日本地球惑星科学連合2021年大会

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[E] 口頭発表

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-EM09] Dynamics of Magnetosphere and Ionosphere

2021年6月6日(日) 10:45 〜 12:15 Ch.05 (Zoom会場05)

コンビーナ:藤本 晶子(九州工業大学)、尾崎 光紀(金沢大学理工研究域電子情報学系)、佐藤 由佳(日本工業大学)、中溝 葵(情報通信研究機構 電磁波研究所)、座長:長谷川 洋(宇宙航空研究開発機構宇宙科学研究所)、西野 真木(宇宙航空研究開発機構宇宙科学研究所)

11:55 〜 12:10

[PEM09-12] Dawn-dusk asymmetry in the mesoscale field-aligned currents embedded in the diminished large-scale Region 1 current

*横山 佳弘1、田口 聡1、家森 俊彦2 (1.京都大学大学院理学研究科地球惑星科学専攻地球物理学教室、2.京都大学)

キーワード:Swarm satellites、low-latitude boundary layer

Irregular magnetic perturbations embedded in the diminished large-scale Region 1 current are observed in almost all MLT except for the near noon region during prolonged northward IMF conditions. Our recent statistical study for the dusk side sector has revealed that the mesoscale field-aligned currents that produce these irregular magnetic perturbations tend to occur under the northward IMF conditions and are possibly generated in the low-latitude boundary layer. Our study has also shown that the current density of the mesoscale field-aligned currents tends to increase as the solar wind proton density increases. To clarify whether or not there exist asymmetries in the mesoscale field-aligned currents between the dawn and dusk sector, by utilizing magnetic data obtained by Swarm satellites during the period from May 2014 to May 2017, we investigated the dependence of the dawn side field-aligned currents on the solar zenith angle, the IMF, and solar wind plasma parameters, and compared the results with those from the dusk side sector. We found that the occurrence ratio of the mesoscale field-aligned current in the dawn sector also shows a strong dependence on the northward IMF condition. Besides, we found that there are weak dawn-dusk asymmetries in the occurrence ratio against the Y component of IMF, and in the current density. From our proposed mechanism of the generation for the mesoscale field-aligned currents, which is associated with the cold dense ion regions in the low-latitude boundary layer, we interpret those dawn-dusk asymmetries.