日本地球惑星科学連合2016年大会

講演情報

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-EM16] 大気圏・電離圏

2016年5月24日(火) 17:15 〜 18:30 ポスター会場 (国際展示場 6ホール)

コンビーナ:*大塚 雄一(名古屋大学太陽地球環境研究所)、津川 卓也(情報通信研究機構)、川村 誠治(独立行政法人 情報通信研究機構)

17:15 〜 18:30

[PEM16-P18] 高い高度分解能を持つロケットGPS-TECトモグラフィ法の検証

*池端 祐太朗1芦原 佑樹1 (1.奈良工業高等専門学校 電子情報工学専攻)

キーワード:電離圏、GPS-TEC、観測ロケット

In the high altitude atmosphere of the earth, there is a layer of atmosphere called ionosphere, filled with extricated electrons, and the observation of the electron density profile in the ionosphere is recently taken notice of.
As an approach to the observation of electron density profile in the ionosphere, there is the remote sensing method called GPS-TEC method, which calculates the total electron counts (TEC) on the transmission path of GPS wave, from its propagation delay. By applying tomography analysis on TEC values in multiple paths, which are one dimensional information, the electron distribution profile can be earned as two dimensional data, and this method is called GPS-TEC tomography method. However, this method has a defect, that it has low resolution in altitude direction.
In order to enhance the altitude resolution, we have proposed “Rocket GPS-TEC Tomography method,” which applies tomography analysis on the TEC values earned by rocket observation. Compared to the conventional GPS-TEC tomography, this method can observe TEC values in horizontal paths, as the observation rocket navigates in both range and altitude direction. By this approach, we assumed that altitude resolution of the tomography result will improve. In this study, we verified the efficacy of proposed method through simulation experiment.