日本地球惑星科学連合2014年大会

講演情報

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_1PM1] Study of coupling processes in Sun-Earth system with large radars and large-area observations

2014年5月1日(木) 14:15 〜 16:00 312 (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:野澤 悟徳(名古屋大学太陽地球環境研究所)

15:00 〜 15:15

[PEM06-31] 赤道大気レーダーとGPS受信機群を用いたVHFレーダーによるプラズマバブル検出の衛星航法補強システムに対する効果の検証

*斎藤 享1山本 衛2大塚 雄一3吉原 貴之1 (1.電子航法研究所、2.京都大学生存圏研究所、3.名古屋大学太陽地球環境研究所)

キーワード:赤道大気レーダー, 衛星航法補強システム, プラズマバブル, 電離圏監視

For global navigation satellite systems (GNSS), ionospheric plasma is one of the most serious error sources. Especially in air navigation where safety is extremely important, augmentation systems corresponding to flight phases are used. Even with augmentation systems of current design, such as ground-based augmentation system (GBAS) or satellite-based augmentation system (SBAS), probability of miss-detection of ionospheric anomalies prevent them from more advance operations. In the low latitude region, ionospheric anomaly detection is a challenge because of frequent occurrence of plasma bubbles.In this study, plasma bubble detection by a VHF backscatter radar is proposed as an external ionospheric monitor. Multi-beam observation of plasma bubbles can detect two dimensional shapes of plasma bubbles in a plane perpendicular to the magnetic field. When satellite-receiver path of GNSS signals pass crosses the magnetic field line, the signals shall be discarded because it may be affected by plasma bubble.To evaluate the performance of this system, a VHF radar-GNSS receivers combined experiment has been conducted. The Equatorial Atmosphere Radar (EAR) is used to detect plasma bubbles. Sets of GNSS receivers around the EAR and in Bangkok are used as the pseudo-user and reference station. The observation started from October 2012, and continues with some technical interruptions. At the meeting, first results of the experiment will be presented.