4.7 Article

Dynamics of fingering convection. Part 2 The formation of thermohaline staircases

Journal

JOURNAL OF FLUID MECHANICS
Volume 677, Issue -, Pages 554-571

Publisher

CAMBRIDGE UNIV PRESS
DOI: 10.1017/jfm.2011.99

Keywords

double-diffusive convection; geophysical and geological flows

Funding

  1. National Science Foundation [NSF-093379, OCE 0547650, ANT 0944536, AST 0806431, CBET 0933057]
  2. NASA [NNG05GG69G, NNG06GD44G, NNX07A2749]
  3. Directorate For Engineering [0933759] Funding Source: National Science Foundation
  4. Division Of Astronomical Sciences
  5. Direct For Mathematical & Physical Scien [0807672] Funding Source: National Science Foundation
  6. Div Of Chem, Bioeng, Env, & Transp Sys [0933759] Funding Source: National Science Foundation

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Regions of the ocean's thermocline unstable to salt fingering are often observed to host thermohaline staircases, stacks of deep well-mixed convective layers separated by thin stably stratified interfaces. Decades after their discovery, however, their origin remains controversial. In this paper we use three-dimensional direct numerical simulations to shed light on the problem. We study the evolution of an analogous double-diffusive system, starting from an initial statistically homogeneous fingering state, and find that it spontaneously transforms into a layered state. By analysing our results in the light of the mean-field theory developed in Part 1 (Traxler et al., J. Fluid Mech. doi:10.1017/jfm.2011.98,2011), a clear picture of the sequence of events resulting in the staircase formation emerges. A collective instability of homogeneous fingering convection first excites a field of gravity waves, with a well-defined vertical wavelength. However, the waves saturate early through regular but localized breaking events and are not directly responsible for the formation of the staircase. Meanwhile, slower-growing, horizontally invariant but vertically quasi-periodic gamma-modes are also excited and grow according to the gamma-instability mechanism. Our results suggest that the nonlinear interaction between these various mean-field modes of instability leads to the selection of one particular gamma-mode as the staircase progenitor. Upon reaching a critical amplitude, this progenitor overturns into a fully formed staircase. We conclude by extending the results of our simulations to real oceanic parameter values and find that the progenitor gamma-mode is expected to grow on a time scale of a few hours and leads to the formation of a thermohaline staircase in about one day with an initial spacing in the order of 1-2 m.

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