日本地球惑星科学連合2025年大会

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[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-EM12] Coupling Processes in the Atmosphere-Ionosphere System

2025年5月26日(月) 09:00 〜 10:30 303 (幕張メッセ国際会議場)

コンビーナ:細川 敬祐(電気通信大学大学院情報理工学研究科)、Liu Huixin(九州大学理学研究院地球惑星科学専攻 九州大学宙空環境研究センター)、大塚 雄一(名古屋大学宇宙地球環境研究所)、Chang Loren(Institute of Space Science, National Central University)、座長:Chang Loren(Institute of Space Science, National Central University)、Lin Charles(Department of Earth Sciences, National Cheng Kung University)

10:15 〜 10:30

[PEM12-24] High-Resolution 3-D Imaging of Electron Density Perturbations Using GNSS Observations Over Japan

*傅 維正1大塚 雄一1 (1.名古屋大学 宇宙地球環境研究所)

This study introduces a newly developed three-dimensional (3-D) computerized ionospheric tomography (CIT) technique designed to reconstruct electron density perturbations caused by ionospheric disturbances. The CIT technique is facilitated by dense total electron content (TEC) measurements from ground-based Global Navigation Satellite System (GNSS) receivers in Japan. The slant TECs used for tomography consist of two components: the background electron density derived from the IRI-2016 model, and the TEC perturbations obtained through a centered moving average for each line-of-sight slant TEC. Simulations were conducted to evaluate the performance of the CIT algorithm, demonstrating high fidelity, with the technique accurately reconstructing over 80% of electron density perturbations. Recently, this method has been successfully applied to investigate different ionospheric phenomena, including traveling ionospheric disturbances (TIDs) driven by acoustic waves, atmospheric gravity waves, or electrodynamic forces, as well as equatorial plasma bubbles (EPBs) extending to midlatitudes.

Acknowledgements
The GNSS observation data from SoftBank used in this study were provided by SoftBank Corp. and ALES Corp. through the Consortium to utilize the SoftBank original reference sites for Earth and Space Science.