日本地球惑星科学連合2022年大会

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[U-09] 気象津波の発生を伴ったトンガ海底火山噴火

2022年5月30日(月) 11:00 〜 13:00 オンラインポスターZoom会場 (40) (Ch.40)

コンビーナ:日比谷 紀之(東京大学大学院理学系研究科地球惑星科学専攻)、コンビーナ:前野 深(東京大学地震研究所)、コンビーナ:中島 健介(九州大学大学院理学研究院地球惑星科学部門)、コンビーナ:田村 芳彦(海洋研究開発機構 海域地震火山部門)、座長:日比谷 紀之(東京海洋大学 海洋環境科学部門)、前野 深(東京大学地震研究所)、中島 健介(九州大学大学院理学研究院地球惑星科学部門)、田村 芳彦(海洋研究開発機構 海域地震火山部門)

11:00 〜 13:00

[U09-P10] 2022年1月15日のトンガ火山噴火に伴う津波のシミュレーション

*藤井 雄士郎1佐竹 健治2 (1.国立研究開発法人 建築研究所 国際地震工学センター、2.東京大学 地震研究所)

キーワード:フンガ・トンガーフンガ・ハアパイ火山噴火、津波シミュレーション、気圧波

We simulated tsunamis generated from the Hunga Tonga-Hunga Ha'pai volcano eruption on January 15, 2022. The atmospheric waves from the eruption were recorded globally with propagation velocities of ~0.31 km/s (Lamb wave) and 0.20 - 0.24 km/s (atmospheric gravity wave). In the far-field, the tsunamis were recorded earlier than the expected arrival time calculated by long-wave velocity, suggesting that at least the initial part of the observed tsunami was caused by propagating atmospheric waves. We numerically solved the linear long-wave equations in the spherical coordinate system with a grid interval of 24 arc-sec for 20-hour tsunami propagation.
We simulated the tsunami from the moving ring-shape sea surface elevation. The ring is parameterized by its propagation speed and peak amplitude. The amplitude decays with a distance as 1/sqrt(R*sin(delta)), where R is Earth radius, delta is epicentral angle distance. From the comparison at three US DARTs and 10 New Zealand DARTs, we assumed a circular source starting at the eruption time (at 04:15). The observed first phase can be reproduced by a ring with an amplitude of 4 m and a rise time of 10 min, propagating at Lamb wave speed of 0.31 km/s. The corresponding ring width is ~370 km. The later phase can be better reproduced by adding another propagating ring with a negative amplitude and a gravity wave speed of 0.20 - 0.24 km/s. The DART stations around the Pacific indicate that the gravity wave speed is higher toward Japan and South America, while it is slightly slower toward North America. The simulated waveforms roughly reproduced the far-field tsunami waveforms recorded on tide gauge stations, including the later phase, suggesting that the large amplitude wave in the later phase may be due to resonance around tide gauge stations.