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Compressible turbulent convection at very high Rayleigh numbers

Fluid Dynamics 2024-11-18 v1 Solar and Stellar Astrophysics

Abstract

Heat transport in highly turbulent convection is not well understood. In this paper, we simulate compressible convection in a box of aspect ratio 4 using computationally-efficient MacCormack-TVD finite difference method on single and multi-GPUs, and reach very high Rayleigh number (Ra\mathrm{Ra}) -- 101510^{15} in two dimensions and 101110^{11} in three dimensions. We show that the Nusselt number NuRa0.3\mathrm{Nu} \propto \mathrm{Ra}^{0.3} (classical scaling) that differs strongly from the ultimate-regime scaling, which is NuRa1/2\mathrm{Nu} \propto \mathrm{Ra}^{1/2}. The bulk temperature drops adiabatically along the vertical even for high Ra\mathrm{Ra}, which is in contrast to the constant bulk temperature in Rayleigh-B\'{e}nard convection (RBC). Unlike RBC, the density decreases with height. In addition, the vertical pressure-gradient (dp/dz-dp/dz) nearly matches the buoyancy term (ρg\rho g). But, the difference, dp/dzρg-dp/dz-\rho g, is equal to the nonlinear term that leads to Reynolds number ReRa1/2\mathrm{Re} \propto \mathrm{Ra}^{1/2}.

Keywords

Cite

@article{arxiv.2411.10372,
  title  = {Compressible turbulent convection at very high Rayleigh numbers},
  author = {Harshit Tiwari and Lekha Sharma and Mahendra K. Verma},
  journal= {arXiv preprint arXiv:2411.10372},
  year   = {2024}
}

Comments

17 pages, 16 figures