日本地球惑星科学連合2021年大会

講演情報

[J] 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] 宇宙プラズマ理論・シミュレーション

2021年6月4日(金) 17:15 〜 18:30 Ch.05

コンビーナ:天野 孝伸(東京大学 地球惑星科学専攻)、三宅 洋平(神戸大学計算科学教育センター)、梅田 隆行(名古屋大学 宇宙地球環境研究所)、中村 匡(福井県立大学)

17:15 〜 18:30

[PEM15-P13] Identifying Terrestrial Magnetospheric Topology using Geodesic Level Set

*CAI DongSheng1 (1.University of Tsukuba)

キーワード:測地線レベルセット法、サドル結合トポロジー、地球磁場トポロジー

The present report introduces a numerical method to identify and visualize the geometrical structure of the earth magnetic field topology with a northward interplanetary magnetic field (IMF) from a 3D global MHD (Magneto-Hydro-Dynamic) simulation. The two-dimensional and one-dimensional stable or unstable manifolds, respectively, are generated from the critical points (CPs) or magnetic nulls obtained in the 3D MHD simulation data using Geodesic Level Set (GLS) method. The Boundary Value Problem (BVP) is solved numerically to forward the next geodesic level set from the current one. These geodesic level sets are placed on the magnetic manifold that determine the magnetic field topology. In the present paper, we introduce: (1) We implement an efficient bisection method applied to BVP to reduce the computation of integrations to avoid computing all subdivided trajectories decided by greater boundaries, which save computation time, significantly; (2) A necessary and reliable method to integrate the shorter trajectory with higher accuracy by a time-reversed 4th order Runge-Kuta method; and (3) a method to prevent the sharp folding angle generated by adjacent mesh that disrupts GLS algorithm. We visualize the separatrices that are the the two magnetic manifolds generated from two CPs or magnetic nulls, and the magnetic topology of the earth magnetosphere in the 3D global MHD simulation.