JpGU-AGU Joint Meeting 2020

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-EM18] 太陽地球系結合過程の研究基盤形成

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)

[PEM18-12] Complimenting regional GPS-TEC computerized ionospheric tomography (CIT) with ionosonde data assimilation

*Nicholas Ssessanga1Mamoru Yamamoto 1Susumu Saito2Akinori Saito3Michi Nishioka4 (1.RISH 、2.ENRI、3.Kyoto Univ.、4.NICT)

キーワード:Ionosphere, Tomography, Data assimilation , GPS-TEC, Ionosonde

The accurate probing of the three-dimensional (3-D) structure of the ionosphere endures a unique set of challenges that include for example high campaign costs, poor distribution of instruments and collected data, and geometric limitations. To remedy these challenges, over the East-Asian sector (covering 110°–160°E and 10°–60°N, and extending from 80 to 20,000 km in altitude) a near real-time regional 3-D computerized ionospheric tomography (CIT) technique has been developed using a plethora of GPS (Global Positioning System) observations of total electron content. A validation of the CIT results using ionosonde and occulation data shows the technique adequately reconstructs the regional ionosphere vertical structure, however, with room for improvement in estimating the peak height and avoiding physically unrealistic negative densities in the final solution. This paper presents preliminary results from a technique that addresses these problems, by incorporating CIT results into a data assimilation (DA) technique. The DA technique adds ionosonde bottomside measurements into CIT results, thereby improving the accuracy of the reconstructed peak height and bottomside 3-D structure. Further, we assume that ionosphere electron densities are better described by probability log-nomal distribution, which introduces the non-negativity constraint.