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Updated: Sep 30, 2025

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Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
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Incompressible Rayleigh-Taylor mixing in circular and spherical geometries
1Department of Physics and INFN, University of Torino, via P. Giuria 1, 10125 Torino, Italy.
Physical Review. E
|March 16, 2022
Summary
Convergent geometries in fluid dynamics cause mixing layers to drift inward, unlike planar cases. This inward drift in turbulent Rayleigh-Taylor instability is explained by a simple geometrical relation.
Area of Science:
- Fluid Dynamics
- Plasma Physics
- Astrophysics
Background:
- Rayleigh-Taylor instability drives turbulent mixing in fluids.
- Understanding mixing layer evolution is crucial for various scientific fields.
Purpose of the Study:
- Investigate turbulent mixing layer evolution in convergent geometries.
- Compare convergent vs. planar geometries for Rayleigh-Taylor instability.
- Analyze density flux and radial profile changes.
Main Methods:
- Numerical simulations in circular (2D) and spherical (3D) geometries.
- Application of the Boussinesq approximation.
- Analysis of turbulent fluid evolution.
Main Results:
- Convergent geometries cause mixing layer centers to drift inward.
- Radial density flux profiles exhibit inward drift.
- A geometrical relation for inward drift based on mass conservation was derived.
- Late-stage evolution shows inward-outward asymmetry in radial profiles.
Conclusions:
- Geometry significantly impacts mixing layer dynamics in Rayleigh-Taylor instability.
- Inward drift is a key characteristic of convergent geometries.
- The derived geometrical relation provides a predictive tool for fluid mixing.
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