Current-vortex-sheet model of the magnetic Rayleigh-Taylor instability

This study investigates the Rayleigh-Taylor instability in the magnetic field applied parallel to the interface. The motion of the interface is described using a current-vortex-sheet model. The growth rate of the interface is obtained from a linear stability analysis of the model. The interface of a single mode k=1 is linearly stable for R_{A}≤1, where R_{A} denotes the Alfvén number. Further, we conduct numerical computations for the evolution of the interface from the model for both regimes of R_{A}≤1 and R_{A}>1. For R_{A}≤1, the interface oscillates vertically but does not intrude into the opposite phase. The amplitude of the interface and the oscillation period decrease with decrease in R_{A}. For 1<R_{A}≲1.5, the interface undergoes some growth at early times and then decreases. This oscillation is repeated, and no roll-ups are observed at the interface. Therefore, the nonlinear growth of the Rayleigh-Taylor instability is stabilized by a sufficiently strong magnetic field. For R_{A}≳3 the interface is unstable and the pattern of the interface evolution differs from the density ratio. In addition, the magnetic field is greatly amplified as R_{A} increases.

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Publication Details

Journal
Physical review. E
Published
2024-11-05
DOI
https://doi.org/10.1103/physreve.110.055102
Citations
1
Primary Topic
Fluid Dynamics and Turbulent Flows
Type
article
Field-Weighted Citation Impact
0.37

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article

Current-vortex-sheet model of the magnetic Rayleigh-Taylor instability

Sung-Ik Sohn, Seunghyeon Baek
1 citations
Physical review. E
Fluid Dynamics and Turbulent Flows
0.37
article

Current-vortex-sheet model of the magnetic Rayleigh-Taylor instability

Sung-Ik Sohn, Seunghyeon Baek
article en
1 citations

Abstract

This study investigates the Rayleigh-Taylor instability in the magnetic field applied parallel to the interface. The motion of the interface is described using a current-vortex-sheet model. The growth rate of the interface is obtained from a linear stability analysis of the model. The interface of a single mode k=1 is linearly stable for R_{A}≤1, where R_{A} denotes the Alfvén number. Further, we conduct numerical computations for the evolution of the interface from the model for both regimes of R_{A}≤1 and R_{A}>1. For R_{A}≤1, the interface oscillates vertically but does not intrude into the opposite phase. The amplitude of the interface and the oscillation period decrease with decrease in R_{A}. For 1<R_{A}≲1.5, the interface undergoes some growth at early times and then decreases. This oscillation is repeated, and no roll-ups are observed at the interface. Therefore, the nonlinear growth of the Rayleigh-Taylor instability is stabilized by a sufficiently strong magnetic field. For R_{A}≳3 the interface is unstable and the pattern of the interface evolution differs from the density ratio. In addition, the magnetic field is greatly amplified as R_{A} increases.

Physical review. EVol. 110(5)
Gangneung–Wonju National University (KR)
National Research Foundation of Korea
Openalex Percentile: Top 41%
Fluid Dynamics and Turbulent Flows
0.37
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Current-vortex-sheet model of the magnetic Rayleigh-Taylor instability — Sung-Ik Sohn, Seunghyeon Baek · Physical review. E (2024) | TGRS Research Map | TGRS