arXiv Analytics

Sign in

arXiv:2009.07675 [physics.flu-dyn]AbstractReferencesReviewsResources

Correlation of internal flow structure with heat transfer efficiency in turbulent Rayleigh-Bénard convection

Ao Xu, Xin Chen, Feng Wang, Heng-Dong Xi

Published 2020-09-16Version 1

To understand how internal flow structures manifest themselves in the global heat transfer, we study the correlation between different flow modes and the instantaneous Nusselt number ($Nu$) in a two-dimensional square Rayleigh-B\'enard convection cell. High-resolution and long-time direct numerical simulations are carried out for Rayleigh number between $10^{7}$ and $10^{9}$ and Prandtl number of 5.3. The investigated Nusselt numbers include the volume-averaged $Nu_{\text{vol}}$, the wall-averaged $Nu_{\text{wall}}$, the kinetic energy dissipation based $Nu_{\text{kinetic}}$ and the thermal energy dissipation based $Nu_{\text{thermal}}$. The Fourier mode decomposition and proper orthogonal decomposition are adopted to extract the coherent flow structure. Our results show that the single-roll mode, the horizontally stacked double-roll mode, and the quadrupolar flow mode are more efficient for heat transfer on average. In contrast, the vertically stacked double roll mode is inefficient for heat transfer on average. The volume-averaged $Nu_{\text{vol}}$ and the kinetic energy dissipation based $Nu_{\text{kinetic}}$ can better reproduce the correlation of internal flow structure with heat transfer efficiency than that of the wall-averaged $Nu_{\text{wall}}$ and the thermal energy dissipation based $Nu_{\text{thermal}}$, even though these four Nusselt numbers give consistent time-averaged mean values. The ensemble-averaged time trace of $Nu$ during flow reversal shows that only the volume-averaged $Nu_{\text{vol}}$ can reproduce the overshoot phenomena that is observed in the previous experimental study. Our results reveal that the proper choice of the $Nu$ is critical to obtain a meaningful interpretation.

Related articles: Most relevant | Search more
arXiv:1412.6299 [physics.flu-dyn] (Published 2014-12-19)
Turbulent Rayleigh-Bénard convection described by projected dynamics in phase space
arXiv:2505.02580 [physics.flu-dyn] (Published 2025-05-05)
Temperature and pressure reconstruction in turbulent Rayleigh-Bénard convection by Lagrangian velocities using PINN
arXiv:2205.11355 [physics.flu-dyn] (Published 2022-05-23)
Turbulent Rayleigh-Bénard convection with bubbles attached to the plate