Thin-jet scaling in large-scale shallow water quasigeostrophic flow

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS
B. H. Burgess
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引用次数: 1

Abstract

The evolution of thin frontal jets in large-scale shallow water quasigeostrophic flow is studied, with a focus on jet curvature and arclength. The flow is large-scale in the sense that mixed regions of potential vorticity (PV) are much larger than the deformation length . However the presence of sharp PV fronts with widths drives the ongoing growth of the flow's length scale; in particular the PV fronts and collocated jets support long undulations that facilitate jet interactions and the merger of mixed regions. The flow develops large dynamically active multilevel vortices containing two main mixed levels of PV, as well as small dynamically inactive vortices that persist for long times; these regions and their frontal jets display markedly different scaling properties. The frontal jets bounding the large dynamically active mixed regions follow power laws consistent with the scaling symmetries of the modified Korteweg-de Vries (mKdV) equation, which governs the motion of the jet axis in the thin-jet limit. These jets have population total arc length decaying approximately as , average arc length growing like , rms curvature as and typical curvature fluctuation as .
大尺度浅水准等转流中的薄射流结垢
研究了大尺度浅水准等转流中薄锋面射流的演化,重点研究了射流曲率和弧长。从位涡混合区比变形长度大得多的意义上说,流动是大规模的。然而,宽度较大的PV锋面的存在推动了气流长度尺度的持续增长;特别是PV锋面和并列的射流支持长波动,促进了射流的相互作用和混合区域的合并。气流发展出包含两个主要混合水平PV的大型动态活跃多层涡,以及持续时间较长的小型动态不活跃涡;这些区域及其锋面喷流表现出明显不同的标度特性。在大型动态活跃混合区域的前缘射流遵循与修正Korteweg-de Vries (mKdV)方程的标度对称性相一致的幂律,该幂律控制了薄射流极限下射流轴的运动。这些射流的总体弧长衰减近似为,平均弧长增长近似为,均方根曲率为,典型曲率波动为。
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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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