日本地球惑星科学連合2024年大会

講演情報

[J] 口頭発表

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) 15:30 〜 16:30 101 (幕張メッセ国際会議場)

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)、座長:松本 洋介(千葉大学国際高等研究基幹)、三宅 洋平(神戸大学大学院システム情報学研究科)

15:45 〜 16:00

[PEM17-08] ジャイロ運動論的シミュレーションコードGKVの双極子磁場配位への適用

*渡邉 智彦1藤田 慶二1 (1.名古屋大学大学院理学研究科)

キーワード:シミュレーション、磁気圏、ジャイロ運動論

Gyrokinetic simulations have widely been applied to study of turbulent transport in magnetic fusion plasmas, revealing a variety of transport phenomena related to drift wave turbulence and zonal flows. The gyrokinetic code GKV [1] is now utilized to explore the Alfvenic magnetosphere-ionosphere coupling and the auroral dynamics including the electron acceleration process for a slab configuration with straight field lines [2].
While the GKV code is applicable to various magnetic field geometries, such as toroidal (tokamak and helical systems) and ring dipole configurations, application to the dipole field has not been fully tested. Extension of the GKV code to the dipole geometry, self-consistently including kinetic effects and wave-particle interactions, should have an impact on studies of ULF waves, auroral dynamics, physics of radiation belt, and so on.
In this study, we have introduced the dipole configuration in the local flux tube limit and have carried out benchmark tests on a drift wave instability. Numerical difficulties in application to the dipole geometry and possible extensions of the code will also be discussed.

[1] T.-H. Watanabe and H. Sugama, Nuclear Fusion 46, 24 (2006).
[2] K. Fujita and T.-H. Watanabe in this meeting.