Scales of vertical motions due to an isolated vortex in ageostrophic balanced flows

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2023-10-24 DOI:10.1080/03091929.2023.2262100
William J. McKiver
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Abstract

AbstractHere we consider a model of an isolated vortex to understand the vertical dynamics induced by mesoscale eddies in the ocean. We use the analytical solutions to a balanced model for an ellipsoid of uniform potential vorticity to examine how the vertical motions induced depend on the vortex shape and its orientation, i.e. whether the vortex is vertically upright or tilted with respect to the vertical axis. The motion induced by the vortex can be divided into two kinds: (1) the interior flow which acts on the vortex itself and (2) the exterior flow which acts on its surroundings. For an upright ellipsoid, there are no self-induced vertical motions and the vortex rotates steadily about the vertical axis. However, for a tilted ellipsoid we find solutions exist where the vortex rotates about the vertical axis, while the vertical motions cause the tilt angle of the vortex to oscillate. This effect is stronger as the tilt angle is increased. Considering the exterior flow, there exists an exterior vertical velocity for the upright and tilted ellipsoids. However, the dynamics induced by the exterior vertical velocity is very different for the upright and tilted cases. We find that for an upright ellipsoidal vortex, the vertical motions are largest for vortices with high horizontal eccentricity and a vertical height-to-width aspect ratio near unity, vanishing as the horizontal cross-section of the vortex becomes circular. Instead for the tilted case, the vertical motions are largest when the horizontal cross section is circular, and for strongly prolate vortices, with the largest vertical motions occurring when the tilt angle is 45∘.Keywords: Vortexgeophysicalbalancedvertical motions Disclosure statementNo potential conflict of interest was reported by the author(s).
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地转平衡流中由孤立涡旋引起的垂直运动尺度
在这里,我们考虑了一个孤立涡旋模型来理解海洋中尺度涡旋诱导的垂直动力学。我们使用平衡模型的解析解为一个均匀位涡椭球来研究如何诱导垂直运动取决于涡的形状和它的方向,即涡是垂直直立或倾斜相对于垂直轴。涡旋引起的运动可分为两种:(1)作用于涡旋本身的内部流动和(2)作用于其周围环境的外部流动。对于垂直椭球体,不存在自激垂直运动,旋涡沿垂直轴稳定旋转。然而,对于倾斜椭球,我们发现存在这样的解,即涡旋绕垂直轴旋转,而垂直运动导致涡旋的倾斜角振荡。这种效果随着倾斜角度的增加而增强。考虑外流,竖直和倾斜椭球均存在外垂直速度。然而,在垂直和倾斜情况下,由外垂直速度引起的动力学是非常不同的。我们发现,对于垂直椭球形涡来说,高水平偏心率和垂直高宽比接近1的涡的垂直运动最大,随着涡的水平截面变为圆形而消失。相反,在倾斜的情况下,当水平横截面为圆形时垂直运动最大,而对于强烈的长旋涡,当倾斜角度为45°时垂直运动最大。关键词:涡旋地球物理平衡垂直运动披露声明作者未报告潜在利益冲突。
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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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