Rayleigh-Taylor Unstable Flames: Thin and Thick

TL;DR

This paper investigates the structure of Rayleigh-Taylor unstable flames, showing they can be thickened by turbulence but differ from classical turbulent flames, impacting subgrid modeling in complex systems.

Contribution

It introduces a large parameter study and direct measurements to analyze RT unstable flames, revealing their unique thickening behavior and structural differences from turbulent flames.

Findings

RT unstable flames can be thickened by self-generated turbulence

Their structure differs from classical turbulent flames

Implications for subgrid modeling in practical applications

Abstract

A Rayleigh-Taylor (RT) unstable flame is a thin burning interface sandwiched between heavy fuel and light ash layers. RT unstable flames play an important role in complex systems like novel aviation turbine engines, storage facilities for alternative fuels and refrigerants and Type Ia supernovae. Simulations of these systems must use subgrid models of RT flame behavior, but choosing the subgrid model is difficult because RT unstable flames have characteristics of both the classical RT instability and turbulent combustion. In this paper, we investigate whether the flame structure of RT unstable flames can be described using ideas from turbulent combustion theory. We use a large parameter study of Boussinesq model flames and direct measurements of the internal flame structure to show that RT unstable flames can be thickened by their own self-generated turbulence, but that the structure of these thickened flames differs from turbulent flames. Finally, we discuss the implications for modelling RT unstable flames in practical applications.