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-EM15] Dynamics of Magnetosphere and Ionosphere

2025年5月29日(木) 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:今城 峻(京都大学大学院理学研究科附属地磁気世界資料解析センター)、佐藤 由佳(日本工業大学)、藤本 晶子(九州工業大学)、山本 和弘(名古屋大学宇宙地球環境研究所)


17:15 〜 19:15

[PEM15-P07] 惑星間空磁場朝夕成分卓越時の昼間側4層沿磁力線電流系を再現する磁気流体シミュレーション

*渡辺 正和1田中 高史2藤田 茂3 (1.九州大学大学院理学研究院、2.九州大学 国際宇宙惑星環境研究センター、3.情報・システム研究機構 統計数理研究所)

キーワード:沿磁力線電流、4層構造、惑星間空間磁場BY、MHDシミュレーション

When the dawn-dusk component of the interplanetary magnetic field (IMF BY) is dominant, in particular, for northward IMF, there often appears a field-aligned current (FAC) system consisting of four longitudinally elongated current sheets in the prenoon or postnoon sector of the ionosphere, depending on the polarity of IMF BY. It has been suggested that while the equatorward two sheets are the dayside extension of the ordinary region 1 and region 2 currents, the poleward two sheets are the “cusp” and “mantle” currents on open field lines that are controlled by the IMF BY. Although the morphology of the dayside FAC systems including the four-sheet current system is well established, their generation mechanisms are still within the realm of imagination. Very recently, we have been successful in reproducing the four-sheet current system using the high spatial resolution version of the Reproduce Plasma Universe (REPPU) code which solves magnetohydrodynamic equations in the magnetosphere and the ionosphere self-consistently. The simulation run was performed under southward IMF conditions with a clock angle of 120 degrees. To the best of our knowledge, this is the first successful numerical modeling of the four-sheet FAC system. We believe that high resolution in the ionosphere (about 0.6 degrees in arc length) contributed significantly to the successful reproduction. We now plan another simulation run under northward IMF conditions for which the four-sheet structure is expected to appear more distinctively. We report in the presentation the initial results of our analysis. In addition, we discuss the generation mechanisms of the four-sheet current system. Previously, Watanabe and Sofko (2009) proposed a scenario in which lobe-to-closed interchange reconnection that modifys the Dungey cycle plays a central role in producing the four-sheet structure. From our preliminary analysis, the reproduced four-sheet FAC system seems consistent with this scenario.