日本地球惑星科学連合2025年大会

講演情報

[E] ポスター発表

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-EM14] 太陽地球系結合過程の研究基盤形成

2025年5月28日(水) 17:15 〜 19:15 ポスター会場 (幕張メッセ国際展示場 7・8ホール)

コンビーナ:山本 衛(京都大学生存圏研究所)、小川 泰信(国立極地研究所)、野澤 悟徳(名古屋大学宇宙地球環境研究所)、吉川 顕正(九州大学大学院理学研究院地球惑星科学部門)

17:15 〜 19:15

[PEM14-P09] Statistical Studies of Large-scale Field-aligned Currents based on FY-3E Observations

*Jie Ren1、Qiugang Zong2、Yongfu Wang2、Xiangqian Yu2 (1.China University of Geosciences Beijing、2.Peking University)

キーワード:Field-aligned currents, Energetic electron boundary, Geomagnetic storm, Solar wind

Field-aligned currents (FACs) are the main agents for transporting energy and mass in the solar wind-magnetosphere-ionosphere coupling process. The recently launched FY-3E satellite in early morning orbit can provide the simultaneous and long-term measurements of magnetic fields and energetic electrons. It provides a good opportunity to investigate the distribution and variation of large-scale FACs in the dawnside and duskside of both hemispheres. Based on the statistical results with one and a half years of data, we find that the location of region 1 (R1) and region 2 (R2) currents is closely associated with the high-latitude energetic electron boundary, these FACs in the northern hemisphere are preferentially located in higher magnetic latitudes than in the southern hemisphere especially during geomagnetic quiet time, and the location of FACs has a larger equatorward motion than the electron boundary during active time. We have quantified the location and current intensity of FACs in different sectors of Earth's magnetosphere as a function of Kp index, Sym-H index and IMF Bz. Comparisons between different sectors also indicate that the current intensities of both R1 and R2 currents have a north-south asymmetry, and they are stronger in the dawnside northern hemisphere than other sectors.