JpGU-AGU Joint Meeting 2020

講演情報

[J] ポスター発表

セッション記号 M (領域外・複数領域) » M-IS ジョイント

[M-IS27] 地球流体力学:地球惑星現象への分野横断的アプローチ

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)

[MIS27-P02] Axial flow characteristics of a liquid metal roll convection under a horizontal magnetic field

澤田 航希1、*田坂 裕司1柳澤 孝寿2,1村井 祐一1桜庭 中3 (1.北海道大学大学院工学研究院、2.海洋研究開発機構、3.東京大学地球惑星科学専攻)

キーワード:熱対流、磁場、流れの遷移

Magneto-convection is one of important flow systems for describing behavior of the earth’s outer core. It is well known that applying sufficiently strong horizontal magnetic field to thermal convection in a liquid metal layer stabilizes the convections into quasi-two-dimensional rolls aligned parallel to the magnetic field. The corresponding phenomena of convection rolls are, however, not so simple because of existence of side boundaries; pressure gradient nearby the wide wall perpendicular to the magnetic field causes axial flow due to Ekman pumping in Bödewadt layer. And, the flow provides complexity on the convection.
We examined axial flow and advection structures on quasi-two-dimensional convection rolls by laboratory experiment using liquid metal layer imposed by horizontal magnetic field. Ultrasonic velocity profiler visualized and quantified roll structures and axial flows by multiple measurement lines set in the fluid layer. The measurements were performed for different Rayleigh and Chandrasekhar numbers and variations of the axial flow velocity were investigated. Visualized flow pattern suggested influence of Lorenz force on the axial flow and scaling law with considering the Lorenz force effect was discussed.