日本地球惑星科学連合2025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

2025年5月25日(日) 15:30 〜 17:00 303 (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:細川 敬祐(電気通信大学大学院情報理工学研究科)、傅 維正(名古屋大学 宇宙地球環境研究所)


15:30 〜 15:45

[PEM12-13] Development of the Chinese Dual Auroral Radar Network and Preliminary Results

★Invited Papers

*Jiaojiao Zhang1,2,3、Hang Li1,2,3、Wei Wang1,2,3、Xiang Deng1,2,3、Ailan Lan1,2,3、Jingye Yan1,2、Chi Wang1,2、J. Michael Ruohoniemi4Nozomu Nishitani5、S G Shepherd6 (1.National Space Science Center Chinese Academy of Sciences, Beijing, China、2.University of Chinese Academy of Sciences, Beijing, China、3.Siziwang Observatory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Ulanqab, China、4.Center for Space Science and Engineering Research (Space@VT), Virginia Polytechnic Institute and State University, VA, USA、5.Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Japan、6.Thayer School of Engineering, Dartmouth College, Hanover, NH, USA)

Led by the National Space Science Center of the Chinese Academy of Sciences, we have built a Chinese dual auroral radar network in northern China, which is called the CN-DARN. The CN-DARN consists of three pairs of high-frequency coherent scattering radar facilities and is one of the key parts of the Chinese Meridian Project Phase II. It has been fully constructed and started trial operations at the end of 2023. The detection range of the radar network extends longitudinally over approximately 9 hr of local times and covers the middle to high latitudes of the entire Asia region above 40° . In this paper, we present the basic design of the CN-DARN and its preliminary observations of ionospheric irregularities, subauroral polarization streams (SAPSs) and traveling ionospheric disturbances (TIDs). We also investigate its contribution to the ionospheric convection pattern of the Northern Hemisphere derived from Super Dual Auroral Radar Network (SuperDARN) observations. The results indicate that the CN-DARN provides excellent measurements and better specifications of flows in the Asian sector, improving our understanding of the global-scale ionospheric convection pattern in the Northern Hemisphere. These encouraging results lead us to believe that the CN-DARN will play an important role in studies on the evolution of ionospheric irregularities, the characteristics and evolution of SAPSs, the propagation of TIDs, and global-scale ionospheric convection dynamics.