Geostrophic Turbulence, Stable Baroclinic Eddies, and Self-Exciting Dynamos in Rotating Fluid Systems: A Summary

1994 ◽  
Vol 268 ◽  
pp. 211-229 ◽  
Author(s):  
Keke Zhang

It has been suggested that in a rapidly rotating fluid sphere, convection would be in the form of slowly drifting columnar rolls with small azimuthal scale (Roberts 1968; Busse 1970). The results in this paper show that there are two alternative convection modes which are preferred at small Prandtl numbers. The two new convection modes are, at leading order, essentially those inertial oscillation modes of the Poincaré equation with the simplest structure along the axis of rotation and equatorial symmetry: one propagates in the eastward direction and the other propagates in the westward direction; both are trapped in the equatorial region. Buoyancy forces appear at next order to drive the oscillation against the weak effects of viscous damping. On the basis of the perturbation of solutions of the Poincaré equation, and taking into account the effects of the Ekman boundary layer, complete analytical convection solutions are obtained for the first time in rotating spherical fluid systems. The condition of an inner sphere exerts an insignificant influence on equatorially trapped convection. Full numerical analysis of the problem demonstrates a quantitative agreement between the analytical and numerical analyses.


1991 ◽  
Vol 225 ◽  
pp. 241-270 ◽  
Author(s):  
L. M. Polvani

The process of alignment, a new fundamental interaction between vortices in a stratified and rapidly rotating fluid, is defined and studied in detail in the context of the two-layer quasi-geostrophic model. Alignment occurs when two vortices in different density layers coalesce by reducing their horizontal separation. It is found that only vortices whose radii are comparable with or larger than the Rossby deformation radius can align. In the same way as the merger process (in a single two-dimensional layer) is related to the reverse energy cascade of two-dimensional turbulence, geostrophic potential vorticity alignment is related the barotropic-to-baroclinic energy cascade of geostrophic turbulence in two layers. It is also shown how alignment is intimately connected with the existence of two-layer doubly connected geostrophic potential vorticity equilibria (V-states), for which the analysis of the geometry of the stream function in the corotating frame is found to be a crucial diagnostic. The finite-area analogues of the hetons of Hogg & Stommel (1985) are also determined: they consist of a propagating pair of opposite-signed potential vorticity patches located in different layers.


1983 ◽  
Vol 126 ◽  
pp. 315-333 ◽  
Author(s):  
Stuart C. Dickinson ◽  
Robert R. Long

Experiments were performed to investigate some aspects of turbulence in rotating and non-rotating fluid systems where the turbulence was induced by a horizontal grid oscillating vertically. An earlier theory by the second author made use of a planar source of energy, which appeared to be similar to the energy source of the grid, in determining the characteristics of the turbulence at points some distance away. The simplicity of the theory was in the parameterization of the grid ‘action’ by a single quantity K, with dimensions and characteristics of eddy viscosity.The experimental results provide additional confirmation of the theory in the non-rotating case, and indicate the usefulness of the idealized energy source in the rotating case. In the latter, we measured the propagation of the front separating disturbed and undisturbed fluid, moving along the axis of rotation. The thickness d(t) of the disturbed region increases at first as (Kt)½, as in a non-rotating fluid, until the Rossby number K/Ωd2k becomes of order unity.Beyond this the disturbances are wavelike and rotationally dominated, and the thickness now increases linearly with time, yielding a speed of propagation for the front proportional to the wave speed (KΩ)½. Finally, the disturbances reach the bottom and the vessel is in statistical steady state. Then a region of thickness dk independent of time is found, and it contains motion that resembles ordinary, three-dimensional turbulence. dk ∼ (K/Ω)½ is analogous to the depth of the turbulent Ekman layer H ∼ (K/Ω)½, where K is taken as an eddy viscosity.McEwan constructed a similar rotating experiment, although with a different energy source, and observed vortices parallel to the axis of rotation, provided that the Rossby number was less than a critical value. Our observations and theory indicate that the disappearance of the vortices corresponds to h < dk, where h is the total depth of the fluid. At that point, the whole tank is filled with three-dimensional turbulence.


1966 ◽  
Vol 26 (2) ◽  
pp. 393-410 ◽  
Author(s):  
F. P. Bretherton ◽  
G. F. Carrier ◽  
M. S. Longuet-Higgins

A symposium on ‘Rotating fluid systems’ was held at La Jolla, California, from 28 March to 1 April 1966. The meeting was organized under the auspices of the International Union of Theoretical and Applied Mechanics, and took place at the Institute of Geophysics and Planetary Physics of the University of California. There were 75 participants, and attendance was by invitation. The subjects discussed included steady flows, both thermally driven and non-thermal; transient motions and instabilities; planetary waves and gravity waves affected by rotation; inertial oscillations; and hydromagnetic flows relating to the Earth's interior. The following is a brief account of the proceedings as seen by the authors. No formal volume of the papers presented is to be published, but references to published or unpublished work are given at the end of this article.


2010 ◽  
Vol 22 (1) ◽  
pp. 011701 ◽  
Author(s):  
Ligang Li ◽  
Xinhao Liao ◽  
Kit H. Chan ◽  
Keke Zhang

Tellus ◽  
1973 ◽  
Vol 25 (3) ◽  
pp. 233-246 ◽  
Author(s):  
H. Leonard Steinberg

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