日本地球惑星科学連合2021年大会

講演情報

[E] 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-EM09] Dynamics of Magnetosphere and Ionosphere

2021年6月6日(日) 17:15 〜 18:30 Ch.05

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

17:15 〜 18:30

[PEM09-P20] SuperDARNレーダーで観測されたMHD波動のLomb-Scargle解析によるモード特定

*森田 洸生1、西谷 望1、堀 智昭1 (1.名古屋大学宇宙地球環境研究所)

キーワード:磁気流体波動、Pc5、トロイダル、ポロイダル

Ultralow frequency (ULF) waves are magnetohydrodynamic plasma waves. The ULF waves in the ionospheric plasma motion obtained by the Super Dual Auroral Radar Network (SuperDARN) can be categorized into toroidal and poloidal modes. Since different oscillation modes come from different generation mechanisms, the identification of the mode as a function of geomagnetic latitude (MLAT) and magnetic local time (MLT) might provide clues to the generation mechanisms of ULF waves. We analyzed Pc5 oscillation modes in ULF waves using the SuperDARN Hokkaido East high-frequency radar data. First, we applied the Lomb-Scargle frequency analysis method to the Doppler shifts of ionospheric irregularities obtained from the radar and identified Pc5 oscillation modes by comparing the Doppler velocity amplitude at one geomagnetic latitude with different beam directions. Next, we conducted statistical analysis on Pc5 oscillation modes in order to reveal the MLAT and MLT dependence of the dominant mode. As a result of the initial statistical analysis from Jan. 10 to Feb. 14 in 2008, we find the following characteristics: 1. The occurrence probability of the Pc5 oscillation is the highest at 0 to 1 MLT. 2. The Pc5 oscillation mode was poloidal at 51° to 52° MLAT and toroidal at 48° to 51° MLAT. The former result is explained by the difference in electrical conductivity between day and night. The latter result is interpreted in terms of the external oscillation propagating from higher magnetic latitudes and mode-converted to toroidal mode magnetic field line resonance.