Drive Asymmetry, Convergence and the Origin of Turbulence in ICF Implosions
Vincent A. Thomas, Robert J. Kares

TL;DR
This paper uses high-resolution 3D simulations to explore how drive asymmetry causes turbulence and mixing in ICF implosions, revealing that vortical instabilities are a major turbulence source beyond surface imperfections.
Contribution
It demonstrates that three-dimensional vortical instabilities induced by asymmetries are a key source of turbulence, challenging the view that surface imperfections are the primary cause.
Findings
Vortical structures lead to turbulence and mix in ICF implosions.
Higher convergence increases hydrodynamic disruption and turbulence.
Asymmetry-induced instabilities are a significant turbulence source.
Abstract
2D and 3D numerical simulations with the adaptive mesh refinement Eulerian radiation-hydrocode RAGE are used to investigate hydrodynamic disruption of asymmetrically driven ICF implosions. A central aspect of this phenomenon is the connection between drive asymmetry and the generation of turbulence in the DT fuel. Long wavelength deviations from spherical symmetry in the pressure drive lead to the generation of coherent vortical structures in the DT gas and it is the three dimensional instability of these structures that in turn leads to turbulence and mix. RAGE simulations with spatial resolutions as high as 0.05 {\mu}m in 3D are presented to exhibit the detailed mechanisms of turbulence growth. These simulations suggest that the amplification of small initial surface imperfections by acceleration-induced instabilities is not the only important source of turbulent mix in ICF implosions…
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