日本地球惑星科学連合2019年大会

講演情報

[E] 口頭発表

セッション記号 A (大気水圏科学) » A-OS 海洋科学・海洋環境

[A-OS09] 海洋混合学:物質循環・気候・生態系の維持と長周期変動の解明

2019年5月27日(月) 15:30 〜 17:00 301B (3F)

コンビーナ:安田 一郎(東京大学大気海洋研究所)、日比谷 紀之(東京大学大学院理学系研究科地球惑星科学専攻)、西岡 純(北海道大学低温科学研究所)、伊藤 進一(東京大学大気海洋研究所)、座長:日比谷 紀之(東京大学 大学院理学系研究科 地球惑星科学専攻)

16:15 〜 16:30

[AOS09-21] Revisiting the Characteristics of Mixing Efficiency in the Brazil Basin

*伊地知 敬1Louis St. Laurent1Kurt Polzin1 (1.ウッズホール海洋研究所)

It is still controversial whether or not the dissipation flux coefficient Γ, often referred to as the “mixing efficiency”, is a global constant of 0.2. A primary justification for continuing to use this conventional value comes from a number of dedicated tracer-release/microstructure surveys done over the past three decades. Most notably, studies in the Brazil Basin have been the basis for examining the characteristics of mixing in the abyssal interior of the global ocean. Here, using recent microstructure data also collected in the Brazil Basin, we revisit the characteristics of Γ in the abyssal interior. It is shown that Γ, estimated from averaged profiles of the TKE dissipation rate and the thermal variance dissipation rate, actually lies around 0.2 in the pycnocline, but on the other hand, it tends to increase up to 0.4-0.8 toward the bottom. Such near-bottom high efficiency appears to be associated with weak stratification in the bottom water. Furthermore, one microstructure profile appears to reach down to within the thin bottom boundary layer: Γ abruptly decreases to O(10-2) within 50 m above the bottom, which is reasonable given the no buoyancy flux condition at the bottom. We will also examine these results using the earlier generation microstructure datasets collected in the Brazil Basin.