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Scaling transition in horizontal convection near the density maximum

Zhiyang Cai, Shengqi Zhang, Kaizhen Shi, Zhouxin Jiang, Shijun Liao

TL;DR

The paper tackles horizontal convection under a nonlinear equation of state near water's density maximum, advancing beyond the OB approximation. It develops an extended Shishkina-Grossmann-Lohse framework by introducing a NOB potential-energy transfer term $\Phi_{i2}$ and linking plume height $\hat{z}$ to global transport scalings, predicting a transition when plumes penetrate the full depth ($\hat{z}\sim H$). Direct numerical simulations reveal a flow-topology shift in NOB-SHC from a bicellular structure to a full-depth single-roll circulation, with heat-transport scaling transitioning from $Nu \sim Ra^{1/4}$ to $Ra^{1/3}$ and Reynolds scaling from $Re \sim Ra^{1/2}$ to $Ra^{4/9}$. The results unify OB and NOB HC scalings within the GL/SGL framework and elucidate how density anomalies can drive enhanced mixing and transport in geophysical-like systems.

Abstract

Horizontal convection (HC) serves as a canonical model for geophysical and industrial flows driven by differential heating along a surface. While the classical Oberbeck-Boussinesq (OB) approximation is well-established, the impact of a nonlinear equation of state, specifically the density maximum of water near $4^\circ\mathrm{C}$, remains underexplored. This study investigates Non-Oberbeck-Boussinesq (NOB) effects on HC via direct numerical simulations (DNS) over a Rayleigh number range of $10^6 \le Ra \le 5\times 10^{10}$. We examine two configurations: Classical HC (CHC) and Symmetric HC (SHC). Our results reveal that the NOB-SHC case undergoes a structural transition, evolving from a bicellular structure to a full-depth, single-roll circulation driven by central `mixing plumes'. This reorganization manifests as transitional anomalies in Reynolds number ($Re$) scaling, whereas the emergence of full-depth plumes fundamentally alters the heat transport mechanism. Consequently, unlike the classical Rossby scaling ($Nu \sim Ra^{1/5}$) observed in reference cases, the NOB-SHC regime exhibits an enhanced heat transport scaling ranging from $Nu \sim Ra^{1/4}$ to $Ra^{1/3}$. To rationalize this behavior, we extend the Shishkina-Grossmann-Lohse (SGL) theory by incorporating a generalized potential energy transfer term ($Φ_{i2}$). The theoretical framework demonstrates that the global scaling law is dictated by the characteristic plume height ($\hat{z}$). Specifically, when plumes penetrate the entire cavity depth ($\hat{z} \sim H$), as observed in the NOB-SHC case, the flow transcends classical bounds for OB HC, accessing a regime analogous to Rayleigh Bénard convection. The proposed theory successfully unifies the scaling laws for both OB and NOB fluids, showing excellent agreement with numerical data.

Scaling transition in horizontal convection near the density maximum

TL;DR

The paper tackles horizontal convection under a nonlinear equation of state near water's density maximum, advancing beyond the OB approximation. It develops an extended Shishkina-Grossmann-Lohse framework by introducing a NOB potential-energy transfer term and linking plume height to global transport scalings, predicting a transition when plumes penetrate the full depth (). Direct numerical simulations reveal a flow-topology shift in NOB-SHC from a bicellular structure to a full-depth single-roll circulation, with heat-transport scaling transitioning from to and Reynolds scaling from to . The results unify OB and NOB HC scalings within the GL/SGL framework and elucidate how density anomalies can drive enhanced mixing and transport in geophysical-like systems.

Abstract

Horizontal convection (HC) serves as a canonical model for geophysical and industrial flows driven by differential heating along a surface. While the classical Oberbeck-Boussinesq (OB) approximation is well-established, the impact of a nonlinear equation of state, specifically the density maximum of water near , remains underexplored. This study investigates Non-Oberbeck-Boussinesq (NOB) effects on HC via direct numerical simulations (DNS) over a Rayleigh number range of . We examine two configurations: Classical HC (CHC) and Symmetric HC (SHC). Our results reveal that the NOB-SHC case undergoes a structural transition, evolving from a bicellular structure to a full-depth, single-roll circulation driven by central `mixing plumes'. This reorganization manifests as transitional anomalies in Reynolds number () scaling, whereas the emergence of full-depth plumes fundamentally alters the heat transport mechanism. Consequently, unlike the classical Rossby scaling () observed in reference cases, the NOB-SHC regime exhibits an enhanced heat transport scaling ranging from to . To rationalize this behavior, we extend the Shishkina-Grossmann-Lohse (SGL) theory by incorporating a generalized potential energy transfer term (). The theoretical framework demonstrates that the global scaling law is dictated by the characteristic plume height (). Specifically, when plumes penetrate the entire cavity depth (), as observed in the NOB-SHC case, the flow transcends classical bounds for OB HC, accessing a regime analogous to Rayleigh Bénard convection. The proposed theory successfully unifies the scaling laws for both OB and NOB fluids, showing excellent agreement with numerical data.

Paper Structure

This paper contains 13 sections, 28 equations, 9 figures, 2 tables.

Figures (9)

  • Figure 1: Schematic of the computational domain and boundary conditions. No-slip conditions are applied to all boundaries. A fixed buoyancy profile (Dirichlet condition) is imposed on the bottom boundary, while the remaining walls are adiabatic. The parameters $b_0$ and $\Delta_b$ denote the reference buoyancy and the maximum buoyancy difference, respectively.
  • Figure 2: Instantaneous temperature fields (colour contours) and streamlines for the SHC cases at various Rayleigh numbers. Solid lines represent clockwise circulation, while dashed lines represent counter-clockwise circulation.
  • Figure 3: Instantaneous temperature fields (colour contours) and streamlines for the CHC cases at various Rayleigh numbers. Solid lines represent clockwise circulation, while dashed lines represent counter-clockwise circulation.
  • Figure 4: Horizontally averaged vertical profiles of kinetic energy under different $Ra$.
  • Figure 5: Time-averaged kinetic energy contributed by the (1, 1), (1, 2), (2, 1) and (2, 2) modes at different Rayleigh numbers in the NOB-SHC case.
  • ...and 4 more figures