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-P23] 金属原子・イオン層同時観測のための共鳴散乱ライダーの開発

*江尻 省1,2、桂川 眞幸3、橋本 彩香3、小林 蒼汰3津田 卓雄3中村 卓司1,2 (1.国立極地研究所、2.総合研究大学院大学、3.電気通信大学)

キーワード:中間圏・熱圏、共鳴散乱ライダー観測、カルシウム原子・イオン層

In a transition region between neutral atmosphere and geospace plasma (80 - 500 km), vertical mass transport processes have still to be revealed because simultaneous measurement of neutral atmosphere and plasma is quite difficult. There are meteoric metal atoms and ions with a long chemical lifetime in this region. Calcium is the only metal that can be observed both of atom (Ca) and ion (Ca+) by ground-based resonant scattering lidar observations. To measure temporal variation in vertical density distributions of Ca and Ca+ ion, as a dynamical tracer in this region, and investigate the vertical mass transport, we are developing a resonance scattering lidar for simultaneous observation of Ca and Ca+ ion. The lidar system has an injection-locked Ti:Sapphire laser with a broad frequency tunability as a transmitter and receives the resonance scatter signals by a telescope with ~80cm diameter. The laser oscillator is designed that can be tuned to the resonance lines of Ca and Ca+ ion. We successfully receive the signals from each layer while a development for simultaneous observation is still ongoing. In this presentation, we will introduce the new lidar system and show some preliminary results of test observations.