日本地球惑星科学連合2014年大会

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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-IT04_28AM1] Fluid flow, deformation and physical properties of the subduction boundary and forearc mantle

2014年4月28日(月) 09:00 〜 10:35 414 (4F)

コンビーナ:*ウォリス サイモン(名古屋大学大学院環境学研究科地球環境科学専攻地球惑星科学教室)、平松 良浩(金沢大学理工研究域自然システム学系)、平内 健一(静岡大学大学院理学研究科地球科学専攻)、水上 知行(金沢大学理工学域自然システム学類地球学コース)、座長:ウォリス サイモン(名古屋大学大学院環境学研究科地球環境科学専攻地球惑星科学教室)、平内 健一(静岡大学大学院理学研究科地球科学専攻)

09:25 〜 09:40

[SIT04-02] スラブとマントルがデカップリングする深さの空間変化がスラブ表面温度に与える影響

*森重 学1van Keken Peter2 (1.独立行政法人海洋研究開発機構、2.ミシガン大学)

キーワード:subduction zone, slab-mantle decoupling depth, slab surface temperature

In the subduction zone, we generally observe low seismic attenuation in the forearc mantle. In addition, surface heat flow shows low value in the forearc and a sudden transition to high value in the arc. These observations suggest that the forearc mantle is cold and is not involved in the corner flow in the mantle wedge. We can understand it in terms of slab-mantle decoupling depth (Ddec). Above Ddec, the mantle does not move with the slab just beneath it. Therefore, it becomes cold quickly due to the cooling from the overriding plate and the slab. Below Ddec, on the other hand, the mantle moves with the slab. It keeps this part of mantle warm by advection of hot material due to the corner flow. Thus, Ddec is a key parameter which strongly affects thermal structure in the subduction zone. Comparison of the observed surface heat flow and the one predicted with 2D numerical model suggests that Ddec does not vary much for each subduction zone and is 70-80km, but in each subduction zone Ddec may show some degree of along-arc variation. One such example is the junction between Japan and Kurile arcs, where the down-dip limit of thrust type earthquake is locally deepened by around 15km. In this presentation, we investigate the effects of a local deepening of Ddec on slab surface temperature.Toward the goal, we use time-dependent 3D finite element models to compute mantle flow and temperature. Only mantle wedge is treated as a dynamic entity. We use a simple slab geometry and assume a local deepening of Ddec to see its effects. We find that the increase in slab surface temperature at Ddec is larger where we assume a deepening of Ddec, which produces a warmer region there. It is caused by 3D flow in the mantle wedge due to along-arc variation of Ddec. We also calculate surface heat flow from obtained thermal structure, but it does not show significant along-arc variation. These results do not change even when we use a realistic slab geometry which is similar to that of the junction between Japan and Kurile arcs. While the surface heat flow anomaly and deepening of the seismic belt in S. Hokkaido cannot be easily explained by these models, the temperature excursions at the slab surface are significant. These models predict potentially strong variations in the conditions that the fluids leave the slab, which may be visible by various new geothermometers, such as those based on the H2O/Ce ratio.