日本地球惑星科学連合2015年大会

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セッション記号 M (領域外・複数領域) » M-IS ジョイント

[M-IS22] 地球流体力学:地球惑星現象への分野横断的アプローチ

2015年5月27日(水) 09:00 〜 10:45 106 (1F)

コンビーナ:*伊賀 啓太(東京大学大気海洋研究所)、中島 健介(九州大学大学院理学研究院地球惑星科学部門)、吉田 茂生(九州大学大学院理学研究院地球惑星科学部門)、柳澤 孝寿(海洋研究開発機構 地球内部ダイナミクス領域)、相木 秀則(海洋研究開発機構)、座長:吉田 茂生(九州大学大学院理学研究院地球惑星科学部門)

09:30 〜 09:45

[MIS22-03] 磁場の影響下での水平循環による流れ場の反転

*柳澤 孝寿1浜野 洋三1櫻庭 中2 (1.海洋研究開発機構、2.東京大学大学院)

キーワード:流れ場反転, 水平循環, 低プラントル数, 磁場

Coherent flow structures in the outer core are controlled by the magnetic field and rotation of the Earth. It is important to know the basic behavior of flow in relation to the magnetic field, for understanding the flow patterns observed in the real Earth and core dynamo simulations. On the other hand, spontaneous flow reversals generally observed in high Rayleigh number thermal convections may provide clue to the mechanism of random geomagnetic field reversals. As the most basic setting to observe the nature of flow structures with their time variations, we performed numerical simulations of Rayleigh-Benard convection in a three-dimensional square vessel by an electrically conductive low Prandtl number fluid, under a uniform horizontal magnetic field. Computed behaviors are consistent with the result of laboratory experiment (Yanagisawa et al., 2013) that shows flow reversals, and detailed process of reversals is clarified. The key mechanism is the emergence of a global circulation in the horizontal plane and following reconnection between rolls. An increase of global circulation induces bend and reconnection of convection rolls. It establishes a reversed flow state through roll number transitions. The horizontal circulation is related to the skewed-varicose instability of two-dimensional roll structure aligned in the direction of the magnetic field. This is a newly identified mechanism of flow reversal that works in large-scale three-dimensional geometry.