Numerical convergence of 2D solar convection in implicit large-eddy simulations

TL;DR

This study investigates the numerical convergence of implicit large-eddy simulations (ILES) for 2D turbulent solar convection, demonstrating that even low-resolution simulations can accurately capture large-scale dynamics.

Contribution

It provides the first detailed analysis of convergence and effective Reynolds numbers in 2D ILES of solar-like convection, establishing minimal resolution requirements.

Findings

Convergence occurs at resolutions ≥512^2 grid points.

Low-resolution (128^2) simulations still capture large-scale dynamics.

High resolution is necessary for detailed structures and gravity wave interactions.

Abstract

Large-eddy simulations (LES) and implicit LES (ILES) are wise and affordable alternatives to the unfeasible direct numerical simulations (DNS) of turbulent flows at high Reynolds numbers (Re). However, for systems with few observational constraints, it is a formidable challenge to determine if these strategies adequately capture the physics of the system. Here we address this problem by analyzing numerical convergence of ILES of turbulent convection in 2D, with resolutions between $64^2$ and $2048^2$ grid points, along with the estimation of their effective viscosities, resulting in effective Reynolds numbers between $1$ and $\sim10^4$. The thermodynamic structure of our model resembles the solar interior, including a fraction of the radiative zone and the convection zone. In the convective layer, the ILES solutions converge for the simulations with $\ge 512^2$ grid points, as evidenced by the integral properties of the flow and its power spectra. Most importantly, we found that even a resolution of $128^2$ grid points, Re$\sim10$, is sufficient to capture the dynamics of the large scales accurately. This is a consequence of the ILES method allowing that the energy contained in these scales is the same in simulations with low and high resolution. Special attention is needed in regions with a small density scale height driving the formation of fine structures unresolved by the numerical grid. In the stable layer we found the excitation of internal gravity waves, yet high resolution is needed to capture their development and interaction.