Abstract

We report experimental and theoretical results on how a fluid (homogeneous or continuously stratified) is spun up in a closed, semicircular cylinder. Experiments were performed for Rossby numbers $Ro=0.02$, 0.2 and 1 (the latter corresponding to the limiting case of spin-up from rest), with the Ekman number $E=O({10^{-5}})$, and the Burger number ($S$) varied between 0 and 10. There are two key processes: Ekman pumping that drives the core flow; and the formation and breakdown of the vertical-wall boundary layers, with respective characteristic time scales $t\sim E^{-1/2}$ and $Ro^{-1}$. When these time scales are comparable, the observed flow is dominated by the gradual spin-up of the initial anticyclone that forms when the rotation rate is increased, which fills the container's interior; vorticity generated adjacent to the vertical walls throughout remains confined to the neighbourhood of the container's walls and corners. Conversely, when ${E^{1/2}/Ro\ll 1}$, the vertical-wall boundary layers rapidly break down, resulting in the formation of cyclonic vortices in the container's vertical corners, which grow and interact with the initial anticyclone, leading to the formation of a three-cell flow pattern. For $Ro=0.02$, our theoretical description of the flow generally agrees well with experiments, and the computation of the eruption times for the unsteady boundary layers is consistent with the observations for both $Ro=0.02$ and $Ro=0.2$.

Highlights

  • Spin-up problems have been studied extensively and are mostly associated with how a bounded rotating fluid adjusts from one state of solid-body rotation to another, due to an increase in rotation rate of the confining boundaries

  • Howard (1963) described axisymmetric spin-up of a homogeneous fluid in the linear regime, i.e. for small Rossby number, Ro = ΔΩ/Ω, where Ω − ΔΩ and Ω are the initial and final angular frequencies, respectively. They showed that spin-up is driven by a meridional circulation that forms in the interior of the fluid column due to the Ekman boundary layers that form at the horizontal confining boundaries

  • The Ekman layers transport spun-up fluid radially outwards, which is replaced by a vertical flux from the inviscid interior

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Summary

Introduction

Spin-up problems have been studied extensively and are mostly associated with how a bounded rotating fluid adjusts from one state of solid-body rotation to another, due to an increase in rotation rate of the confining boundaries. One study of note is that by Foster & Munro (2012), who reported an asymptotic theory, valid for Ro E1/2 1, to describe linear spin-up in a regular square container They showed that the formation of cyclonic vortices in the container’s vertical corner regions – due to the breakdown of the sidewall boundary layers – occurs on the time scale Ro−1Ω−1, and so is of less significance in the linear regime. In a subsequent study of nonlinear spin-up in a regular square container, Munro et al (2015) showed the sidewall Prandtl boundary layers do break down at a finite time of order Ro−1Ω−1 following an impulsive change in rotation rate, which leads to the formation of cyclonic vortices in the container’s vertical corner regions.

Apparatus and set-up
Measurements and notation
Observations for Ro = 1 (nonlinear, spin-up from rest)
Short-time behaviour
Flow development on the spin-up time scale
Numerical, unsteady solution
A limiting case: S → 0
Sidewall boundary layers
Composite solutions
Final remarks
Findings
Steady-state solution
Full Text
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