JpGU-AGU Joint Meeting 2020

講演情報

[E] 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-EM13] Dynamics of Magnetosphere and Ionosphere

コンビーナ:中溝 葵(情報通信研究機構 電磁波研究所)、尾崎 光紀(金沢大学理工研究域電子情報学系)、藤本 晶子(九州工業大学)、佐藤 由佳(日本工業大学)

[PEM13-22] Feedback instability theory extended to the magnetosphere-ionosphere coupling with field-aligned inhomogeneity

*渡邉 智彦1樋渡 淳也1前山 伸也1 (1.名古屋大学大学院理学研究科)

キーワード:フィードバック不安定性、アルヴェン波、磁気圏-電離圏結合

The feedback instability theory for Alfvenic coupling of the magnetosphere and the ionosphere has been extended by introducing inhomogeneous profiles of the ionospheric collision frequency and the magnetospheric Alfven speed. The eigenvalue analysis clarifies the stabilizing mechanism of high frequency components of the ionospheric Alfven resonator (IAR) mode for the strongly inhomogeneous collision frequency profile in the ionosphere. The stabilization is brought by an effective internal resistivity due to the ionospheric inhomogeneity, not by a shear of the ionospheric current. Low frequency components of the field line resonance (FLR) mode remain unstable even when the high frequency components are stabilized. The theoretical results demonstrate a robustness of the feedback instability mechanism providing spontaneous growth of the auroral arc structure in the magnetosphere-ionosphere coupling.