日本地球惑星科学連合2014年大会

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インターナショナルセッション(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-EM06_30AM2] Study of coupling processes in Sun-Earth system with large radars and large-area observations

2014年4月30日(水) 11:00 〜 12:45 312 (3F)

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(名古屋大学太陽地球環境研究所)、橋口 浩之(京都大学生存圏研究所)、座長:山本 衛(京都大学生存圏研究所)

11:45 〜 12:00

[PEM06-03] SEALIONと赤道大気レーダーによる電離圏観測

*横山 竜宏1津川 卓也1石井 守1 (1.情報通信研究機構)

キーワード:SEALION, 赤道大気レーダー, 赤道スプレッドF, 赤道電離圏

Equatorial spread F (ESF) is a well-known phenomenon in the equatorial ionoshperic F region. As it causes severe scintillation in the amplitude and phase of radio signals, it is important to understand and forecast the occurrence of ESF from a space weather point of view. Ionospheric observation with the 47-MHz Equatorial Atmosphere Radar (EAR) in West Sumatra, Indonesia (0.20S, 100.32E, 10.36S dip latitude) has been conducted since 2001, and its unique observational data has been obtained for more than one solar cycle. The EAR is sensitive to 3-m scale ionospheric irregularities, which can be regarded as a tracer of ESF. Along with the EAR observations, Southeast Asia Low-latitude Ionospheric Network (SEALION) project by NICT started in 2003 for the purpose of monitoring and forecasting ESF. The SEALION consists of multiple ionosondes, GPS receivers and several other instruments in the Southeast Asian region. Since the developed ESF usually drifts eastward, monitoring ESF in this region can provide important space weather information for the Japanese longitude sector. We will summarize observational results with the SEALION and EAR, and discuss future potential of the ionospheric observation in the Southeast Asian region.