日本地球惑星科学連合2024年大会

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[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-EM17] 宇宙プラズマ科学

2024年5月30日(木) 17:15 〜 18:45 ポスター会場 (幕張メッセ国際展示場 6ホール)

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)、諌山 翔伍(九州大学総合理工学研究院)、梅田 隆行(北海道大学 情報基盤センター)

17:15 〜 18:45

[PEM17-P07] An implicit-explicit Runge-Kutta scheme strictly satisfying Gauss’s Laws for the full two-fluid plasma model

*エマヤ ヨナ1三好 隆博2 (1.総合研究大学院大学、2.広島大学大学院先進理工系科学研究科)

キーワード:完全二流体プラズマモデル、離散的ガウスの法則、スタッガード格子、陰陽的ルンゲ=クッタ法

We present a new numerical scheme for the full-two fluid plasma model, which couples the Euler Equations for ion and electron fluids with Maxwell’s Equations to account for electromagnetic interactions. The fluid equations are solved with the HLLC approximate Riemann solver [1], while the electric and magnetic fields are arranged in a staggered grid [2] and calculated with a central differencing scheme. By using different spatial discretization, we ensure that the discrete Gauss’s laws are conserved over time and therefore the divergence constraints of the Maxwell equations will be satisfied permanently, given that the initial conditions do so. Therefore, our model can calculate even very small polarization electric fields with high accuracy. We present algorithms for both explicit and implicit-explicit temporal integration using Runge-Kutta methods [3]. By calculating the stiff source term implicitly, we aim to exclude rapid oscillations, that happen on a time scale irrelevant to the problem which is to be solved. The implicit-explicit scheme does not require iteration to converge and is significantly more robust than the solely explicit scheme. Finally, we validate our scheme by performing several standard numerical experiments, such as the electron plasma oscillation and the Brio-Wu shock tube.

References
[1] Batten et al., SIAM J. Sci. Statist. Comput. 18, 1553-1570, 1997.
[2] Yee, IEEE Trans. Antennas Propag. 14, 302-307, 1966.
[3] Ascher, Ruuth, and Spiteri, Appl. Numer. Math., 25 (2–3), 151–167, 1997.