日本地球惑星科学連合2023年大会

講演情報

[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-P01] ラプラシアン演算子を用いた陽的FDTD法の分散関係の異方性の低減

*関戸 晴宇1,2梅田 隆行2三好 由純2 (1.名古屋大学工学研究科、2.名古屋大学宇宙地球環境研究所)


キーワード:FDTD、クーラン条件、分散関係、位相速度、ラプラシアン、異方性

The Finite-Difference Time-Domain (FDTD) method is a numerical method for solving the time development of electromagnetic fields (Yee 1966). The time-development equations used in the FDTD method is obtained by approximating Maxwell's equations with the finite difference of second-order accuracy in both time and space. A staggered grid (Yee grid) system is used in the spatial differences so that Gauss's law for both electric and magnetic fields is always satisfied. However, the FDTD method has a disadvantage that numerical oscillations occur in discontinuous waveforms and even in continuous waveforms with a large slope. Higher-order finite differences reduce the numerical error in the phase velocity. The FDTD(2,4) method uses the fourth-order spatial difference (Fang 1989, Petropoulos 1994). The numerical phase velocity error of FDTD(2,4) is smaller than that of FDTD(2,2). However, the Courant condition of FDTD(2,4) method is more restricted than that of FDTD(2,2). In general, higher-order finite differences in space with the second-order finite difference in time make the Courant condition more restrictive, which requires smaller Δt and larger number of time steps. Recently, FDTD methods which relaxes the Courant condition has been developed (Sekido 2023). The time-development equations of these method are derived by adding third- and fifth-degree difference terms with coefficients to these of FDTD(2,4) and FDTD(2,6). However, there exists an anisotropy in the numerical dispersion, which results in numerical oscillations. In the present study, a new explicit and non-dissipative FDTD method in two and three dimensions is proposed for reduction of anisotropy in numerical dispersion and relaxation of the Courant condition. By adding the third-degree spatial difference terms including Laplacian with coefficients to the time-development equations of FDTD(2,4), a new schemes are developed. Optimal coefficients are obtained by a brute-force search of the dispersion relations, which reduces phase velocity errors averaged over the entire wavenumber space but satisfies the numerical stability as well. The new scheme is stable with large Courant numbers up to C = 1. The new scheme also has smaller numerical errors in the phase velocity than conventional FDTD methods.