日本地球惑星科学連合2025年大会

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-EM12] Coupling Processes in the Atmosphere-Ionosphere System

2025年5月26日(月) 09:00 〜 10:30 303 (幕張メッセ国際会議場)

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)、座長:Chang Loren(Institute of Space Science, National Central University)、Lin Charles(Department of Earth Sciences, National Cheng Kung University)

09:30 〜 09:45

[PEM12-21] Investigation of the daytime sporadic-E layer by the RIDE campaign 2025

*齊藤 昭則1阿部 琢美2松岡 彩子3石坂 圭吾4斎藤 義文2田川 雅人5熊本 篤志6小嶋 浩嗣7栗田 怜7横田 久美子5西岡 未知8安藤 慧8斎藤 享9高橋 透9細川 敬祐10中田 裕之11横山 竜宏7Liu Huixin12西山 尚典13江尻 省13坂崎 貴俊1 (1.京都大学大学院理学研究科地球物理学教室、2.宇宙航空研究開発機構・宇宙科学研究所・、3.京都大学 理学研究科 地磁気世界資料解析センター、4.富山県立大学工学部電気電子工学科、5.神戸大学、6.東北大学大学院理学研究科地球物理学専攻、7.京都大学生存圏研究所、8.国立研究開発法人情報通信研究機構、9.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、10.電気通信大学大学院情報理工学研究科、11.千葉大学大学院工学研究院、12.九州大学理学研究院地球惑星科学専攻、13.国立極地研究所)

キーワード:電離圏、スポラディックE層、電波伝搬、観測ロケット

The Rocket Investigation of the Daytime E-region (RIDE) campaign is scheduled to take place in the summer of 2025 in Japan. This is a coordinated observational campaign involving the S-310-46 sounding rocket launched from Uchinoura, Japan, along with a ground-based network that includes ionosondes, VHF receivers, and GNSS receivers. The campaign was postponed due to technical issues with the sounding rocket in the summer of 2024." There are three objectives of this campaign as follows:
(1) Elucidate phenomena in which the interaction between neutral atmosphere and plasma is important by combining in-situ observations by the sounding rocket with a numerical model and ground-based observations.
(2) Develop instrumental packages to measure the neutral atmosphere, plasma, and electromagnetic fields for sounding rockets and satellites.
(3) Foster human resources for future missions.
This campaign is designed to reveal sporadic-E layers' formation and transportation process. Such information is essential for predicting anomalous radio wave propagation caused by sporadic-E layers. The ground-based network of ionosondes and GNSS receivers monitors the horizontal structure and movement of Es layers. This information will be used to make the launch decision for the sounding rocket aimed at the moderate or intense Es layer. Seven scientific payloads are carried on the RIDE rocket. These include the Neutral Mass Spectrometer (NMS), Neutral Density and Wind Instrument (IOG), Ion Velocity Analyzer (IVA), Impedance Probe (NEI), Fast Langmuir Probe (FLP), Electric Field Detector (EFD), and Magnetometer (MAG). The physical parameters of both the neutral and ionized atmosphere, inside and outside the Es layers, will provide crucial information to help solve several unresolved questions about the Es layers. Why are Es layers so sporadic? Do they have frontal structures? What role does the electric field play in their formation and transport? Do atmospheric gravity waves contribute significantly? Combination of high-resolution data of the in-situ measurement, and wide field-of-view data of the ground-based network, and three-dimensional numerical simulation coupled with a global model is expected to elucidate the Es layer processes that have been unclear so far. The outline of the observation and scientific targets will be presented in the presentation.