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The paper presents new concepts and results for the eddy structure of turbulent convection in a horizontal fluid layer of depth h which lies above a solid base with thickness hb .T hefluid parameters are the kinematic viscosity ν ,t he therma ld if fusivity κ ,w hich istaken to be comparable with ν ,t hedensity ρ ,t hespecific heat cp and the expansion parameter β .T he thermal diffusivity of the solid is κb .T heresults are an extension of the more commonly studied cases, where a constant heat flux or constant temperature is applied at the interface between the fluid and the base. The buoyancy forces induce eddy motions with a typical velocity w∗ ∼ (gβFθ h)1/3 where ρcpFθ is the average heat flux and Fθ the covariance of the fluctuations of the temperature and of the vertical velocity. At moderate Reynolds numbers (Re = w∗h/ν), say less than about 103 ,a n order-of-magnitude analysis shows that for the case of high diffusivity of the base (i.e. κb  κ )e longated 'plumes' form at the surface and extend to the to po ft he fluid layer. When the base diffusivity is low (i.e. κb κ )t he surface cools below the developing 'plume' and either the plume breaks up into elongated puffs or, if κb  κ ,h orizontal pressure gradients form so that only small-scale puffs can form near the surface. At very high Reynolds numbers, approximately greater than 104 ,t he surface boundary layer below each puff/plume is highly turbulent with a local logarithmic velocity and temperature profile. An approximate analysis indicates for this case that there is insufficient buoyancy flux from the base, irrespective of its diffusivity, to maintain plumes, because of the high turbulent heat transfer. So puffs dominate high-Reynolds-number thermal convection as numerical simulations and field experiments demonstrate. However, when the surface heat flux is uniform, for example as a result of radiant heat transfer or by forcing with a constant heat flux below a very thin conducting base, plumes are the dominant form of eddy motion, as is commonly observed. In the numerical solutions presented here, where Re ∼ 3 × 102 and the slab thickness hb = h ,i t is shown that the spatial scales of eddy structures in the fluid layer close to the surface become significantly smaller as κb/κ is reduced from 100 to 0.1. At the same time in the core of the convective layer the change in the autocorrelation and spatial correlation function indicates that there is a transition from long-duration plumes into shorter-duration and smaller-length-scale elongated puffs. The simulations show that the largest temperature fluctuations near the surface occur when a constant heat flux is applied at the bottom of the fluid layer. The smallest temperature fluctuations are associated with the constant-temperature boundary condition. The finite base diffusivity cases lie in between these limits, with the largest fluctuations occurring when the thermal diffusivity of the base is

The influence of the thermal diffusivity of the lower boundary on eddy motion in convection