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-IT03_29PM2] Structure and dynamics of Earth and Planetary deep interiors

2014年4月29日(火) 16:15 〜 18:00 418 (4F)

コンビーナ:*田中 聡(海洋研究開発機構 地球内部ダイナミクス領域)、芳野 極(岡山大学地球物質科学研究センター)、亀山 真典(国立大学法人愛媛大学地球深部ダイナミクス研究センター)、趙 大鵬(東北大学大学院理学研究科附属地震・噴火予知研究観測センター)、ヘルンランド ジョン(東京工業大学 地球生命研究所)、座長:Hernlund John(Earth-Life Science Institute, Tokyo Institute of Technology)、太田 健二(東京工業大学大学院理工学研究科地球惑星科学専攻)

17:00 〜 17:15

[SIT03-25] Can a stably stratified layer interrupt the top-down dynamics of Earth’s core?

*中川 貴司1 (1.IFREE, JAMSTEC)

キーワード:Earth's core, heterogeneity, core-mantle boundary, stably stratified layer, thermal wind

Takashi NakagawaIn some of previous studies of numerical dynamo simulation with a stably stratified region below the outer boundary, the long-wavelength feature of radial magnetic field can be only found on the outer boundary because a stratified layer can filter small-scale features of radial magnetic field generated in the convective region below the stratified boundary [Christensen, 2006; Nakagawa, 2011]. The existence of stably stratified region below the core-mantle boundary (CMB) is recently exposed from high pressure mineral physics [e.g. Pozzo et al., 2012] and seismological data analysis [e.g. Helffrich and Kaneshima, 2013]. Regarding the modeling on geomagnetic secular variation from numerical dynamo simulations, the heterogeneous thermal/chemical anomalies at the core-mantle boundary is important for understanding the time-scale of secular variation such as polarity reversals and excursions suggested from paleomagnetic observations [e.g. Olson et al., 2011; Olson et al., 2013] and current observational magnetic field [Aubert et al., 2013]. However, their investigation was not included in the effects of stably stratified region below the CMB in their dynamo simulations. Here we introduce several examples of numerical dynamo simulations with both heterogeneous outer boundary prescribed by the CMB heat flux calculated from numerical mantle convection simulations and a stably stratified layer. Preliminary results are found that the large-scale and ?amplitude of thermal/chemical anomalies induced by the heterogeneous boundary condition, that is, thermal wind type flow, may be trapped at the imposed stratified boundary. This may imply that the geomagnetic secular variations related to the core-mantle coupling may be suggested that the core surface flow would be a key physics.