Faraday Disk Dynamo
Laminar and Turbulent Flow
Magnetostatic Boundary Conditions
Eulerian and Lagrangian Flow Descriptions
Navier–Stokes Equations
Accelerating Fluids
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Updated: May 7, 2026

Investigating the Three-dimensional Flow Separation Induced by a Model Vocal Fold Polyp
Published on: February 3, 2014
I V Khalzov1, C M Cooper, C B Forest
1Center for Magnetic Self Organization in Laboratory and Astrophysical Plasmas, University of Wisconsin-Madison, 1150 University Avenue, Madison, Wisconsin 53706, USA.
This study numerically shows that fast dynamos can be achieved in realistic, self-consistent fluid flows within a sphere. These findings are crucial for understanding plasma dynamics and magnetic field generation in astrophysical and experimental settings.
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