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The '''Chandrasekhar number''' is a [[dimensionless quantity]] used in magnetic [[convection]] to represent ratio of the [[Lorentz force]] to the [[viscosity]]. It is named after the [[India]]n [[astrophysicist]] [[Subrahmanyan Chandrasekhar]].
 
The number's main function is as a measure of the [[magnetic field]], being proportional to the square of a characteristic magnetic field in a system.
 
== Definition ==
 
The Chandrasekhar number is usually denoted by the letter <math>\ Q</math>, and is motivated by a dimensionless form of the [[Navier-Stokes equation]] in the presence of a magnetic force in the equations of [[magnetohydrodynamics]]:
 
:: <math>\frac{1}{\sigma}\left(\frac{\partial^{}\mathbf{u}}{\partial t^{}}\ +\ (\mathbf{u} \cdot \nabla) \mathbf{u}\right)\ =\ - {\mathbf \nabla }p\ +\ \nabla^2 \mathbf{u}\ +\frac {\sigma}{\zeta} {Q}\ ({\mathbf \nabla} \wedge \mathbf{B}) \wedge\mathbf{B}, </math>
 
where <math>\ \sigma</math> is the [[Prandtl number]], and <math>\ \zeta</math> is the magnetic Prandtl number.  
 
The Chandrasekhar number is thus defined as:<ref>N.E. Hurlburt, P.C. Matthews and A.M. Rucklidge, "Solar Magnetoconvection," ''Solar Physics'', 192, p109-118 (2000)</ref>
 
:: <math> {Q}\ =\ \frac{{B_0}^2 d^2}{\mu_0 \rho \nu \lambda} </math>
 
where <math>\ \mu_0</math> is the [[magnetic permeability]], <math>\ \rho</math> is the [[density]] of the fluid, <math>\ \nu</math> is the [[kinematic viscosity]], and <math>\ \lambda</math> is the magnetic [[diffusivity]]. <math>\ B_0</math> and <math>\ d</math> are a characteristic magnetic field and a length scale of the system respectively.
 
It is related to the [[Hartmann number]], <math>\ H</math>, by the relation:
 
:: <math> Q\ {=}\ H^2\ </math>
 
==References==
 
<references />
 
==See also==
 
*[[Rayleigh number]]
*[[Taylor number]]
 
[[Category:Dimensionless numbers|Chandrasekhar number]]
[[Category:Magnetohydrodynamics]]

Revision as of 20:44, 16 March 2013

The Chandrasekhar number is a dimensionless quantity used in magnetic convection to represent ratio of the Lorentz force to the viscosity. It is named after the Indian astrophysicist Subrahmanyan Chandrasekhar.

The number's main function is as a measure of the magnetic field, being proportional to the square of a characteristic magnetic field in a system.

Definition

The Chandrasekhar number is usually denoted by the letter Q, and is motivated by a dimensionless form of the Navier-Stokes equation in the presence of a magnetic force in the equations of magnetohydrodynamics:

1σ(ut+(u)u)=p+2u+σζQ(B)B,

where σ is the Prandtl number, and ζ is the magnetic Prandtl number.

The Chandrasekhar number is thus defined as:[1]

Q=B02d2μ0ρνλ

where μ0 is the magnetic permeability, ρ is the density of the fluid, ν is the kinematic viscosity, and λ is the magnetic diffusivity. B0 and d are a characteristic magnetic field and a length scale of the system respectively.

It is related to the Hartmann number, H, by the relation:

Q=H2

References

  1. N.E. Hurlburt, P.C. Matthews and A.M. Rucklidge, "Solar Magnetoconvection," Solar Physics, 192, p109-118 (2000)

See also