The role of boundary conditions in the simulation of rotating, stratified turbulence

Citation
Dg. Dritschel et C. Macaskill, The role of boundary conditions in the simulation of rotating, stratified turbulence, GEOPH ASTRO, 92(3-4), 2000, pp. 233-253
Citations number
18
Categorie Soggetti
Space Sciences
Journal title
GEOPHYSICAL AND ASTROPHYSICAL FLUID DYNAMICS
ISSN journal
03091929 → ACNP
Volume
92
Issue
3-4
Year of publication
2000
Pages
233 - 253
Database
ISI
SICI code
0309-1929(2000)92:3-4<233:TROBCI>2.0.ZU;2-G
Abstract
In this paper we use the CASL method to explore the role of boundary condit ions in determining the long-time behaviour of rotating, stratified, quasi- geostrophic turbulence. We End that initially two-dimensional (sufficiently tall) columns of potential vorticity (PV) break down through three-dimensi onal instability to give a fully three-dimensional dow consisting of ellips oidal structures. This is the case both for rigid-lid (isothermal) vertical boundary conditions and for vertically periodic boundaries. However, the r igid boundary case gives rise to semi-ellipsoids at both the top and bottom boundaries, and, for sufficient domain depths, preferred depths for the fo rmation of ellipsoids in the interior. By contrast, in the vertically perio dic case, the distribution of ellipsoids is homogeneous in depth. The role of the horizontal boundaries is indirect, but still significant. I n all cases doubly periodic horizontal boundary conditions are imposed. We consider a range of initial conditions where in each case equal numbers of two-dimensional columns of positive and negative vorticity are used, taking up a fixed, but relatively small fraction of the domain (approximately 5%) . Thus when there is only a small number of vortices, they have larger radi us. When the initial number of vortices is small enough (i.e., when the rad ius is not small compared with the horizontal domain width), at long time t here is a two-dimensionalisation giving rise to a single column of positive PV and a single column of negative PV, as has been observed in some previo us simulations. We find the same phenomenon for both vertically periodic an d rigid lid boundary conditions, but it occurs over a broader range of init ial conditions in the vertically periodic case. However, in all cases fully three-dimensional final states are regained when the number of vortices is increased while keeping the fraction of the domain occupied by vortices fi xed, i.e., when the vortex radius/domain width ratio is sufficiently small.