Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-29T17:28:09.384Z Has data issue: false hasContentIssue false
  • English
  • Français

Summary-Introduction: Similarity arguments for fully developed turbulence

Published online by Cambridge University Press:  19 March 2018

W. V. R. Malkus
W. V. R. Malkus*
Affiliation:
Woods Hole Oceanographic Institution - Woods Hole, Mass.

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

In the study of turbulent flows similarity arguments are used to explore the consequences of non-mechanistic assertions concerning the general behavior of the flow. For example, it is currently assumed that viscosity plays no role in the determination of the mean velocity profile of turbulent shearing flow far from a boundary. The consequences of this assumption are that the amplitude of the mean velocity will be determined by the momentum transported into such a region and that the velocity profile will be a solution to Euler's equations.

Type
Part IV. Considerations on Localized Velocity Fields in Stellar Atmospheres: Prototype — The Solar Atmosphere
Information
Symposium - International Astronomical Union , Volume 12: Aerodynamic Phenomena in Stellar Atmospheres , 1960 , pp. 376 - 384
Copyright
Copyright © Italian physical society 1960 

References

Laufer, J., 1950, Nat. Adv. Comm. Aero. , Wash., MO. 2123.Google Scholar
Malkus, W. V. R., 1954, Proc. Boy. Soc., A 225, 196.Google Scholar
Malkus, W. V. R., 1956, J. Fluid Mech. , 2, 521.CrossRefGoogle Scholar
Priestley, C. H. B., 1954, Austral. J. Phys. , 7, 176.Google Scholar
Townsend, A. A., 1958, The Structure of Turbulent Shear Flow (Cambridge).Google Scholar
Townsend, A. A., 1959, J. Fluid Mech. , 5, 209.Google Scholar