English

Helicity subgrid-scale models and their numerical validation

Fluid Dynamics 2026-03-30 v1 Solar and Stellar Astrophysics

Abstract

Large-eddy simulations (LES) with an appropriate subgrid-scale (SGS) model provide a powerful tool for investigating real-world turbulence. The Smagorinsky model, one of the simplest and most used SGS models, often shows an over-dissipative behavior even when using dynamic procedures to adjust the model coefficient. By incorporating the structural or geometrical information of turbulence provided by helicity (velocity-vorticity correlations), the helicity SGS model is expected to alleviate these issues in the standard Smagorinsky framework, in which only information of turbulence intensity is considered through the turbulent energy. The validity of helicity SGS models is investigated here with the aid of direct numerical simulations (DNSs). Using configurations with and without net rotation, and with large-scale helicity gradients sustained by a mechanical forcing, we show that to better model SGS turbulence, SGS helicity effects should be incorporated into the model together with the Smagorinsky-like eddy viscosity.

Keywords

Cite

@article{arxiv.2603.26559,
  title  = {Helicity subgrid-scale models and their numerical validation},
  author = {Nobumitsu Yokoi and Pablo D. Mininni and Annick Pouquet and Duane Rosenberg and Raffaele Marino},
  journal= {arXiv preprint arXiv:2603.26559},
  year   = {2026}
}

Comments

36 pages, 27 figures

R2 v1 2026-07-01T11:41:04.269Z