Considering the full spectrum of linear unstable modes allows the turbulent diffusion coefficient in thermohaline convection to self-consistently interpolate between previously discrepant theoretical scalings.
J., Glebbeek, E., Izzard, R
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Unifying Transport Models of Thermohaline Convection in Stars
Considering the full spectrum of linear unstable modes allows the turbulent diffusion coefficient in thermohaline convection to self-consistently interpolate between previously discrepant theoretical scalings.