The polar ionospheric and thermospheric response of space hurricane
ID:357 View Protection:ATTENDEE Updated Time:2024-04-10 19:15:07 Hits:1965 Invited speech

Start Time:2024-05-18 13:45(Asia/Shanghai)

Duration:15min

Session:S10 主题10、行星科学与空间物理 » S10-1主题10、行星科学与空间物理 专题10.10、专题10.11(18日下午,4F国际会议厅)

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Abstract
The space hurricane is a three-dimensional magnetic vortex structure with strong flow shears and electron precipitation in the polar cap. This study investigates for the first time how a space hurricane disturbs the polar thermosphere. During the formation and development of the space hurricane, the directional reversal of the horizontal neutral wind and the plasma convection will both be relocated from the poleward auroral oval boundary to the edge of the space hurricane, but the neutral wind responds slower compared to the plasma convection. Strong flow shears in the space hurricane causes enhanced Joule heating in the polar cap, which heats the thermosphere and triggers Atmospheric Gravity Waves (AGWs). Statistical results reveal that significant AGWs mainly are located on the dawnside of the space hurricane, suggesting that the space hurricane plays a significant role in ion-neutral coupling and generation of polar cap AGWs.
 
Keywords
Polar ionosphere,space
Speaker
马羽璋
Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, Institute of Space Sciences, Shandong University, Weihai, Shandong, China

Submission Author
马羽璋 Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, Institute of Space Sciences, Shandong University, Weihai, Shandong, China
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    May 17

    2024

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    May 20

    2024

  • Mar 31 2024

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  • Mar 31 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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