日本地球惑星科学連合2025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-EM17] 宇宙プラズマ科学

2025年5月27日(火) 17:15 〜 19:15 ポスター会場 (幕張メッセ国際展示場 7・8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 〜 19:15

[PEM17-P04] ブラソフ方程式に対する高次重み付きPFC法

*簑島 敬1松本 洋介2 (1.海洋研究開発機構 数理科学・先端技術研究開発センター、2.千葉大学)

キーワード:ブラソフ方程式、移流方程式、高次精度スキーム、非線形スキーム

Kinetic plasma simulations are extensively utilized to investigate nonlinear physics in astrophysical, space, and laboratory plasma environments, including instabilities, wave-particle interactions, and particle acceleration. The Vlasov simulation is an Eulerian method that discretizes the distribution function to solve the Vlasov equation as an advection equation in phase space (Cheng and Knorr, 1976). While it can address numerical difficulties inherent in familiar Particle-In-Cell simulations and provide high-resolution solutions, its primary limitation is the substantial computational cost to allocate grid points in up to six-dimensional phase space, thereby necessitating high-order schemes for accurate solutions.

High-order Semi-Lagrangian methods for the advection equation are widely used in the Vlasov simulation (e.g., Sonnendrucker et al., 1999; Nakamura and Yabe, 1999). When employing high-order methods, nonlinear schemes are necessary to suppress numerical oscillations inherent in linear schemes. In Vlasov simulations, nonlinear schemes help to prevent the unphysical generation of plasma waves and negative densities in phase space. A drawback of using nonlinear schemes is the loss of accuracy, which can obscure physically meaningful profiles and degrade the conservation of energy and entropy.

In this paper, we introduce a new high-order semi-Lagrangian scheme that is conservative, positivity-preserving, and non-oscillatory, for solving the Vlasov equation. The scheme builds upon the third-order positive and flux conservative (PFC) method (Filbet et al., 2001), extending it to attain fifth-order accuracy. This is achieved by a convex combination of low-order polynomials in substencils, inspired by the weighted essentially non-oscillatory (WENO) scheme (Jiang and Shu, 1996). Unlike conventional WENO schemes, however, we utilize positive and non-oscillatory polynomials derived from the PFC method. This approach allows us to assign higher weights to substencils with larger L2 norm, enhancing resolution. An approximate dissipation relation indicates that the spectral properties of the new scheme outperform those of the underlying linear scheme, improving both accuracy and stability. We apply this scheme to the Vlasov simulation to evaluate its performance, demonstrating improved conservation of energy and entropy.