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Ocean Management, 1981
Abstract The pattern of flow in a tidal estuary is largely determined by the vertical transport of momentum and density due to turbulence. In a well-mixed estuary the turbulent mixing throughout the depth is dominated by turbulence associated with friction at the bed, although the effect of shear at mid-depth due to the density driven residual flow ...
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Abstract The pattern of flow in a tidal estuary is largely determined by the vertical transport of momentum and density due to turbulence. In a well-mixed estuary the turbulent mixing throughout the depth is dominated by turbulence associated with friction at the bed, although the effect of shear at mid-depth due to the density driven residual flow ...
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The Physics of Fluids, 1965
The radial pressure gradient in combination with either a positive or negative radial gradient of angular momentum makes possible the realization of two dynamically different flows. When the angular momentum gradient is positive, the flow is stable; when it is negative, the flow is unstable.
D.P. Margolis, J. L. Lumley
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The radial pressure gradient in combination with either a positive or negative radial gradient of angular momentum makes possible the realization of two dynamically different flows. When the angular momentum gradient is positive, the flow is stable; when it is negative, the flow is unstable.
D.P. Margolis, J. L. Lumley
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2002
In this paper, we study turbulent mixing with sprays using a low Mach number DNS code coupled with a Lagrangian solver. We investigate the impact of turbulence on the spray dispersion, and its consequence on the global vaporization rates of the whole spray.
Rafik Ben Dakhlia +3 more
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In this paper, we study turbulent mixing with sprays using a low Mach number DNS code coupled with a Lagrangian solver. We investigate the impact of turbulence on the spray dispersion, and its consequence on the global vaporization rates of the whole spray.
Rafik Ben Dakhlia +3 more
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AIP Conference Proceedings, 2005
Turbulent mixing layers have been proposed to explain observations of line ratios of highly ionized elements in the interstellar medium. We present preliminary results of numerical simulations of turbulent mixing layers in a magnetized medium. We developed a MHD code with radiative cooling.
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Turbulent mixing layers have been proposed to explain observations of line ratios of highly ionized elements in the interstellar medium. We present preliminary results of numerical simulations of turbulent mixing layers in a magnetized medium. We developed a MHD code with radiative cooling.
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Layering, Instabilities, and Mixing in Turbulent Stratified Flows
Annual Review of Fluid Mechanics, 2021Colm-cille Caulfield
exaly