日本地球惑星科学連合2023年大会

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[J] 口頭発表

セッション記号 M (領域外・複数領域) » M-IS ジョイント

[M-IS12] 地球流体力学:地球惑星現象への分野横断的アプローチ

2023年5月23日(火) 13:45 〜 15:00 202 (幕張メッセ国際会議場)

コンビーナ:伊賀 啓太(東京大学大気海洋研究所)、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(国立研究開発法人海洋研究開発機構 海域地震火山部門)、相木 秀則(名古屋大学)、座長:中島 健介(九州大学大学院理学研究院地球惑星科学部門)

13:45 〜 14:00

[MIS12-01] Heat transport and mixing in extremely confined Rayleigh-Bénard convection

*能登 大輔1、Ulloa Hugo1、Letelier Juvenal2 (1.University of Pennsylvania、2.Universidad de Chile)

キーワード:Thermal convection、Heat transport、Mixing、Hele-Shaw

Thermally driven flows in strongly confined environments, such as permeable media, are ubiquitous in nature. They contribute to the heat transfer across the Earth’s lithosphere and fluid mixing process within aquifers. The Hele-Shaw system is a laboratory analog for such geometrically constrained convective flows. In this work, we study heat transport and mixing characteristics of thermal convection in Hele-Shaw systems through laboratory experiments. Transparent fluid layers built for the laboratory experiments allow elucidation of velocity fields, and heat distributions were obtained for quasi-steady states throughout the heat equation. The experimental results are partially in agreement with the theoretical and numerical ones, except for the high Rayleigh-Darcy number at which the system becomes three-dimensional. We will discuss the flow features, heat transport characteristics, and mixing efficiency of thermal convection in extremely confined domains, covering Darcy, Hele-Shaw (quasi-two-dimensional), and three-dimensional regimes.