日本地球惑星科学連合2025年大会

講演情報

[E] 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

2025年5月25日(日) 17:15 〜 19:15 ポスター会場 (幕張メッセ国際展示場 7・8ホール)

コンビーナ:細川 敬祐(電気通信大学大学院情報理工学研究科)、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)

17:15 〜 19:15

[PEM12-P07] 共鳴散乱ライダーによるCa/Ca同時・同領域観測

*江尻 省1,2桂川 眞幸3,1橋本 彩香3、小林 蒼汰3、三好 咲也子3、宮城 晃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:共鳴散乱ライダー観測、カルシウム原子とイオン、中間圏・下部熱圏、中性・イオン結合

To measure temporal variation in vertical density distributions of meteoric metal atom and ion, as a dynamical tracer in the Mesosphere and Thermosphere, and investigate the vertical mass transport, we are developing a resonance scattering lidar for simultaneous observation of Calcium atom (Ca) and ion (Ca+). 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 ~80 cm diameter. The laser oscillator is designed so that the oscillation frequencies can be tuned simultaneously to the resonance lines of Ca and Ca+ ion. Laser pulses of two wavelengths were emitted from a single laser resonator simultaneously, and common-volume and simultaneous measurements of Ca and Ca+ densities were successes in Tachikawa (36N, 139E) at 10:50-21:10 UT on December 24, 2024. Both of Ca and Ca+ layers were observed at 80 – 105 km during all the night. Dense-thin layers of Ca+ were seen at ~100 km before 13 UT and ~95 km around 17 UT which were slightly higher altitudes than top of Ca layer. After 16:45 UT until sunrise, Ca+ layer had a dense-thin layer with a few km FWHM at 90 – 95 km, while Ca did not show such a dense-thin layer. In this presentation, we will discuss dynamics and chemical process of neutral atom and ion coupling by comparison in density, height and fine structures between Ca and Ca+.