The Magnetic Reynolds number (R_{m}) is a dimensionless group that occurs in magnetohydrodynamics. It gives an estimate of the effects of magnetic advection to magnetic diffusion, and is typically defined by:

\mathrm{R}_\mathrm{m} = \frac{U L}{\eta}
where

U is a typical velocity scale of the flow

L is a typical length scale of the flow

\eta is the magnetic diffusivity
Contents

General Characteristics for Large and Small Rm 1

Relationship to the Reynolds Number and Péclet Number 2

Relationship to Eddy Current Braking 3

See also 4

References 5
General Characteristics for Large and Small R_{m}
For \mathrm{R}_\mathrm{m} \ll 1, advection is relatively unimportant, and so the magnetic field will tend to relax towards a purely diffusive state, determined by the boundary conditions rather than the flow.
For \mathrm{R}_\mathrm{m} \gg 1, diffusion is relatively unimportant on the length scale L. Flux lines of the magnetic field are then advected with the fluid flow, until such time as gradients are concentrated into regions of short enough length scale that diffusion can balance advection.
Relationship to the Reynolds Number and Péclet Number
The Magnetic Reynolds number has a similar form to both the Péclet number and the Reynolds number. All three can be regarded as giving the ratio of advective to diffusive effects for a particular physical field, and have a similar form of a velocity times a length divided by a diffusivity. The magnetic Reynolds number is related to the magnetic field in an MHD flow, while the Reynolds number is related to the fluid velocity itself, and the Péclet number a related to heat. The dimensionless groups arise in the nondimensionalization of the respective governing equations, the induction equation, the momentum equation, and the heat equation.
Relationship to Eddy Current Braking
The dimensionless magnetic Reynolds number, R_m, is also used in cases where there is no physical fluid involved.

R_m = \mu \sigma × (characteristic length) × (characteristic velocity)

where

\mu is the magnetic permeability

\sigma is the electrical conductivity.
For R_m < 1 the skin effect is negligible and the eddy current braking torque follows the theoretical curve of an induction motor.
For R_m > 30 the skin effect dominates and the braking torque decreases much slower with increasing speed than predicted by the induction motor model.^{[1]}
See also
References

^ Ripper, M.D; Endean, V.G (Mar 1975). "EddyCurrent BrakingTorque Measurements on a Thick Copper Disc". Proc IEE 122 (3): 301–302.
Weisstein, Eric W., Magnetic Reynolds Number from ScienceWorld.
Moffatt, H. Keith, 2000, Reflections on Magnetohydrodynamics. In: Perspectives in Fluid Dynamics (ISBN 0521531691) (Ed. G.K. Batchelor, H.K. Moffatt & M.G. Worster) Cambridge University Press, p347391.
P. A. Davidson, 2001, "An Introduction to Magnetohydrodynamics" (ISBN 0521794870), Cambridge University Press.
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