DOE OSTI · 2311793
Ablative Magnetohydrodynamic Rayleigh-Taylor Instability (Final Technical Report)
Abstract
The Rayleigh-Taylor Instability (RTI) is a ubiquitous flow phenomenon occurring in a multitude of natural and engineered systems in which buoyancy forces exist. RTI is primarily a limiting process in many HED applications and there are significant efforts within the NNSA-ICF program to account for its effect in large scale simulations of ICF implosions both in two- and three-dimensions. The goal of the proposed research is to develop a fundamental understanding of the evolution and role of magnetic fields in the ablative Rayleigh–Taylor instability (aRTI) in the deeply nonlinear stage.
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Aluie, Hussein. 2024-03-07. Ablative Magnetohydrodynamic Rayleigh-Taylor Instability (Final Technical Report). https://doi.org/10.2172/2311793
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