日本地球惑星科学連合2024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-EM15] 太陽地球系結合過程の研究基盤形成

2024年5月29日(水) 17:15 〜 18:45 ポスター会場 (幕張メッセ国際展示場 6ホール)

コンビーナ:山本 衛(京都大学生存圏研究所)、小川 泰信(国立極地研究所)、野澤 悟徳(名古屋大学宇宙地球環境研究所)、吉川 顕正(九州大学大学院理学研究院地球惑星科学部門)

17:15 〜 18:45

[PEM15-P05] Study of ionospheric E-F region coupling by the long-term MU radar observation

*横山 竜宏1、森下 怜依1山本 衛1 (1.京都大学生存圏研究所)

キーワード:MUレーダー、沿磁力線イレギュラリティ、E-F領域結合

Field Aligned Irregularities(FAI) is one of the plasma instability phenomena that occur in the ionospheric E and F regions. It is a phenomenon in which plasma density perturbation grows in the direction perpendicular to the magnetic field lines. The MU radar, a large atmospheric radar, has been used to observe FAI for several decades. By pointing the radar beam in the direction orthogonal to the magnetic field lines, coherent backscatter echoes can be received. In this study, we performed a statistical analysis of the long-term FAI observations by the MU radar from 1986 to 2013.
The simultaneous observations show that the occurrence of F-region FAI was preceded by E-region FAI in the most cases, although there were some cases where F-region FAI preceded. This result is consistent with the E-F region coupling theory, in which the electric field in the E region strengthens the instability growth in the F region. In addition, we used GPS-TEC data to survey the correlation between the occurrence of FAI and the occurrence of MSTID. As a result, among 70 days when FAI echoes were observed in both the E and F regions, MSTID was also observed on 69 days. This suggests that the coupling process is also important for MSTID generation as well as F-region FAI, which is also consistent with previous studies.