The Chandrasekhar number is a dimensionless quantity used in magnetic

convection Convection is single or multiphase fluid flow that occurs spontaneously due to the combined effects of material property heterogeneity and body forces on a fluid, most commonly density and gravity (see buoyancy). When the cause of the conve ...

to represent ratio of the Lorentz force to the

viscosity The viscosity of a fluid is a measure of its resistance to deformation at a given rate. For liquids, it corresponds to the informal concept of "thickness": for example, syrup has a higher viscosity than water. Viscosity quantifies the inte ...

. It is named after the

India India, officially the Republic of India (Hindi: ), is a country in South Asia. It is the seventh-largest country by area, the second-most populous country, and the most populous democracy in the world. Bounded by the Indian Ocean on the so ...

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

\ 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 Magnetohydrodynamics (MHD; also called magneto-fluid dynamics or hydromagnetics) is the study of the magnetic properties and behaviour of electrically conducting fluids. Examples of such magnetofluids include plasmas, liquid metals, ...

: ::

\frac\left(\frac\ +\ (\mathbf \cdot \nabla) \mathbf\right)\ =\ - p\ +\ \nabla^2 \mathbf\ +\frac  \ ( \wedge \mathbf) \wedge\mathbf,

where

\ \sigma

is the Prandtl number, and

\ \zeta

is the magnetic Prandtl number. The Chandrasekhar number is thus defined as:N.E. Hurlburt, P.C. Matthews and A.M. Rucklidge, "Solar Magnetoconvection," ''Solar Physics'', 192, p109-118 (2000) ::

\ =\ \frac

where

\ \mu_0

is the magnetic permeability,

\ \rho

is the

density Density (volumetric mass density or specific mass) is the substance's mass per unit of volume. The symbol most often used for density is ''ρ'' (the lower case Greek letter rho), although the Latin letter ''D'' can also be used. Mathematical ...

of the fluid,

\ \nu

is the

kinematic viscosity The viscosity of a fluid is a measure of its resistance to deformation at a given rate. For liquids, it corresponds to the informal concept of "thickness": for example, syrup has a higher viscosity than water. Viscosity quantifies the int ...

, and

\ \lambda

is the magnetic diffusivity.

\ B_0

and

\ d

are a characteristic magnetic field and a length scale of the system respectively. It is related to the

Hartmann number The Hartmann number (Ha) is the ratio of electromagnetic force to the viscous force, first introduced by Julius Hartmann (18811951) of Denmark. It is frequently encountered in fluid flows through magnetic fields. It is defined by: : \mathrm = B L\s ...

\ Ha

, by the relation: ::

Q\ \ Ha^2\

References

{{Dimensionless numbers in fluid mechanics Chandrasekhar number Magnetohydrodynamics Dimensionless numbers of fluid mechanics Fluid dynamics Astrophysics

Definition

See also

References