A new slantwise convection parameterization is developed for global ocean models of icy moons and tested against convection-resolving simulations, reproducing key heat transport inside the tangent cylinder.
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Parameterizing slantwise convection in icy moon oceans
A new slantwise convection parameterization is developed for global ocean models of icy moons and tested against convection-resolving simulations, reproducing key heat transport inside the tangent cylinder.