Numerical Simulations of Shock-driven Heavy Fluid Layer

The present study presents the numerical simulations for a shocked-heavy fluid layer with a stratified N2/SF6/N2 configuration. Simulations were conducted using a third-order modal discontinuous Galerkin method to solve the compressible two-component Euler equations. The results were validated against experimental data, confirming the accuracy of the computational approach. Dynamics of the heavy fluid layer were found to be strongly influenced by the shock Mach numbers Ms = 1.15, 1.25, 1.5. At a lower Mach number Ms = 1.15, the interface deformations remained smooth and relatively symmetric, with limited vorticity generation and weak perturbations. Baroclinic effects at this stage were minimal, and the instability growth remained linear. As the Mach number increased to Ms = 1.25, the interaction became nonlinear, leading to the formation of small-scaled vortex structures driven by moderate baroclinic effects. Interface mixing intensified as rotational motion increased. At the highest Mach number Ms = 1.5, the interface rapidly evolved into chaotic structures, characterized by significant vorticity amplification, vortex roll-up, and the onset of turbulence. The baroclinic vorticity, resulting from the misalignment of pressure and density gradients, dominated the vorticity production mechanism, particularly at higher Mach numbers. Quantitative analysis demonstrated that average vorticity, baroclinic vorticity, and enstrophy grew rapidly with increasing Mach numbers. Enstrophy, which quantifies turbulence intensity, exhibited pronounced growth at Ms = 1.5, marking the transition to turbulent mixing.

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Publication Details

Journal
Journal of Graphic Era University
Published
2025-02-05
DOI
https://doi.org/10.13052/jgeu0975-1416.1314
Citations
5
Primary Topic
Gas Dynamics and Kinetic Theory
Type
article
Field-Weighted Citation Impact
18.64

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article

Numerical Simulations of Shock-driven Heavy Fluid Layer

Satyvir Singh
5 citations
Journal of Graphic Era University
Gas Dynamics and Kinetic Theory
18.64
article

Numerical Simulations of Shock-driven Heavy Fluid Layer

Satyvir Singh
article en
5 citations

Abstract

The present study presents the numerical simulations for a shocked-heavy fluid layer with a stratified N2/SF6/N2 configuration. Simulations were conducted using a third-order modal discontinuous Galerkin method to solve the compressible two-component Euler equations. The results were validated against experimental data, confirming the accuracy of the computational approach. Dynamics of the heavy fluid layer were found to be strongly influenced by the shock Mach numbers Ms = 1.15, 1.25, 1.5. At a lower Mach number Ms = 1.15, the interface deformations remained smooth and relatively symmetric, with limited vorticity generation and weak perturbations. Baroclinic effects at this stage were minimal, and the instability growth remained linear. As the Mach number increased to Ms = 1.25, the interaction became nonlinear, leading to the formation of small-scaled vortex structures driven by moderate baroclinic effects. Interface mixing intensified as rotational motion increased. At the highest Mach number Ms = 1.5, the interface rapidly evolved into chaotic structures, characterized by significant vorticity amplification, vortex roll-up, and the onset of turbulence. The baroclinic vorticity, resulting from the misalignment of pressure and density gradients, dominated the vorticity production mechanism, particularly at higher Mach numbers. Quantitative analysis demonstrated that average vorticity, baroclinic vorticity, and enstrophy grew rapidly with increasing Mach numbers. Enstrophy, which quantifies turbulence intensity, exhibited pronounced growth at Ms = 1.5, marking the transition to turbulent mixing.

Journal of Graphic Era University
RWTH Aachen University (DE)
Deutsche Forschungsgemeinschaft
Openalex Percentile: Top 1%
Gas Dynamics and Kinetic Theory
18.64
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Numerical Simulations of Shock-driven Heavy Fluid Layer — Satyvir Singh · Journal of Graphic Era University (2025) | TGRS Research Map | TGRS