日本地球惑星科学連合2021年大会

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[J] 口頭発表

セッション記号 A (大気水圏科学) » A-CG 大気海洋・環境科学複合領域・一般

[A-CG38] 海洋と大気の波動・渦・循環の力学

2021年6月6日(日) 10:45 〜 12:15 Ch.10 (Zoom会場10)

コンビーナ:田中 祐希(福井県立大学 海洋生物資源学部)、青木 邦弘(国立研究開発法人 海洋研究開発機構)、久木 幸治(琉球大学)、杉本 憲彦(慶應義塾大学 法学部 日吉物理学教室)、座長:青木 邦弘(国立研究開発法人 海洋研究開発機構)、久木 幸治(琉球大学)、田中 祐希(福井県立大学 海洋生物資源学部)

11:30 〜 11:45

[ACG38-04] Impacts of bottom topography on the formation of the North Pacific subtropical-subarctic frontal zone

*三寺 史夫1、芦田 隼人2、美山 透3 (1.北海道大学低温科学研究所、2.北海道大学大学院環境科学院、3.海洋研究開発機構)

キーワード:亜熱帯ー亜寒帯循環境界、天皇海山、移行領域、準定常ジェット

The subtropical-subarctic frontal zone in the North Pacific exhibits a complex water mass structure because the water of Kuroshio origin and the water of Oyashio origin are confluent, stirred there and mixed. Despite this complexity, two quasi-stationary fronts form in this region that characterize the frontal zone, which are the subarctic front (SAF), recognized by potential temperature of 4 ℃ contour at a depth of 100 m, and the subarctic boundary (SAB), recognized by salinity of 34 contour at a depth of 100 m; the so-called transition domain forms in between. This frontal zone is generally considered as a wind-driven gyre boundary between the subtropical and subarctic gyres. However, the frontal zone is located around 40 °N, which is further south than the location of the Sverdrup gyre boundary that forms at approximately ~45 °N. Here, we study the effects of bottom topography on the formation of the subtropical-subarctic frontal zone in the western North Pacific, with a particular attention to the Emperor Seamounts. We conducted an eddy-resolving two-layer modeling with a realistic topography of the ETOPO1, forced by a zonally-averaged wind stress derived from the JRA-55 do. The model exhibits a realistic frontal zone structure of the North Pacific comprising the SAF and SAB, as well as the transition domain. Eddy driven bottom currents are generated over topography, which in turn causes substantial impacts on the formation of upper layer frontal-zone structures. By conducting topography on/off experiments, we found that the Emperor Seamounts bring the subarctic thin layer southward across the Sverdrup gyre boundary. The thinner layer of the subarctic origin and thicker layer of the subtropical origin meet and mix there, leading to the formation of the SAB and the transition domain.