Butterfly distributions of energetic electrons driven by ducted and nonducted chorus waves
ID:3367 View Protection:ATTENDEE Updated Time:2024-04-13 15:18:43 Hits:1885 Invited speech

Start Time:2024-05-19 14:25(Asia/Shanghai)

Duration:10min

Session:S10 主题10、行星科学与空间物理 » S10-3主题10、行星科学与空间物理 专题10.8、专题10.9、专题10.12、专题10.13、专题10.14(19日下午,307)

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Abstract
Bursts of electron butterfly distributions at 10s keV correlated with chorus waves are frequently observed in the Earth’s magnetosphere. Strictly ducted (parallel) upper-band chorus waves are proposed to cause them by nonlinear cyclotron trapping. However, chorus waves in these events are probably nonducted or not strictly ducted. In this study, test-particle simulations are conducted to investigate electron scattering driven by ducted (quasi-parallel) and nonducted upper-band chorus waves. Simulation results show butterfly distributions of 10s keV electrons can be created by both ducted and nonducted upper-band chorus waves in seconds. Ducted upper-band chorus waves cause these butterfly distributions mainly by accelerating electrons due to cyclotron phase trapping. However, nonducted waves tend to decelerate electrons to form these butterfly distributions via cyclotron phase bunching. Our study provides new insights into the formation mechanisms of electron butterfly distributions and demonstrates the importance of nonlinear interactions in the Earth’s magnetosphere.
 
Keywords
chorus wave,simulation,nonlinear interaction,electron butterfly distribution
Speaker
柯阳光
副研究员 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
陆全明 中国科学技术大学
汪学毅 奥本大学
陈瑞 中国科学技术大学
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    May 17

    2024

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    May 20

    2024

  • Mar 31 2024

    Draft paper submission deadline

  • Mar 31 2024

    Contribution Submission Deadline

  • May 20 2024

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青年地学论坛理事会
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厦门大学近海海洋环境科学国家重点实验室
中国科学院城市环境研究所
自然资源部第三海洋研究所
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