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-P10] Beam or temperature anisotropy instabilities in unmagnetized plasma

*yumeng fan1松清 修一1 (1.九州大学)

キーワード:ワイベル不安定性、異方的分布関数 、PICシミュレーション

Both Weibel (1959) and Fried (1959) demonstrated that an anisotropic distribution function can lead to a purely growing electromagnetic instability, commonly referred to as the Weibel instability. This instability arises because the Lorentz force from a perturbed magnetic field induces a current that amplifies the perturbation, resulting in spontaneous growth. Traditionally, the Weibel instability has been attributed to macroscopic temperature anisotropy. However, recent studies suggest that its properties depend not only on temperature anisotropy but also on the specific form of the distribution function. For example, Silva (2021) showed that different distribution functions with the same temperature anisotropy can produce varying growth rates and wavevector directions. Similarly, Zaheer (2007) compared Maxwellian, kappa, and generalized (r, q) distribution functions with the same effective temperature, demonstrating that the instability characteristics are highly sensitive to the particular form of the distribution function. In this study, we will discuss the detailed properties of these instabilities in unmagnetized plasmas.