Double-diffusive overflow reservoir 2026-10-14
Layered convection in a giant planet 2026-10-06
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.
Past exam of the mathematics course of the University of Cambridge 2001 iii Paper 43 4 c Solution Created 2026-10-03 Updated 2026-10-14
Use positive jumps and for the hot salty lower reservoir. The Boussinesq density excess below the interface is proportional to . Static stability therefore requireswith 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.