Surfing Acceleration of Radiation Belt Relativistic Electrons Induced by the Propagation of Interplanetary Shock
ID:3364 View Protection:ATTENDEE Updated Time:2024-04-13 13:59:15 Hits:1816 Oral Presentation

Start Time:2024-05-19 16:10(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
Interplanetary shocks (IPS) can initiate prompt acceleration of relativistic electrons in the Earth’s radiation belt, which is related to the generation and propagation of impulsive electric field (IEF). We investigate the effect of IEF on accelerating radiation belt electrons in the 6 September 2017 IPS event. A ‘surfing’ effect of electrons with respect to the electric field, referring to electrons that drift together with the tailward-propagating IEF in the duskside, is investigated in this study. Our results show that the maximum increase of electron differential flux is at 3.4 MeV by a factor of 2.2, corresponding to a drift velocity of 531 km/s, which is more consistent with the IPS propagating speed of 621 km/s rather than the fast-mode speed of 1074 km/s. We suggest that the effect of IPS propagation is important for radiation belt dynamics, and we highlight the potential importance of the parameter of IPS propagation speed.
Keywords
外辐射带,行星际激波,地球磁层
Speaker
张典钧
讲师 北京航空航天大学

Submission Author
张典钧 北京航空航天大学
刘文龙 北京航空航天大学
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    May 17

    2024

    to

    May 20

    2024

  • Mar 31 2024

    Draft paper submission deadline

  • Mar 31 2024

    Contribution Submission Deadline

  • May 20 2024

    Registration deadline

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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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