode waves can be trapped inside the enhanced density ducts. These trapped waves remain quasi-parallel and usually get much larger amplitudes than those unducted whistler waves during propagation away from the magnetic equator, and tend to focus at a spatially narrow channel, consistent with observations. Our results imply density irregularities may be significant to modulate radiation-belt electrons.   
关键字
whistler-mode wave,density duct,Earth
报告人
柯阳光
中国科学技术大学

稿件作者
柯阳光 中国科学技术大学
高新亮 中国科学技术大学
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