Regional Abyssal Vorticity Balance in the Northeast South China Sea: External and Internal Dynamics of Abyssal Circulation

IF 2.8 2区 地球科学 Q1 OCEANOGRAPHY Journal of Physical Oceanography Pub Date : 2023-11-15 DOI:10.1175/jpo-d-23-0060.1
Hua Zheng, X. Zhu, Min Wang, Juntian Chen, Feng Nan, F. Yu
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Abstract

Abyssal vorticity balance in the northeast South China Sea was assessed for over a year based on observations from 28 current- and pressure-recording inverted echo sounders distributed west of the Luzon Strait. The regional first-order balance was dominated by the planetary vorticity flux and bottom pressure torque, which reflect the external and internal dynamics of abyssal circulation. Vertical motion considerably contributed to the planetary vorticity flux, whereas the contribution of horizontal motion was negligible. Positive and negative planetary vorticity fluxes dominate the areas along the eastern and western boundaries, indicating upward and downward vertical transport, respectively. The opposite planetary vorticity fluxes in the different areas were accompanied by different current patterns; regional anticyclonic and cyclonic characteristics appeared near the western and eastern boundaries, respectively, owing to the deep topography as the abyssal current followed the boundary. The planetary vorticity flux near the eastern boundary was substantial in spring and autumn; in contrast, along the western boundary it was enhanced only in spring. Deep eddies played important roles in planetary vorticity flux and regional vorticity balance. The results of this study reveal the formation dynamics of abyssal circulation in the South China Sea as well as its spatiotemporal distributions, providing a more detailed description of abyssal circulation.
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南海东北部的区域深海涡度平衡:深海环流的外部和内部动力
根据分布在吕宋海峡以西的 28 个海流和压力记录倒置回声探测仪的观测结果,对南海东北部一年多的深海涡度平衡进行了评估。区域一阶平衡由行星涡度通量和底压扭矩主导,它们反映了深海环流的外部和内部动态。垂直运动对行星涡度通量的贡献很大,而水平运动的贡献可以忽略不计。正负行星涡度通量在东部和西部边界沿线占主导地位,分别表示向上和向下的垂直传输。不同地区相反的行星涡度通量伴随着不同的海流模式;由于深海海流沿边界流动,深海地形使西部和东部边界附近分别出现了区域性反气旋和气旋特征。东部边界附近的行星涡度通量在春季和秋季显著增加;相比之下,西部边界附近的行星涡度通量仅在春季增加。深涡在行星涡度通量和区域涡度平衡中发挥了重要作用。该研究结果揭示了南海深海环流的形成动力学及其时空分布,为更详细地描述深海环流提供了依据。
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来源期刊
CiteScore
2.40
自引率
20.00%
发文量
200
审稿时长
4.5 months
期刊介绍: The Journal of Physical Oceanography (JPO) (ISSN: 0022-3670; eISSN: 1520-0485) publishes research related to the physics of the ocean and to processes operating at its boundaries. Observational, theoretical, and modeling studies are all welcome, especially those that focus on elucidating specific physical processes. Papers that investigate interactions with other components of the Earth system (e.g., ocean–atmosphere, physical–biological, and physical–chemical interactions) as well as studies of other fluid systems (e.g., lakes and laboratory tanks) are also invited, as long as their focus is on understanding the ocean or its role in the Earth system.
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