日本地球惑星科学連合2018年大会

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セッション記号 S (固体地球科学) » S-CG 固体地球科学複合領域・一般

[S-CG53] Science of slow earthquakes: Toward unified understandings of whole earthquake process

2018年5月24日(木) 15:30 〜 17:00 コンベンションホールB(CH-B) (幕張メッセ国際会議場 2F)

コンビーナ:井出 哲(東京大学大学院理学系研究科地球惑星科学専攻)、廣瀬 仁(神戸大学都市安全研究センター)、氏家 恒太郎(筑波大学生命環境系、共同)、波多野 恭弘(東京大学地震研究所)、座長:波多野 恭弘麻生 尚文

16:30 〜 16:45

[SCG53-35] New dynamic model of slow earthquakes considering stochasticity in rupture simulation

*麻生 尚文1,2安藤 亮輔1井出 哲1 (1.東京大学大学院理学系研究科、2.東京工業大学理学院)

Slow earthquakes are often modeled under the heterogeneous distribution of the frictional parameters of rate-and-state friction law. To consider heterogeneity at smaller scales than the grid size, we adopt stochastic governing equations, which we traditionally assume deterministically. An external force including tidal stress is known to affect both regular and slow earthquakes not deterministically but stochastically, so we also add a stochastic body force. In this study, we solve mode III problem using BIEM scheme, but we add stochastic perturbations in the governing equations. To focus on the classic effect of introducing stochasticity, we select simple conditions including slip-weakening friction law and homogeneous initial/boundary conditions. As a result, we reproduced slow rupture propagations without introducing any heterogeneity explicitly. We may need to consider the origin of the stochasticity more carefully, we could use rate-and-state friction laws instead, and we could assume heterogeneous initial/boundary conditions, but it is pivotal finding that only stochasticity could reproduce slow rupture propagations.