Japan Geoscience Union Meeting 2023

Presentation information

[J] Online Poster

P (Space and Planetary Sciences ) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM17] Space Plasma Physics: Theory and Simulation

Tue. May 23, 2023 9:00 AM - 10:30 AM Online Poster Zoom Room (2) (Online Poster)

convener:Takanobu Amano(Department of Earth and Planetary Science, University of Tokyo), Yohei Miyake(Graduate School of System Informatics, Kobe University), Takayuki Umeda(Institute for Space-Earth Environmental Research, Nagoya University), Tadas Nakamura(Fukui Prefectural University)

On-site poster schedule(2023/5/22 17:15-18:45)

9:00 AM - 10:30 AM

[PEM17-P01] Reduction of Anisotropy in Numerical Dispersion of the Explicit Finite-Difference Time-Domain Method with Laplacian operator

*Harune Sekido1,2, Takayuki Umeda2, Yoshizumi Miyoshi2 (1.Graduate School of Engineering, Nagoya University, 2.Institute for Space-Earth Environmental Research, Nagoya University)


Keywords:FDTD, Courant condition, dispersion relation, phase velocity, Laplacian, anisotropy

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.