Hostname: page-component-cd9895bd7-dzt6s Total loading time: 0 Render date: 2024-12-17T22:41:49.788Z Has data issue: false hasContentIssue false

Thermally driven motions in a rotating stratified fluid: theory and experiment

Published online by Cambridge University Press:  25 May 1997

J. PEDLOSKY
Affiliation:
Physical Oceanography Department, Woods Hole Oceanographic Institution, Woods Hole, MA 02543, USA
J. A. WHITEHEAD
Affiliation:
Physical Oceanography Department, Woods Hole Oceanographic Institution, Woods Hole, MA 02543, USA
GRAHAM VEITCH
Affiliation:
Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Silver Street, Cambridge CB3 9EW, UK

Abstract

A radial temperature distribution is applied to the top of a cylinder of rotating stably stratified fluid. Thermal wind shear drives the interior flow. Linearized theory predicts, and laboratory experiments confirm, that when the stratification is large enough it completely suppresses the Ekman pumping into the interior. The interior velocity field, which is primarily azimuthal, responds by satisfying the no-slip boundary conditions without the need of Ekman layers on the horizontal surfaces. Moreover, for large stratification a thermal boundary layer beneath the top surface traps the thermal disturbance applied at the upper surface. The greatest azimuthal velocity occurs at the base of this layer. Below this layer the azimuthal velocity viscously diffuses downward with thermal wind adjusting the temperature. The Rossby radius of deformation based on this layer depth is the cylinder's radius divided by the square root of the Prandtl number. Detailed measurements of the velocity field generated in the cylinder by the heating are compared with the theory in the case where the Ekman layers are eliminated by stratification. The theory and experiments agree qualitatively well over a range of four orders of magnitude of imposed parameters and over a large parameter range the quantitative comparison is also very good.

Type
Research Article
Copyright
© 1997 Cambridge University Press

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)