日本地球惑星科学連合2014年大会

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インターナショナルセッション(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-IT04_28AM2] Fluid flow, deformation and physical properties of the subduction boundary and forearc mantle

2014年4月28日(月) 11:00 〜 12:45 414 (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:平松 良浩(金沢大学理工研究域自然システム学系)、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)

Subduction brings oceanic crustal material into direct contact with the overlying mantle wedge. The subduction boundary changes its slip behaviour from seismic to aseismic with increasing depth. The deep forearc region around the tip of mantle wedge shows a transitional nature with episodic tremor and slip which are probably strongly influenced by sustained fluid flow. The amount of fluid release in the forearc is not well constrained but is thought to depend on the thermal structure of the subduction zone. Fluid released into the forearc mantle will cause a transformation of mantle rock to serpentinite. This metamorphic transformation implies a major volume change and a change in physical properties of the mantle. Despite considerable recent advances in understanding these processes, there is no good consensus on how strong this forearc region is likely to be or how fluids are transported. Such information is vital in developing more complete tectonic models of these geologically and geophysically important regions. In this session we aim to contribute to our understanding of the deep forearc by bringing together the results of a variety of different approaches including field based observations, experimental work, theoretical modeling and geophysical observations on deformation, reaction and physical properties in fluid-rock systems.