日本地球惑星科学連合2023年大会

講演情報

[E] オンラインポスター発表

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

2023年5月26日(金) 15:30 〜 17:00 オンラインポスターZoom会場 (4) (オンラインポスター)

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)

現地ポスター発表開催日時 (2023/5/26 17:15-18:45)

15:30 〜 17:00

[PEM15-P02] Improvement and case analysis of three dimensional ionospheric tomography based on GNSS-TEC observation with ionosonde data assimilation

*野崎 太成1斎藤 享2Nicholas Ssessanga3山本 衛1 (1.京都大学生存圏研究所、2.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、3.4-D Space, Department of Physics, University of Oslo, Blindern, 0316 Oslo, Norway)

キーワード:トモグラフィ、データ同化、3次元変分法

Structures of the electron density in the ionosphere cause reflection, absorption, and delay of radio waves, which can lead to interference in radio communications. Therefore, the observation of the ionospheric electron density is of great importance. One method of ionospheric analysis is tomography, which estimates the three-dimensional structure of the ionosphere from the GNSS-TEC observation data.
The original algorithm employed to cover the Japanese archipelago and the nearby surrounding region was the constrained least-squared fitting method implemented by Seemala et al. (2014) and Suzuki (2016). The method used the spatial gradient of the electron density as the constraint, and in addition, introduced boundary conditions at the top and the bottom to stabilize the results. The original algorithm was stable and useful. But it had problems with negative electron density as the solution. It also tended to estimate the peak electron density higher than the true height during autumn and winter.
To solve these problems, Ssessanga et al. (2021) proposed an improved algorithm based on a 3D-VAR method by adding ionosonde data. Recently we analyzed the improved version, and a discussion with the authors (private communication) revealed some inconsistencies in the background error covariance matrix (B), which specifies the correlation of voxels in vertical and horizontal directions. This study presents results after improving B; a comparison of the tomography solution of the modified algorithm and the original algorithm using MU radar’s observation confirmed that the modified algorithm improved the accuracy of peak height estimation. Also, a case study was conducted on the traveling ionospheric disturbance (TID) event from the Tonga eruption in January 2022. This is a unique ionospheric event, and the results were validated by modifying the algorithm.