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-EM12] Coupling Processes in the Atmosphere-Ionosphere System

2023年5月22日(月) 10:45 〜 12:15 オンラインポスターZoom会場 (2) (オンラインポスター)

コンビーナ: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)、Yue Deng(University of Texas at Arlington)


現地ポスター発表開催日時 (2023/5/21 17:15-18:45)

10:45 〜 12:15

[PEM12-P09] Development of an Ionospheric-Plasmaspheric Data Assimilation Model

*CHIYEN LIN1,2Jann-Yenq LIU1,2,3Charles Lin4 (1.Center for Astronautical Physics and Engineering, National Central University, TAIWAN、2.Department of Space Science and Engineering, National Central University, Taiwan、3.Center for Space and Remote Sensing Research, National Central University, Taiwan.、4. Department of Earth Sciences, National Cheng Kung University, Taiwan.)

キーワード:Ionosphere, Plasmasphere, Data Assimilation, FORMOSAT-7/COSMIC-2

The data assimilation model global ionospheric specification (GIS) reconstructs ionospheric three-dimensional electron density structure by using a Gaussian-Markov Kalman filter to assimilate ground-based GNSS slant total electron content (TEC) and FORMOSAT-7/COSMIC-2 radio occultation slant TEC observations. The study based on GIS to extends the altitude boundary of the model from the ionosphere to the lower plasmasphere (from 1,000 to 21,000 km). The new ionospheric-plasmaspheric data assimilation model could assimilate the completed sounding path of ground-based GNSS slant TEC and F7/C2 absolute TEC (podTc2) to improve ionospheric electron density structure and also reconstruct the plasmasphere. The observing system simulation experiment (OSSE) is applied to confirm the accuracy of the reconstructed electron density structure in the ionosphere and plasmasphere. The OSSE demonstrates that analysis results are similar to the simulation truth, indicating that the model can reconstruct the ionosphere and the plasmasphere. In addition, electron density reconstruction is also being implemented to study the influence of geomagnetic storms on the ionosphere and plasmasphere.