Non-self-similar viscous gravity currents

Bruce R. Sutherland, Kristen Cote, Youn Sub (Dominic) Hong, Luke Steverango, and Chris Surma
Phys. Rev. Fluids 3, 034101 – Published 15 March 2018
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Abstract

Lock-release experiments are performed focusing upon the evolution of near-pure glycerol flowing into fresh water. If the lock height is sufficiently tall, the current is found to propagate for many lock lengths close to the speed predicted for energy-conserving moderately non-Boussinesq gravity currents. The current then slows to a near stop as the current head ceases to be elevated relative to its tail and the current as a whole forms a wedge shape. By contrast, an experiment of near-pure glycerol advancing under air exhibits the well-known slowing of the current such that the front position increases as a one-fifth power of time. The evolution of a viscous gravity current in water is also qualitatively different from that for a high-Reynolds number gravity current which transitions smoothly from a constant speed to self-similar to viscous regime. The reason a viscous gravity current flowing under water moves initially at near-constant speed is not due to a lubrication layer forming below the current. Rather it is due to the return flow of water into the lock establishing a current with an elevated head that is taller than the viscous boundary layer depth near the current nose. The flow near the top of the head advances to the nose where it comes into contact with the tank bottom. Meanwhile the ambient fluid is pushed up and over the head rather than being drawn underneath it. The front slows rapidly to a near stop as the head height reduces to that comparable to the boundary layer depth underneath the head. The initial speed and entrainment into the current are shown to depend upon the ratio, R, of the starting current height to the characteristic boundary layer depth. In particular, entrainment via the turbulent shear flow over the head is found to increase the volume by less than 10% during its evolution if R10 but increases by as much as 100% for high-Reynolds number gravity currents. A conceptual model is developed that captures the transition from an inertially driven current to its sudden near stop by viscous forces.

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  • Received 2 November 2017

DOI:https://doi.org/10.1103/PhysRevFluids.3.034101

©2018 American Physical Society

Physics Subject Headings (PhySH)

Fluid Dynamics

Authors & Affiliations

Bruce R. Sutherland1,2,*, Kristen Cote1,†, Youn Sub (Dominic) Hong3, Luke Steverango4, and Chris Surma5

  • 1Department of Physics, University of Alberta, Edmonton, Alberta, T6G 2E1, Canada
  • 2Department of Earth and Atmospheric Sciences, University of Alberta, Edmonton, Alberta, T6G 2E3, Canada
  • 3Department of Engineering Science, University of Toronto, Toronto, Ontario, M5S 1A1, Canada
  • 4Department of Mathematics, McGill University, Montreal, Quebec, Canada
  • 5Department of Mechanical Engineering, University of Alberta, Edmonton, Alberta, Canada

  • *bruce.sutherland@ualberta.ca; https://www.ualberta.ca/∼bsuther
  • Present address: Department of Earth and Space Science and Engineering, York University, Toronto, Ontario, Canada.

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Vol. 3, Iss. 3 — March 2018

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