A steady well-mixed hot salty reservoir receives volume flux and loses the same flux over a weir. Heat and salt balances are and . If and , define . Then and . For and the interface is statically stable while preferential heat transfer can drive double-diffusive convection.
A stabilizing composition gradient can suppress large overturning motions while permitting double-diffusive convection in small layers separated by interfaces. If heat loss is less efficient than in a single well-mixed adiabat, the planet retains more entropy and contracts more slowly. This is a proposed delayed-cooling contribution to hot-Jupiter radius inflation, with an effectiveness that depends on the gradient and layer structure.
Use positive jumps and for the hot salty lower reservoir. The Boussinesq density excess below the interface is proportional to . Static stability therefore requires
with one the neutral limiting value. For the lower layer is lighter overall and ordinary overturning convection replaces the statically stable interface.
In the stable hot-below, salty-below configuration, thermal diffusivity exceeds salt diffusivity. Heat transfer can destabilize thin adjacent fluid regions before the stabilizing salt difference is erased, causing the diffusive regime of double-diffusive convection. As , stabilization by salt dominates, interfacial convective exchange is strongly suppressed, and the specified heat-flux model tends to zero at fixed . This limit is not a claim that molecular heat conduction itself ceases.
Thermosolutal convection 2026-10-14
Thermosolutal convection is double-diffusive convection driven by temperature and concentration gradients. Their buoyancy contributions can oppose one another, while unequal thermal diffusivity and solutal diffusivity allow steady, oscillatory and finite-amplitude states. For a layer heated from below with a stabilizing concentration gradient, thermal buoyancy is destabilizing and solutal buoyancy restoring.