日本地球惑星科学連合2014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-EM32_2AM2] プラズマ宇宙:MHD現象,リコネクション,構造形成

2014年5月2日(金) 11:00 〜 12:45 503 (5F)

コンビーナ:*松清 修一(九州大学大学院総合理工学研究院流体環境理工学部門)、新田 伸也(筑波技術大学)、座長:星野 真弘(東京大学大学院理学系研究科)

12:30 〜 12:45

[PEM32-13] Analysis on turbulent reconnection of three-dimensional resistive MHD simulation

*WANG Shuoyang1YOKOYAMA Takaaki1ISOBE Hiroaki2 (1.The University of Tokyo、2.Kyoto University)

This study starts from a three-dimensional current sheet with random perturbation on velocity, in order to understand more on the 3D reconnection in a more general way.Due to the periodic boundary condition, the core of current sheet quickly develops a resonance netlike pattern under tearing instability. Small reconnection site mainly form two chains on either side of the current sheet center and constitute a zigzag arrangement. The outflow from one reconnection site is fed into the counterpart on the other side thus composes a positive feedback system resembles even double tearing mode. As the inflow being enhanced, slow-mode shocks are identified along the current sheet. The conversion of the magnetic energy is further raised. Total kinetic energy of the current sheet presents 4 steps of development while first 3 exhibit linear growing tendency. At the same time, reconnection rate increases by 5 times compared with the early phase. Thus we have achieved faster reconnection without localized resistivity in a more universal idea.