日本地球惑星科学連合2018年大会

講演情報

[EE] 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-IT26] 地殻応力研究の最前線:観測・実験・モデリングの統合

2018年5月20日(日) 09:00 〜 10:30 A01 (東京ベイ幕張ホール)

コンビーナ:呉 泓昱(海洋研究開発機構)、林 為人(京都大学大学院工学研究科)、真田 佳典((国研)海洋研究開発機構、共同)、Chan Chung-Han(Earth Observatory of Singapore, Nanyang Technological University)、座長:呉 泓昱(海洋研究開発機構)、Chung-Han Chan(Earth Observatory of Singapore)

09:15 〜 09:30

[SIT26-02] Orientation of the SHmax in accretionary prisms from real-scale numerical sandbox experiments

★Invited Papers

*古市 幹人1西浦 泰介1Bauville Arthur1桑野 修1堀 高峰1阪口 秀1 (1.海洋研究開発機構)

キーワード:付加体、砂箱実験、個別要素法、スーパーコンピュータ

The stress states in accretionary prisms are important for understanding the building and releasing of seismic energy. The in-situ stress states estimated from borehole data in IODP expeditions showed significant deviations in the maximum horizontal stress (SHmax) orientation from the plate convergence. These deviations reflect the 3D structure of the stress state rather than the 2D structure; however the 3D stress structures as well as their effects on the evolution of the accretionary prism are not clear. Analog sandbox experiments can be used to deduce such stress states. We performed real-scale and threfore large-scale numerical sandbox experiments using the discrete element method to understand the 3D stress state in the accretionary prism. The stress chain analyses demonstrate that the in-situ stress orientation from borehole data can be a signal of either the regional direction of plate convergence or the local stress orientation associated with the stress arch. The formation of stress arches is expected by the nonlinearities inherent in crustal deformation and micro-scale perturbations. I want to discuss the possibility of the long-term monitoring of the SHmax orientations in boreholes to support this hypothesis.