JpGU-AGU Joint Meeting 2020

講演情報

[E] ポスター発表

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-CG57] 広域観測・微視的実験連携による沈み込み帯地震研究の新展開

コンビーナ:木下 正高(東京大学地震研究所)、河野 義生(愛媛大学地球深部ダイナミクス研究センター)、荒木 英一郎(海洋研究開発機構)、Hiroko Kitajima(Texas A&M University College Station)

[SCG57-P06] Dynamic strain energy as new evaluation item of a seismogenic fault

*坂口 有人1市来 政仁2瀧口 吉香1 (1.山口大学、2.アサノ大成基礎エンジニアリング)

キーワード:応力、沈み込み帯、震源断層

Since earthquake is stress response of the crust, the stress-strain record of the host rock around the fault tell us significant clue of the seismic mechanism. During inter-seismic period, host rock around the asperity deformed elastically to cause the earthquake. Immediately before the earthquake, a rupture propagates from deep nucleation point, and high stress must concentrate at tip of the fracture. This stress concentration causes elastic strain momentary in host rock of the fault, and high stress area moves with rupture propagation.

The strain energy of these event can be estimated from paleo-stress distribution around the fault. It is expected that the highest peak of stress must be appeared at fault center, and stress level will decrease with distance from the fault. The area under the stress decay curve in the stress-distance graph indicates strain energy of the host rock.

Paleo-stress of ancient fault rock can be estimated from elastic rebounded rock using calcite twin method (Sakaguchi et al., 2011).

The Okitsu Fault in Shimanto accretionary complex, southwest Japan is ancient seismogenic fault of plate subduction zone. This fault involves pseudotachylyte and can be observed more than 10 km along the strike of the fault. Higher stress than the background stress of regional Shimanto accretionary complex was found around the Okitsu Fault. This may be due to dynamic stress concentration during rupture propagation. The value of estimated dynamic strain energy is approximately 390 MJm^-2 at eastern tip of the Okitsu Fault. The strain energy along the strike of the fault decreases toward west and disappears at 2 km from the eastern tip. The strain energy along the fault increases again to several MJm^-2 at 9 km from the eastern tip. This strain energy variation may show existence of some locked asperities along the strike of the fault.