日本地球惑星科学連合2024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-EM15] 太陽地球系結合過程の研究基盤形成

2024年5月29日(水) 17:15 〜 18:45 ポスター会場 (幕張メッセ国際展示場 6ホール)

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)

17:15 〜 18:45

[PEM15-P10] TromsoのNa lidarに用いる昼間観測と熱圏観測のための超狭帯域フィルタの開発(3)

*川原 琢也1野澤 悟徳2、斎藤 徳人3津田 卓雄4、川端 哲也2、和田 智之3高橋 透5 (1.信州大学工学部、2.名古屋大学宇宙地球環境研究所、3.理化学研究所光量子工学研究センター、4.電気通信大学、5.国立研究開発法人 海上・港湾・航空技術研究所 電子航法研究所)

キーワード:ナトリウムライダー、磁気光学フィルタ

An ultra-narrowband magneto-optical filter, also called a Faraday dispersive filter, is being developed for the Na LIDAR receiver in Tromsø to enable thermonspheric observations and daytime observations in sunlit conditions. The filter consists of a heated Na cell between two crossed polarizers in a strong magnetic field, producing a transmission profile.

Currently, the following stages of development are underway:
1. A new Faraday filter is being built for the new lidar receiver. Its transmission profiles are being measured at RIKEN with a high resolution of a few MHz under different cell temperatures with magnetic fields of 170 mT. The measured transmission profiles are being compared with theoretical ones for validation.
2. A new sapphire cell is being developed for LIDAR daytime measurements. Commercially available glass-type Na cells corrode at high temperatures of over 150°C due to chemically active high-temperature Na atoms in the cell.
3. A thermal stability test of the transmission profiles has been conducted, assuming long-term observation. The filter transmission during observation is required for data analysis, so the transmission needs to be measured between observations.

Discussions on these topics are presented in the talk.