日本地球惑星科学連合2021年大会

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[E] 口頭発表

セッション記号 S (固体地球科学) » S-IT 地球内部科学・地球惑星テクトニクス

[S-IT16] Structure and Dynamics of Earth and Planetary Mantles

2021年6月4日(金) 15:30 〜 16:45 Ch.24 (Zoom会場24)

コンビーナ:中川 貴司(University of Leeds)、芳野 極(岡山大学惑星物質研究所)、趙 大鵬(東北大学大学院理学研究科附属地震・噴火予知研究観測センター)、座長:芳野 極(岡山大学惑星物質研究所)

16:00 〜 16:15

[SIT16-08] Slow anomalies atop the 410-km discontinuity oceanward of the Kurile slab

*大林 政行1、吉光 淳子1、深尾 良夫1 (1.国立研究開発法人究海洋研究開発機構)

キーワード:410-km不連続面、トリプリケーション、トモグラフィー

Previous studies have shown slow anomalies atop the 410-km discontinuity below the subducting Honshu slab, which have been attributed to thermal anomalies (e.g. Obayashi et al., 2006; Bagley & Revenaugh, 2008). The slow anomaly area is, however, located toonly oceanward of the Honshu slab and northern Izu-Bonin slab and its spatial extent is still unknown. At the JpGU-AGU joint meeting 2020, we showed the retrograde-branch waves from the 410-km discontinuity on the Hi-net records from Kamchatka earthquakes arriving later by 2 or 3 seconds than the predictions form IASP91. We attributed this phenomenon to the 2 or 3 % slow anomaly atop the 410-km discontinuity along the Kurile and northern Honshu slabs. And at the 2020 SSJ fall meeting, we suggested the model M200M (Obayashi et al., 2006) that contains slow anomalies and depression of the 410-km discontinuity due to 200℃ excess temperature and less than 1 % melts, by comparing the observed waveforms with the synthetics by the model.

In this study, we inverted differential traveltimes between the first arrivals and later arrivals along the retrograde branch in addition to the first arrival time data of International Seismological Centre catalogue to investigate where these slow anomalies occur. The differential traveltimes are obtained by picking the peak of each phase on the squared envelope waveforms (Figure 1). The obtained tomography model shows strong slow anomalies oceanward Kurile slab near the 410-km discontinuities (Figure 2).