日本地球惑星科学連合2023年大会

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[J] オンラインポスター発表

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-EM17] 宇宙プラズマ理論・シミュレーション

2023年5月23日(火) 09:00 〜 10:30 オンラインポスターZoom会場 (2) (オンラインポスター)

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(神戸大学大学院システム情報学研究科)、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)

現地ポスター発表開催日時 (2023/5/22 17:15-18:45)

09:00 〜 10:30

[PEM17-P02] 相対論的運動方程式の高次精度数値解析手法の研究

*尾崎 理玖1、梅田 隆行1、三好 由純1 (1.名古屋大学宇宙地球研究所)

The purpose of this study is to improve the accuracy of a numerical method for integrating the relativistic equation of motion for charged particles. The Runge-Kutta integrator (RK4) is a classical method for numerically solving various difference equations. Although RK4 has a fourth-order accuracy in time, RK4 does not satisfy the conservation laws in the relativistic motion of charged particles. The Boris integrator [Boris,1970], which has the second-order accuracy in time, has been used conventionally due to the following reasons. The Boris integrator is time-reversible, is simple for implementing to numerical code, and satisfies the energy conservation law during the gyration of charged particles. However, it has been known that the Boris integrator does not give the exact relativistic motion of charged particles for a large Lorentz factor. Recently, a new integrator has been developed based on the theoretical solution to the relativistic equation of motion for charged particles, which is called as the Umeda integrator [Umeda, 2023]. The Umeda integrator is an improved version of the Boris integrator, which satisfies several conservation laws and gives the exact relativistic E-cross-B drift velocity. However, the Umeda integrator has the second-order accuracy in time and is less accurate than RK4. In the present study, we improve the accuracy of the Umeda integrator with multi-step techniques. First, the Umeda integrator is combined with the Euler method, the midpoint rule, the trapezoidal rule, the Heun method, and RK4. Second, the Taylor series expansion of the relativistic gyration angle is performed, and higher-degree terms are included. It is demonstrated that the order of the numerical accuracy with the Euler method, the midpoint rule, and the trapezoidal rule is second-order in time. However, the order of the numerical accuracy with the Heun method and RK4 are improved against the Umeda integrator.