日本地球惑星科学連合2014年大会

講演情報

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-IT05_28AM1] Cause and evolution of plate tectonics: Advances in understanding oceanic plate-continental systems

2014年4月28日(月) 09:00 〜 10:45 315 (3F)

コンビーナ:*Becker Thorsten(Department of Earth Sciences, University of Southern California)、Hernlund John(Earth-Life Science Institute)、中川 貴司(海洋研究開発機構地球内部ダイナミクス領域)、座長:中川 貴司(海洋研究開発機構地球内部ダイナミクス領域)、Hernlund John(Earth-Life Science Institute, Tokyo Institute of Technology)

10:15 〜 10:30

[SIT05-06] Effects of plate-like behavior and material recycling on lateral variation of CMB heat flux

*中川 貴司1 (1.IFREE, JAMSTEC)

キーワード:CMB heat flux, lateral variation, plate tectonics, material recycling

We studied the relationship between heat flux across the core-mantle boundary (CMB) and seismic anomalies in the CMB region in numerical mantle convection simulations in a 3-D spherical shell with a simple temperature- and depth-dependent viscosity [Nakagawa and Tackley, 2008]. That study suggested that the relationship between CMB heat flux and seismic anomalies was not simple linear function because of the post-perovskite phase transition and/or compositional heterogeneous structure in the deep mantle. However, in that study, we did not include the complicated rheology that occurred to the plate tectonics-like behavior and the segregation of oceanic crust in the deep mantle because they would be important for regulating the heat flux across the CMB [e.g. Nakagawa and Tackley, 2010]. Here we revisit to investigate the relationship between heat flux across the CMB and seismic anomalies in the deep mantle including plate tectonics-like behavior and material recycling. Preliminary result suggests that the heat flux tends to be more linear relationship with seismic anomalies in the deep mantle including plate tectonics-like behavior and material recycling but the uncertainty of this relationship between two quantities is very strong. The peak-to-peak of lateral variation of CMB heat flux is much larger than that obtained from our previous study. This is still problematic for magnetic field generation caused by geodynamo.