M. Gupta
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5 records found
1
Energetics of the Upper‐Ocean Under Sea Ice
Frictional Dissipation Versus Baroclinic Production
Plain Language Summary
Eddies are swirling features of various sizes that are ubiquitous in the ocean. At the poles, these features may be damped by the presence of sea ice, which is a layer of frozen sea water that can form on the ocean surface and provide frictional damping to the underlying currents. This work uses numerical simulations representing a patch of the polar ocean to explore how pieces of ice influence ocean eddies, particularly when the sea ice cover is not fully compacted. The simulations show that sea ice indeed damps surface eddies, but also enhances their production rate by generating fine-scale circulation patterns in the upper ocean. These physics are likely not well represented by traditional climate models, which may bias sea ice melt rates and other critical polar ocean processes. This motivates the development of better numerical schemes that can help coarse models capture the detailed mechanisms noted in the high-resolution simulations used in this work. ...
Plain Language Summary
Eddies are swirling features of various sizes that are ubiquitous in the ocean. At the poles, these features may be damped by the presence of sea ice, which is a layer of frozen sea water that can form on the ocean surface and provide frictional damping to the underlying currents. This work uses numerical simulations representing a patch of the polar ocean to explore how pieces of ice influence ocean eddies, particularly when the sea ice cover is not fully compacted. The simulations show that sea ice indeed damps surface eddies, but also enhances their production rate by generating fine-scale circulation patterns in the upper ocean. These physics are likely not well represented by traditional climate models, which may bias sea ice melt rates and other critical polar ocean processes. This motivates the development of better numerical schemes that can help coarse models capture the detailed mechanisms noted in the high-resolution simulations used in this work.
The marginal ice zone represents the periphery of the sea ice cover. In this region, the macroscale behaviour of the sea ice results from collisions and enduring contact between ice floes. This configuration closely resembles that of dense granular flows, which have been modelled successfully with the rheology. Here, we present a continuum model based on the rheology that treats sea ice as a compressible fluid, with the local sea ice concentration given by a dilatancy function. We infer expressions for and by nonlinear regression using data produced with a discrete element method (DEM) that considers polygon-shaped ice floes. We do this by driving the sea ice with a one-dimensional shearing ocean current. The resulting continuum model is a nonlinear system of equations with the sea ice velocity, local concentration and pressure as unknowns. The rheology is given by the sum of a plastic term and a viscous term. In the context of a periodic patch of ocean, which is effectively a one-dimensional problem, and under steady conditions, we prove this system to be well-posed, present a numerical algorithm for solving it, and compare its solutions to those of the DEM. These comparisons demonstrate the continuum model's ability to capture most of the DEM results accurately. The continuum model is particularly accurate for ocean currents faster than 0.25 m s; however, for low concentrations and slow ocean currents, the continuum model is less effective in capturing the DEM results. In the latter case, the lack of accuracy of the continuum model is found to be accompanied by the breakdown of a balance between the average shear stress and the integrated ocean drag extracted from the DEM. Since this balance is expected to hold independently of our choice of rheology, this finding indicates that continuum models might not be able to describe sea ice dynamics for low concentrations and slow ocean currents.
Ocean heat exchanges at the marginal ice zone (MIZ) play an important role in melting sea ice. Mixed-layer eddies transport heat and ice floes across the MIZ, facilitating the pack's access to warm waters. This study explores these frontal dynamics using disk-shaped floes coupled to an upper-ocean model simulating the sea ice edge. Numerical experiments reveal that small floes respond more strongly to fine-scale ocean currents, which favors higher dispersion rates and weakens sea ice drag onto the underlying ocean. Floes with radii smaller than resolved turbulent filaments (∼2–4 km) result in a wider and more energetic MIZ, by a factor of 70% each, compared to larger floes. We hypothesize that this floe size dependency may affect sea ice break-up by controlling oceanic energy propagation into the MIZ and modulate the sea ice pack's melt rate by regulating lateral heat transport toward the sea ice cover.