Abstract
The steady, axially symmetric, viscous, incompressible flow induced by an infinite rotating disk in the presence of a stationary coaxial disk is studied numerically for the complete laminar range of a Taylor number, R. Emphasis is placed on qualitative interpretation of the numerical solutions. The asymptotic state for large R is shown to consist of two well-known special Ekman boundary layers on the disks which are linked by a Taylor column, with Ekman layer suction into one layer just balanced by axial outflow from the other layer.
DOI: https://doi.org/10.3402/tellusa.v20i4.10047 | Journal eISSN: 3035-9554
Language: English
Page range: 667 - 672
Submitted on: Dec 28, 1967
Published on: Jan 1, 1968
Published by: Stockholm University Press
In partnership with: Paradigm Publishing Services
© 1968 Edward R. Benton, published by Stockholm University Press
This work is licensed under the Creative Commons Attribution 4.0 License.
