日本地球惑星科学連合2018年大会

講演情報

[JJ] Eveningポスター発表

セッション記号 A (大気水圏科学) » A-TT 計測技術・研究手法

[A-TT32] GNSS-Rが拓く新しい地球観測

2018年5月21日(月) 17:15 〜 18:30 ポスター会場 (幕張メッセ国際展示場 7ホール)

コンビーナ:市川 香(九州大学応用力学研究所)、日置 幸介(北海道大学大学院理学研究院地球惑星科学部門)

[ATT32-P03] Wind-independent periodic variations of signal intensity of a geostationary GNSS satellite observed at an ocean observation tower

*奥村 立樹1市川 香1海老沼 拓史2李 梓原3根田 昌典4吉川 裕4馬場 康之5 (1.九州大学応用力学研究所、2.中央大学工学部、3.深圳市海洋観測予報センター、4.京都大学理学研究科、5.京都大学防災研究所)

キーワード:GNSS 静止衛星、GNSS-R、風速非同期周期的変動、位相干渉強度変化、経路長変化、潮汐

GNSS-R receivers were deployed to the Shirahama Oceanographic Observatory Tower owned by Kyoto University (33deg 42’32”N, 135deg 19’58”E) at the height of 20 m. The signal intensity, measured as signal-to-noise ratio (SNR), of a geostationary GNSS satellite (Beidou #2) was observed every second for both directly-received signals and signals reflected at the sea surface. In general, the SNR of the reflected signal fluctuates larger than that of the direct signal. Even after removal of high-frequency fluctuations by 3-minute smoothing, the SNR of the reflected signal shows larger changes, and these changes tend to be inversely correlated with the wind speed, which are consistent with less reflection by rougher sea surface. However, the SNR of the reflected signal intermittently shows significant periodic variations whose cycle is about one hour. These variations are not synchronized with variations of the wind speed, and they are observed only when the wind is weaker than 4m/s. Furthermore, similar variations were commonly found even in the direct signal. Therefore, they are considered mutual effects between direct and reflected signals, or interferometric intensity variations. Since the phase of the reflected signal depends on the path length, the tidal sea level changes would cause the path length, and thus interferometric SNR intensity. The path length change calculated from the sea level observed by a tide gauge at the tower provides consistent interferometric variation as the observed SNR.