Simultaneous velocity and density measurements of fully developed Rayleigh-Taylor mixing

Mark Mikhaeil, Prasoon Suchandra, Devesh Ranjan, and Gokul Pathikonda
Phys. Rev. Fluids 6, 073902 – Published 19 July 2021

Abstract

The dynamics of molecular mixing and the energy transfer process in the Rayleigh-Taylor instability (RTI) are studied through the collection of simultaneous density-velocity measurements. These experiments provide simultaneous density-velocity field measurements, in contrast to previous point measurements. Statistically stationary experiments are performed in a “convective-type” gas tunnel facility, with density contrast achieved through the injection of helium into the bottom stream. Three experiments at Atwood number 0.1 are captured at three outer scale Reynolds numbers Re=520,2260, and 4050. Particle image velocimetry and laser induced fluorescence are employed simultaneously. Statistics of the density and velocity show self-similar collapse of RTI profiles at large Reynolds number Re>2000. Flat velocity profiles indicate homogeneous turbulence characteristics in the core of the mixing region. Significant anisotropy develops in the flow, with horizontal velocity fluctuations being only 60% of the vertical velocity fluctuations. The turbulent mass flux is found to be asymmetric about the centerline, with increased peak towards the spike. Measurements of the molecular mixing show that mixing is maximized at the core of the flow and increases with increased Reynolds number. The transport equation of density-specific-volume correlation b shows that it is mostly produced in the core of the mixing region, and that the spatial evolution of its profile is the result of transport by bulk motion of the bubble and spike. Energy transfer from gravitational potential energy to turbulent kinetic energy and viscous dissipation is observed to occur in the experiment with a ratio of dissipated energy to potential energy released of 38%. The analysis of the turbulent kinetic energy transport equation budget reveals that production is the primary mechanism towards the growth of turbulent kinetic energy in the core of the flow, and is asymmetrically slightly skewed towards the spike. However, it is through the transport that the strong advection at the edges of the mixing region is maintained.

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  • Received 15 December 2020
  • Accepted 24 June 2021

DOI:https://doi.org/10.1103/PhysRevFluids.6.073902

©2021 American Physical Society

Physics Subject Headings (PhySH)

Fluid Dynamics

Authors & Affiliations

Mark Mikhaeil*, Prasoon Suchandra2,*, and Devesh Ranjan2,†

  • George W. Woodruff School of Mechanical Engineering, Georgia Institute of Technology, 801 Ferst Drive, Atlanta, Georgia 30332, USA

Gokul Pathikonda

  • School for Engineering of Matter, Transport, and Energy, Arizona State University, 551 East Tyler Mall, Tempe, Arizona 85281, USA

  • *These authors contributed equally to the work.
  • devesh.ranjan@me.gatech.edu

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Issue

Vol. 6, Iss. 7 — July 2021

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