日本地球惑星科学連合2025年大会

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セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM12] Coupling Processes in the Atmosphere-Ionosphere System

2025年5月26日(月) 15:30 〜 17:00 303 (幕張メッセ国際会議場)

コンビーナ:細川 敬祐(電気通信大学大学院情報理工学研究科)、Liu Huixin(九州大学理学研究院地球惑星科学専攻 九州大学宙空環境研究センター)、大塚 雄一(名古屋大学宇宙地球環境研究所)、Chang Loren(Institute of Space Science, National Central University)、座長:西山 尚典(国立極地研究所)、Yang-Yi Sun(China University of Geosciences)


15:30 〜 15:45

[PEM12-37] Ionospheric response to the competition between penetration electric field and thermospheric O/N2

★Invited Papers

*Yongliang Zhang1 (1.Johns Hopkins University Applied Physics Laboratory)

キーワード:Thermosphere composition (O/N2 ratio), Topside ionosphere, Penetration electric field, Thermospheric FUV emission, geomagentic storm, interplanetary electric field

We revisited the November 2004 superstorm by analyzing TIMED/GUVI data which provide information of both thermosphere and ionosphere. When an intense eastward Interplanetary
Electric Field (IEF) or Penetration Electric Field (PEF) occurred,
the dayside equatorial arcs were enhanced and their latitude separation increased.
The enhanced equatorial arcs were hemispherically symmetric or asymmetric in the region with non-depleted O/
N2 or hemispherically asymmetric O/N2 depletion, respectively. When O/N2 depletion reached the magnetic
equator, there was no observable enhancement in the equatorial arcs regardless the IEF or PEF conditions, indicating O/N2 condition significantly modulated the variations in storm-time equatorial arcs. GUVI observations also showed that a westward IEF (PEF) and/or disturbance dynamo electric field could also suppress the dayside equatorial arcs.