Whistler-mode waves trapped by density irregularities in the Earth's magnetosphere
ID:153 View Protection:ATTENDEE Updated Time:2021-06-14 09:06:18 Hits:2001 Oral Presentation

Start Time:2021-07-10 15:30(Asia/Shanghai)

Duration:15min

Session:S9B 9B、行星科学与空间物理 » S9B-19B、行星科学与空间物理-1

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Abstract
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.   
Keywords
whistler-mode wave,density duct,Earth
Speaker
柯阳光
中国科学技术大学

Submission Author
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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    Jul 09

    2021

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    Jul 11

    2021

  • May 30 2021

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  • May 30 2021

    Draft paper submission deadline

  • May 30 2021

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  • Jul 10 2021

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  • Jul 11 2021

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Sponsored By
青年地学论坛理事会
Organized By
中国科学院地球化学研究所
贵州大学
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