Turbulent thermal convection is ubiquitous in nature – occurring in the planets' oceans, atmospheres and mantles, as well as in stars, including our Sun.
Convective heat transport is also important in engineering and technological applications.
Rayleigh–Bénard convection (RBC) is one of paradigm systems to study turbulent thermal convection.
In a RBC cell, a fluid is confined between two horizontal plates, an upper cooled and a lower heated, and adiabatic vertical walls.
All processes inside the RBC cell are determined mainly by the dimensionless Rayleigh number Ra and the Prandtl number Pr,
which both depend on the fluid properties, and Ra is also proportional to the cubed cell height and to the temperature drop between the highest and lowest temperature in the system.
Instantaneous temperature isosurfaces in a turbulent Rayleigh–Bénard flow for the Prandtl number Pr=1 and Rayleigh number Ra=109, as obtained in direct numerical simulations.
A warm fluid moves away from the heated bottom (pink) and a cold fluid moves away from the cooled top (blue).
Viscous and thermal boundary layers (BLs) play a critical role in the heat transfer.
The classical BL Prandtl–Blasius–Pohlhausen theory cannot describe well the BLs in turbulent RBC as its inherent features like pressure gradients within the BLs,
fluctuations and buoyancy, are assumed to be negligible in that approach.
Shishkina et al., Phys. Rev. E 89 (2014)
Shishkina et al., J. Fluid Mech. 730 (2013)
we advanced the BL theory by its extension to the case of a non-vanishing pressure gradient within the BLs, when
a large-scale circulation approaches the heated and cooled plates not parallel to them.
Shishkinaet al., Phys. Rev. Lett. 114 (2015)
we studied the effect of fluctuations within the BLs by considering the turbulent thermal diffusivity κτ there.
We derived that in the vicinity of the plates, κτ is a cubic function on the vertical coordinate ξ, and only later, for larger ξ,
where the velocity and temperature profiles start to follow a log-law, κτ is almost linear on ξ.
The new developed BL equations were solved analytically for the case of infinitely large Prandtl number Pr and Pr ∼ 1 (see figure below) and an excellent agreement with direct numerical simulations was demonstrated.