日本地球惑星科学連合2025年大会

講演情報

[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26日(月) 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:西山 尚典(国立極地研究所)、Yang-Yi Sun(China University of Geosciences)


16:30 〜 16:45

[PEM12-41] Response of ionospheric F2-peak height and sea levels to the lunar gravitational force

*Tsung-Yu Wu1Jann-Yenq LIU1 (1.National Central University)

キーワード:Ionospheric height, Sea level, Lunar gravitational force

The semidiurnal lunar tide (M2) is a well-known phenomenon in the ocean and upper atmosphere. This study utilizes the ionospheric electron density sounded by global navigation satellite system (GNSS) radio occultation (RO) measurements and sea levels (SLs) recorded by NOAA (National Oceanic and Atmospheric Administration) tide gauges to examine the M2 signatures in both the ocean and ionosphere. The F2-peak height (hmF2) and SL yield the M2 amplitude in a range of 0.3–198 cm and 0.7–7.3 km, respectively. The M2 high tide in hmF2 typically leads the sublunar point by about 3 lunar hours. By contrast, the high tide in M2 of SLs at various locations can occur almost anytime, which suggests that the geographic topography plays an important role. Statistical analysis reveals no significant correlation between the M2 amplitude or phase of SL and hmF2, which indicates that SL variations are unlikely to modulate hmF2 under the M2 mode.