Rayleigh-Bénard convection rolls determine the shape evolution of an ice block melting from below

  • Lohse, Detlef (Physics of Fluids Group, Max-Planck Center Tw)
  • Yang, Rui (Physics of Fluids Group, Max-Planck Center Tw)
  • Howland, Christopher (Physics of Fluids Group, Max-Planck Center Tw)
  • Liu, Hao-Ran (Physics of Fluids Group, Max-Planck Center Tw)
  • Verzicco, Roberto (Tor Vergata University)

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We numerically study the melting process of a solid layer heated from below such that a liquid melt layer develops underneath. The objective is to quantitatively describe and understand the emerging topology of the structures (characterized by the amplitude and wavelength), which evolve out of an initially smooth surface. By performing both two-dimensional (achieving Rayleigh number up to Ra = 1011) and three- dimensional (achieving Rayleigh number up to Ra = 109) direct numerical simulations with an advanced finite difference solver coupled to the phase-field method, we show how the interface roughness is sponta- neously generated by thermal convection. With increasing height of the melt the convective flow intensifies and eventually even becomes turbulent. As a consequence the interface becomes rougher but still coupled to the flow topology. The emerging structure of the interface coincides with the regions of rising hot plumes and descending cold plumes. We find that the roughness amplitude scales with the mean height of the liquid layer. We derive this scaling from the Stefan boundary condition and relate it to the non-uniform distribution of heat flux at the interface. For 2D cases, we further quantify the horizontal length scale of the morphology, based on the theoretical upper and lower bounds given for the size of convective cells known from Ref. [1]. These bounds well agree with our simulation results. Our findings highlight the key connection between the morphology of the melting solid and the convective flow structures in the melt beneath. More details on our work can be found in Ref. [2].