日本地球惑星科学連合2025年大会

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-EM14] 太陽地球系結合過程の研究基盤形成

2025年5月28日(水) 13:45 〜 15:15 303 (幕張メッセ国際会議場)

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)、座長:野澤 悟徳(名古屋大学宇宙地球環境研究所)、山本 衛(京都大学生存圏研究所)

14:45 〜 15:00

[PEM14-17] Structures of ionospheric disturbances by using improved GNSS-based 3-D tomography

*斎藤 享1野崎 太成2山本 衛3 (1.国立研究開発法人海上・港湾・航空技術研究所電子航法研究所、2.京都大学大学院情報学研究科、3.京都大学生存圏研究所)

キーワード:電離圏トモグラフィー、電離圏リアルタイム連続観測、電離圏擾乱、電離圏3次元構造

Computerized Ionospheric Tomography (CIT) based on GNSS data is a powerful tool to study 3-D structures of the ionosphere.
We have developed a near-realtime regional ionospheric tomography system over Japan by using 200 selected stations of GEONET (GNSS Earth Observation Network) operated by Geospatial Information Authority of Japan (GSI). It has been operated since 2016.
Although the system generally performs well, it was also noticed that the ionospheric heights were sometimes overestimated when the true heights were quite low. To overcome this, assimilating ionosonde observation data into the 3-D tomography was proposed (Ssessanga et al., 2021).
We further refine the algorithm by optimizing the co-variance matrices and the cost function to be minimized. With this refinement, the ionospheric heights were better reproduced as compared with independent incoherent scatter measurement results by the MU radar. The system can still be operated in near-realtime with latency of a few to several minutes.
By using the improved tomography system, we investigated distinct ionospheric disturbances associated with severe geomagnetic storms occurred in 2023-2024. Signatures of polarization electric field are captured as the vertical displacements of the ionosphere. Thus, the improved 3-D tomography is very useful to study structures and mechanisms of ionospheric disturbances.