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-P29] Hunga Tonga-Hunga Ha’apoi 火山噴火による遠地地震波の解析:序報

*垂水 洸太郎1吉澤 和範1,2 (1.北海道大学理学院、2.北海道大学大学院理学研究院)

キーワード:フンガ・トンガ-フンガ・ハアパイ火山、遠地実体波、表面波、インフラサウンド、爆発的噴火、シングルフォース

An explosive eruption of the Hunga Tonga-Hunga Ha’apoi occurred on January 15, 2022. This eruption generated not only seismic and infrasound waves but also meteotsunamis, which arrived earlier than the expected arrivals of tsunamis. Although this eruption attracted the attention of many researchers on the generation of meteotsunamis, clear seismic signals have also been recorded by broad-band seismometers in the world. Here we summarize the characteristics of long-period seismic waves (10 - 200 s) observed in the Global Seismograph Network (GSN) and preliminary back-projection analysis using the first arrivals of teleseismic P-waves to unravel the seismological characteristics of the eruption sequence.

The first arrivals of P waves have been observed in farther epicentral distances for which P waves are radiated nearly downward from the source. The corresponding PP arrivals can also be seen clearly in the distance greater than 7000 km. These characteristics are consistent with the seismic waves generated by the vertical single-force at the source location, reflecting the eruption mechanisms.

Multiple sequences of the explosive eruptions can be identified from the multiple P and PP wave arrivals until they are masked by the energetic Rayleigh waves from the first explosive event. Long-period surface waves indicate significant variations of frequency contents in each explosive event, some of which have generated multi-orbit Rayleigh waves (up to R3) in the longer-period range (100 s ~). The infrasound waves propagating at 0.3 km/s have also been observed clearly in broad-band seismometers of GSN in the world.

We have used the long-period P-waves (10 – 100 s) for the back-projection analysis. The preliminary back-projection images located the source of long-period P-waves northwest of Hunga Tonga-Hunga Ha’apoi. Further analysis of the multiple arrivals of P and PP waves would enable us to clarify the eruption sequence.