JpGU-AGU Joint Meeting 2020

講演情報

[E] ポスター発表

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] 大気圏ー電離圏結合

コンビーナ:Huixin Liu(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)、Yue Deng(University of Texas at Arlington)、Loren Chang(Institute of Space Science, National Central University)

[PEM12-P28] Vertical profile of ionospheric disturbances associated with Tohoku Earthquake using GPS occultation observation

*中田 裕之1今江 勇人2鷹野 敏明1大矢 浩代1 (1.千葉大学大学院工学研究院、2.千葉大学工学部電気電子工学科)

キーワード:音波、鉛直伝搬、掩蔽、津波、東北自身

Many studies have reported that ionospheric disturbances occur after giant earthquakes. One of the causes is the infrasound wave excited by ground motions and/or tsunami. The horizontal propagation of the ionospheric disturbances after large earthquake have been examined in detail by using a network of ground-based GPS receivers. On the other hand, the vertical propagation of coseismic ionospheric disturbances especially is rarely reported. In this study, to examine the vertical propagation of the ionospheric disturbances excited by tsunami, we have examined electron density profiles observed by GPS radio occultation measurements of FORMOSAT-3/COSMIC satellites. We analyzed the ionospheric disturbances caused by Tohoku Earthquake (M9.0) occurred at 5:46:18UT on 11 March 2011. Density profiles observed within 3 hours after the passage of tsunami were analyzed. In extracting disturbed components from observed density profiles using Chapman model, short wavelength fluctuations were recognized over altitude 300∼500 km. Wavelength spectrums of these fluctuations were calculated using wavelet transform. It is confirmed that the spectrum intensity for the wavelength of 10∼64 km were enhanced. Maruyama and Shinagawa (2014) showed that acoustic waves generated by ground motions of seismic wave excite ionospheric disturbances with the wavelength of several tens kilometers. The present results is consistent with these previous studies.