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Some remarks on the initiation of inertial Taylor columns

Published online by Cambridge University Press:  29 March 2006

Herbert E. Huppert
Affiliation:
Department of Applied Mathematics and Theoretical Physics, University of Cambridge

Abstract

The quasi-geostrophic flow over an obstacle placed on the lower of two horizontal planes in rapid rotation about the vertical z axis is considered. The flow field is calculated in the limit of vanishing viscosity after assuming the flow far upstream of the obstacle to be uniform, of magnitude V. The effects that occur in homogeneous flow are compared with those that occur in stratified flow.

If the flow is homogeneous, there is a region of closed streamlines if \[ h_0R^{-1} > \min_r\left[r\left/\int_0^r xh(x)dx\right. \right], \] where the obstacle is assumed to be cylindrically symmetric and given by z = Hh0h(r/L), H is the distance between the planes and R is the Rossby number V/(fL). For any obstacle the right-hand side of (1) is greater than zero and hence h0 must be positive for a closed-streamline region to occur. It is argued, and illustrated by a particular example, that because (1) involves an integral of h(x) a representative flow pattern can be obtained for obstacles of less than critical height by considering the special case of a flat-topped obstacle, as is done by Ingersoll (1969).

If the flow is stratified with constant Brunt-Väisälä frequency N, the condition for the existence of closed streamlines is shown to be \[ h_0R^{-1} > \min_r \left[B\int_0^{\infty}\int_0^{\infty}xt\cot h(Bt)h(x)J_0(tx)J_1(tr)\,dt\,dx \right]^{-1}, \] where B = NH/fL. In contrast to the homogeneous situation, the right-hand side of (2) can be zero and is so if the obstacle is somewhere vertical. Such obstacles will produce a closed-streamline region no matter now small their height and will hence not lead to patterns representative of smooth obstacles. This is because a stratified column of fluid cannot be stretched or compressed over an infinitesimal distance. Instead, the column bends markedly and the fluid flows around the obstacle. The critical conditions (1) and (2) for a number of specific obstacles are calculated and discussed.

Type
Research Article
Copyright
© 1975 Cambridge University Press

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References

Batchelor, G. K. 1956 On steady laminar flow with closed streamlines at large Reynolds number. J. Fluid Mech., 1, 177190.Google Scholar
Bretherton, F. P. 1967 The time-dependent motion due to a cylinder moving in an unbounded rotating or stratified fluid. J. Fluid Mech., 28, 545579.Google Scholar
Goody, R. M. 1969 Motions in the atmosphere of Jupiter. Comm. Astrophys. Space Phys., 1, 1932.Google Scholar
Hide, R. 1961 Origin of Jupiter's Great Red Spot. Nature, 190, 895896.Google Scholar
Hide, R. & Ibbetson, A. 1966 An experimental study of ‘Taylor columns’. Icarus, 5, 279290.Google Scholar
Hide, R. & Ibbetson, A. 1968 On slow transverse flow past obstacles in a rapidly rotating fluid. J. Fluid Mech., 32, 251272.Google Scholar
Hogg, N. G. 1973 The preconditioning phase of MEDOC 1969. Part II: topographic effects. Deep-sea Res., 20, 449459.Google Scholar
Huppert, H. E. & Stern, M. E. 1974 Ageostrophic effects in rotating stratified flow. J. Fluid Mech., 62, 369385.Google Scholar
Ingersoll, A. P. 1969 Inertial Taylor columns and Jupiter's Great Red Spot. J. Atmos. Sci., 26, 744752.Google Scholar
Jacobs, S. J. 1964 The Taylor column problem. J. Fluid Mech., 20, 58191.Google Scholar
Miles, J. W. & Huppert, H. E. 1969 Lee waves in a stratified flow. Part 4. Perturbation approximations. J. Fluid Mech., 35, 497525.Google Scholar
Phillips, N. A. 1969 Geostrophic motion. Rev. Geophys., 1, 123176.Google Scholar
Proudman, J. 1916 On the motion of solids in a liquid possessing vorticity. Proc. Roy. Soc. A 92, 408424.Google Scholar
Stewartson, K. 1952 On the slow motion of a sphere along the axis of a rotating fluid. Proc. Camb. Phil. Soc., 48, 168177.Google Scholar
Stone, P. H. & Baker, D. J. 1968 Concerning the existence of Taylor columns in atmospheres. Quart. J. Roy. Met. Soc., 94, 576580.Google Scholar
Swallow, J. C. & Caston, G. F. 1973 The preconditioning phase of MEDOC 1969. Part I: observations. Deep-sea Res., 20, 429448.Google Scholar
Szoeke, R. A. De 1972 Baroclinic flow over an obstacle in a rotating system. Woods Hole Ocean. Inst. G.F.D. Notes, no. 2, pp. 110.Google Scholar
Taylor, G. I. 1917 Motion of solids in fluids when the flow is not irrotational. Proc. Roy. Soc. A 93, 99113.Google Scholar
Taylor, G. I. 1923 Experiments on the motion of solid bodies in rotating fluids. Proc. Roy. Soc. A 106, 213218.Google Scholar
Wheelon, A. D. 1968 Tables of Summable Series and Integrals Involving Bessel Functions. Holden-Day.