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-IT39_2AM1] 地球深部ダイナミクス:プレート・マントル・核の相互作用

2014年5月2日(金) 09:00 〜 10:45 416 (4F)

コンビーナ:*綿田 辰吾(東京大学地震研究所海半球観測研究センター)、境 毅(愛媛大学地球深部ダイナミクス研究センター)、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:坂巻 竜也(東北大学大学院理学研究科)、市川 浩樹(愛媛大学地球深部ダイナミクス研究センター)

10:30 〜 10:45

[SIT39-07] 核マントル境界の熱特性モデリング

*土屋 卓久1出倉 春彦1 (1.愛媛大学)

キーワード:第一原理計算, 格子熱伝導率, CMB熱流量

Lattice thermal conductivity of minerals under pressure and temperature is a key property to understanding dynamics and evolution of the Earth's interior. We recently established an efficient ab initio technique for calculating the thermal conductivity of silicate minerals with complex structure and chemistry (Dekura, Tsuchiya, Tsuchiya, PRL, 2013). Calculated lattice thermal conductivity of MgSiO3 perovskite agreed satisfactorily with experimental values at room temperature, and post-perovskite was found to have thermal conductivity quite different from perovskite's, indicating that the D" discontinuity is not only the phase transition boundary but also the conductivity boundary. Using the obtained results, we determine the effective conductivity of the lower mantle and estimate the energy flow across the core-mantle boundary (CMB). Our results demonstrate that the CMB heat flux could change significantly from place to place by reflecting temperature heterogeneity located atop the core. A large CMB heat flow recently suggested from the outer core side can be reconciled only by considering polycrystalline assemblages yielding high-thermal conductivity.