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Andrew Wells

Associate Professor of Physical Climate Science

Research theme

  • Climate physics

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Ice and Fluid Dynamics
Andrew.Wells@physics.ox.ac.uk
Telephone: 01865 (2)82425
Robert Hooke Building, room F60
  • About
  • Publications

Turbulent plumes from a glacier terminus melting in a stratified ocean

Journal of Geophysical Research: Oceans American Geophysical Union 121:7 (2016) 4670-4696

Authors:

Andrew Wells, Samuel J Magorrian

Abstract:

The melting of submerged faces of marine-terminating glaciers is a key contributor to the glacial mass budget via direct thermodynamic ablation and the impact of ablation on calving. This study considers the behavior of turbulent plumes of buoyant meltwater in a stratified ocean, generated by melting of either near-vertical calving faces or sloping ice shelves. We build insight by applying a turbulent plume model to describe melting of a locally planar region of ice face in a linearly stratified ocean, in a regime where subglacial discharge is insignificant. The plumes rise until becoming neutrally buoyant, before intruding into the ocean background. For strong stratifications, we obtain leading-order scaling laws for the flow including the height reached by the plume before intrusion, and the melt rate, expressed in terms of the background ocean temperature and salinity stratifications. These scaling laws provide a new perspective for parameterizing glacial melting in response to a piecewise-linear discretization of the ocean stratification.
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The impact of imperfect heat transfer on the convective instability of a thermal boundary layer in a porous media

Journal of Fluid Mechanics Cambridge University Press (2016)

Authors:

Joseph Hitchen, Andrew Wells

Abstract:

We consider convective instability in a deep porous medium cooled from above with a linearised thermal exchange at the upper surface, thus determining the impact of using a Robin boundary condition, in contrast to previous previous studies using a Dirichlet boundary condition. With the linearised surface exchange, the thermal flux out of the porous layer depends linearly on the temperature difference between the effective temperature of a heat sink at the upper boundary and the temperature at the surface of the porous layer. The rate of this exchange is characterised by a dimensionless Biot number, Bi, determined by the effective thermal conductivity of exchange with the heat sink relative to the physical thermal conductivity of the porous layer. For a given temperature difference between the heat sink at the upper boundary and deep in the porous medium, we find that imperfectly cooled layers with finite Biot numbers are more stable to convective instabilities than perfectly cooled layers which have large, effectively infinite Biot numbers. Two regimes of behaviour were determined with contrasting stability behaviour and characteristic scales. When the Biot number is large the near-perfect heat transfer produces small corrections of order 1/Bi to the perfectly conducting behaviour found when the Biot number is infinite. In the insulating limit as the Biot number approaches zero, a different behaviour was found with significantly larger scales for the critical wavelength and depth of convection both scaling proportional to 1/ √ Bi
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Solidification of a disk-shaped crystal from a weakly supercooled binary melt

Physical Review E: Statistical, Nonlinear, and Soft Matter Physics American Physical Society 92:2 (2015)

Authors:

David Rees Jones, AJ Wells

Abstract:

The physics of ice crystal growth from the liquid phase, especially in the presence of salt, has received much less attention than the growth of snow crystals from the vapor phase. The growth of so-called frazil ice by solidification of a supercooled aqueous salt solution is consistent with crystal growth in the basal plane being limited by the diffusive removal of the latent heat of solidification from the solid-liquid interface, while being limited by attachment kinetics in the perpendicular direction. This leads to the formation of approximately disk-shaped crystals with a low aspect ratio of thickness compared to radius, because radial growth is much faster than axial growth. We calculate numerically how fast disk-shaped crystals grow in both pure and binary melts, accounting for the comparatively slow axial growth, the effect of dissolved solute in the fluid phase, and the difference in thermal properties between solid and fluid phases. We identify the main physical mechanisms that control crystal growth and show that the diffusive removal of both the latent heat released and the salt rejected at the growing interface are significant. Our calculations demonstrate that certain previous parametrizations, based on scaling arguments, substantially underestimate crystal growth rates by a factor of order 10–100 for low aspect ratio disks, and we provide a parametrization for use in models of ice crystal growth in environmental settings.
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Steady turbulent density currents on a slope in a rotating fluid

Journal of Fluid Mechanics Cambridge University Press (CUP) 746 (2014) 405-436

Authors:

GE Manucharyan, W Moon, F Sévellec, AJ Wells, J-Q Zhong, JS Wettlaufer
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Nonlinear mushy-layer convection with chimneys: stability and optimal solute fluxes

JOURNAL OF FLUID MECHANICS 716 (2013) 203-227

Authors:

Andrew J Wells, JS Wettlaufer, Steven A Orszag
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