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Abstracts - KTH Mechanics

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24<br />

Beta-plane turbulence in a basin with no-slip boundaries<br />

W. Kramer ∗ , H.J.H. Clercx ∗ and G.J.F. van Heijst ∗<br />

On a domain enclosed by no-slip boundaries, two-dimensional, geostrophic flows<br />

have been studied by numerical simulations of the Navier-Stokes equation with the<br />

beta-plane approximation at intermediate Reynolds numbers and a range of values<br />

for beta 1 . While most of the results are in agreement with other studies which use<br />

different boundary conditions, some aspects show a different and unexpected behavior.<br />

Without the beta-plane the flow is characterized by the formation of a single domainsized<br />

coherent vortex due to the inverse energy cascade. From the simulations with<br />

the presence of the beta-effect it can be observed that the inverse cascade is clearly<br />

impeded by the presence of a beta-plane. This leads to a refinement of the flow<br />

structures (Figure 1a), which scales are in agreement with the Rhines scale. When<br />

the growing flow scales reach sizes comparable with the Rhines scale, the beta-effect<br />

becomes dynamically more important than advection and, consequently, the Rossby<br />

wave mechanism takes over from the inverse cascade. The arrest of the inverse cascade<br />

is visible as a plateau for wave numbers smaller than the Rhines wave number (Figure<br />

1b). On a closed domain Rossby waves are described by basin modes, which are<br />

solutions of the inviscid flow equation on a bounded domain with free-slip boundaries.<br />

Frequency spectra of the flow profoundly exhibit the existence of basin modes, which<br />

excitation is favoured above the formation of vortices. The presence and apparent<br />

stability of basin modes on a domain with no-slip boundaries is a rather surprising<br />

observation, because these modes are solutions of the inviscid equations. The timemean<br />

flow in forced simulations shows a zonal band structure (Figure 1c) which<br />

resembles the flow on a periodic domain (although the kinetic energy of the mean<br />

flow represents only 2-4% of the kinetic energy of the turbulent flow field itself). This<br />

a rather surprising result as numerous other simulations show a mean flow consisting<br />

of a dual gyre on a closed domain. The difference can be subscribed solely to the<br />

applied no-slip boundary conditions.<br />

∗ Fluid Dynamics Laboratory, Eindhoven University of Technology, The Netherlands.<br />

1 W. Kramer et al., Phys. Fluids, accepted for publication.<br />

<br />

a<br />

b<br />

<br />

c<br />

k -5/3 k -3<br />

<br />

<br />

<br />

E(k)<br />

<br />

<br />

<br />

<br />

<br />

kRhines<br />

kf<br />

k<br />

<br />

Figure 1: The stream function for the time dependent flow field (a) the 1D Chebyshev<br />

spectrum of the kinetic energy (b) and the time averaged stream function (c) .

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