日本地球惑星科学連合2022年大会

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-IS21] 地球流体力学:地球惑星現象への分野横断的アプローチ

2022年6月1日(水) 11:00 〜 13:00 オンラインポスターZoom会場 (31) (Ch.31)

コンビーナ:伊賀 啓太(東京大学大気海洋研究所)、コンビーナ: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)、コンビーナ:相木 秀則(名古屋大学)、座長:伊賀 啓太(東京大学大気海洋研究所)

11:00 〜 13:00

[MIS21-P02] Emergence of longitudinal roll structures in horizontal convection under non-uniform heating

*能登 大輔1,2田坂 裕司1柳澤 孝寿3宮腰 剛広3 (1.北海道大学、2.ペンシルバニア大学、3.海洋研究開発機構)

キーワード:水平対流、成層流れ

Since a baroclinic adjustment induces a convective flow even with a presence of a weak horizontal temperature gradient, heat is exchanged horizontally resulting in a global circulating flow. This phenomenon is called horizontal convection, and it is one of the key phenomena present in natural systems as well as in industrial applications. In the case of horizontal convection under a stably stratified system, i.e., non-uniform heating/cooling from top/bottom, the convective flow is confined to a shallow region at the vicinity of the horizontal wall with the non-uniform temperature. Due to the shallow roll structure, strong shear is induced on the wall. Meanwhile, the downstream (longitudinal) flow is accompanied by a heated fluid, and it goes immediately beneath the cooler wall. These two effects yield formations of roll structures having axes in the longitudinal direction when the horizontal temperature gradient is sufficiently strong. A similar three-dimensional structure is often considered in a forced boundary condition, such as a condition with wind, and it is known as horizontal convective rolls. We study the details of the longitudinal roll structures that emerged spontaneously in horizontal convection confined in a rectangular box throughout laboratory experiments.