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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Simulations show that 3D electromagnetic induction effects from ice-shell thickness variations on Enceladus can constrain ocean conductivity and provide lower bounds on salinity if detected by low-altitude orbiter measurements.
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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.
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Exploring Enceladus's Interior Structure Using Electromagnetic Induction
Simulations show that 3D electromagnetic induction effects from ice-shell thickness variations on Enceladus can constrain ocean conductivity and provide lower bounds on salinity if detected by low-altitude orbiter measurements.