中尺度湍流对地形封闭盆地风驱动环流的影响

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS
L. Zavala Sansón
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引用次数: 2

摘要

本文研究了随时间变化的中尺度湍流对地形变化的封闭盆地中风驱动海洋环流的影响。对具有有限地形的单层流体在倾斜边界处进行了数值模拟。这种气流是由一种稳定的、盆地尺度的风(产生经典的西部增强的反气旋环流)和一种较短的、随时间变化的力(在较窄的尺度范围内注入能量)的适当组合所驱动的。这里考虑了两种截然不同的情况。首先,在没有大规模强迫的情况下,湍流产生了沿盆地周围地转等高线的气旋流。其次,研究了同时考虑大尺度和小尺度强迫条件下的平均环流。特别讨论了反气旋环流的改变可能是由湍流引起的气旋环流引起的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Effects of mesoscale turbulence on the wind-driven circulation in a closed basin with topography
This paper studies the effects of time-dependent, mesoscale turbulence on the wind-driven ocean circulation in a closed basin with variable topography. Numerical simulations of a single-layer fluid with finite topography at the sloping boundaries are performed. The flow is forced by a suitable combination of a steady, basin-scale wind that generates the classical western-intensified anticyclonic gyre, plus a shorter, time-dependent forcing that injects energy at a narrow range of scales. Two contrasting situations are considered. First, in the absence of the large-scale forcing, the turbulence generates a cyclonic flow that follows the geostrophic contours around the basin. Second, the resulting mean circulation is studied when the large and small-scale forcing terms are considered together. In particular, it is discussed that the alteration of the anticyclonic gyre may be due to the turbulent-induced cyclonic circulation.
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来源期刊
Geophysical and Astrophysical Fluid Dynamics
Geophysical and Astrophysical Fluid Dynamics 地学天文-地球化学与地球物理
CiteScore
3.10
自引率
0.00%
发文量
14
审稿时长
>12 weeks
期刊介绍: Geophysical and Astrophysical Fluid Dynamics exists for the publication of original research papers and short communications, occasional survey articles and conference reports on the fluid mechanics of the earth and planets, including oceans, atmospheres and interiors, and the fluid mechanics of the sun, stars and other astrophysical objects. In addition, their magnetohydrodynamic behaviours are investigated. Experimental, theoretical and numerical studies of rotating, stratified and convecting fluids of general interest to geophysicists and astrophysicists appear. Properly interpreted observational results are also published.
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