日本地球惑星科学連合2024年大会

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[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

2024年5月31日(金) 10:45 〜 12:00 展示場特設会場 (2) (幕張メッセ国際展示場 6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)、Chairperson:Jia Yue(NASA Goddard Space Flight Center)、Chang Loren(Institute of Space Science, National Central University)

11:00 〜 11:15

[PEM12-27] Investigation of the Local Time Dependence of Post-Sunset Medium-Scale Traveling Ionospheric Disturbances Over Japan

*傅 維正1大塚 雄一1 (1.名古屋大学 宇宙地球環境研究所)

キーワード:中規模伝搬性電離圏擾乱、衛星測位システム-TEC、電離圏イレギュラリティ

Ionospheric irregularities have extensively been an intriguing subject of research. Medium-scale traveling ionospheric disturbances (MSTIDs) serve as a common and significant manifestation of ionospheric perturbations predominantly observed in midlatitude regions. Particularly during nighttime, MSTIDs commonly exhibit a preference for a northwest-southeast (NW-SE) (northeast-southwest; NE-SW) alignment in the Northern (Southern) Hemisphere. Although the prevailing theory on the generation of nighttime MSTID is the E-F coupling, the limited observation coverage or spatiotemporal resolution inherent in many observational techniques prevent us from gaining a deeper understanding of this intricate process. In this research, we focus on the transition period when nighttime MSTIDs begin to generate. Dense GNSS observations from GEONET and SoftBank networks over Japan, complemented by multi-source data from other ground- and space-based ionosphere sounding techniques, are used to provide valuable insights into the MSTID generation, development, and persistence. In addition to the 2-D analysis, a 3-D tomography technique has been developed to analyze the structure variations of post-sunset MSTIDs. Preliminary findings indicate a clear correlation between local time and MSTID development after sunset. The complex interactions between the atmosphere and ionosphere could be important for comprehending the post-sunset MSTIDs.

Acknowledgements
The authors thank GSI and SoftBank Corp. and ALES Corp. for providing the GNSS RINEX files.