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Magnetohydrodynamics MHD


References
S. Chandrasekhar: Hydrodynamic and Hydromagnetic Stability T.G. Cowling: Magnetohydrodynamics E. Parker: Magnetic Fields B. Rossi and S. Olbert: Introduction to the Physics of Space T.J.M. Boyd and J.J Sanderson The Physics of Plasmas F. Shu: The Physics of Astrophysics, Vol. 2, Gas Dynamics

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General physical references
J.D. Jackson: Classical Electrodynamics L.D. Landau & E.M. Lifshitz: The Electrodynamics of Continuous Media E.M. Lifshitz & L.P. Pitaevskii: Physical Kinetics K. Huang: Statistical Mechanics

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Maxwell's equations (Gaussian units)
Ampere's law

Displacement current Electric current

Gauss's law of electrostatics

No magnetic monopoles

r·B

r · E = 4e =0

1 @B r E + c @t

r B =

4 1 @E Je + c c @t

=0

Faraday's law of induction

Particle equations of motion
dv v m =q E+ B dt c
Lorentz force





mr

Gravitational force 4


Cartesian form of Maxwell's equations
@ Ej @ xj @ Bj @ xj @ Bk ij k @ xj @ Ek 1 @ Bi + @ xj c @t = = = = 4 0 4 1 @ Ei Ji + c c @t 0
e

ij

k

Particle equations of motion dvi vj m = q Ei + ij k Bk dt c

@ m @ xi
5


Energy density, Poynting flux and Maxwell stress tensor
EM S
i

= = = =

EM i B ij

M

M

E ij

=

E2 + B2 = Electromagnetic energy density 8 c ij k Ej Bk = Poynting flux 4 Si = Electromagnetic momentum density 2 c 1 12 Bi Bj B ij = Magnetic component of 4 2 Maxwell stress tensor 12 1 Ei E j E ij = Electric component of 4 2 Maxwell stress tensor
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Relationships between electromagnetic energy, flux and momentum

@EM @ Si + @t @ xi @ i @ Mij @t @ xj

= =

Ji Ei Jj e Ei + ij k Bk c

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Momentum equations
Consider the em force acting on a particle vj refers to specific Fi = q Ei + ij k Bk c particle Consider a unit volume of gas and the em force acting on this volume " # # " X X vj em Fi = q Ei + ij k Bk q c where the sum is over all particles within the unit volume. N.B. The velocity here is the particle velocity not the fluid velocity.
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Momentum (cont'd)
F
em i

=

"

X


q



#

Ei + ij

k

"

X


q

vj

#

Bk

We can identify the following components

so that the electromagnetic force can be written
Jj F = e Ei + ij k Bk c 1 i . e . F = e E + J B c
em i

X


X


q



= e = Electric charge density = Ji = Electric current density

q

vj

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Momentum (cont'd)
We add the body force to the momentum equations to obtain

dvi = dt

@p @ xi

@ Jj + e Ei + ij k Bk @ xi c

Now use the equation for the conservation of electromagnetic momentum:

1 e E i + c

ij k Jj

Bk =

@ i @ Mij + @t @ xj
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Momentum (cont'd)
so that the momentum equations become:
Bulk transport of momentum Flux of momentum due to EM field
ij

@ @ (vi + i )+ ( v i v j + p @t @ xj
Mechanical + EM momentum density

Mij ) =

@ @x

i

Flux of momentum due to pressure

Gravitational force

For non-relativistic motions and large conductivity some very useful approximations are possible
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Limit of infinite conductivity
In the plasma rest frame (denoted by primes), Ohm's law is
0 Ji

=E

0 i

Conductivity

The conductivity of a plasma is very high so that for a finite current 0 Ei 0 This has implications for the lab-frame electric and magnetic field

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Transformation of electric and magnetic fields
Lorentz transformation of electric and magnetic fields vB 0 E= E+ c = Lorentz factor vE 0 B= B c
If E0 = 0

vB E+ c

=0 vB =O c vB c

)E =

This is the magnetohydrodynamic approximation.

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Maxwell tensor
Since then
M =O
E ij

E=O



vB c





v2 c2



M

B ij

Hence, we neglect the electric component of the Maxwell tensor. We can also neglect the displacement current.

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Electromagnetic momentum
We want to compare the electromagnetic momentum density with the matter momentum density, i.e. compare
1 = ij k Ej Bk 4 c 2 vB =O c2



EM i

with

vi vi = O(v )

EM i

EM i =O vi



B2 4c2


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Electromagnetic momentum
EM i =O vi B2 4c2

As we shall discover later, the quantity
B 2 2 = vA = (Alfven speed) 4
2

where the Alfven speed is a characteristic wave speed within the plasma. We assume that the magnetic field is low enough and/or the density is high enough such that
2 vA c2

and we neglect the electromagnetic momentum density.

1

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Final form of the momentum equation
Given the above simplifications, the final form of the momentum equations is:
dvi = dt @p @ xi @ @ + @ xi @ xj Bi Bj 4 B2 8

ij

We also have

1 BB curlB B = div 4 4



B I 8

2

where I is the unit tensor
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Thus the momentum equations can be written:
dv = dt rp 1 r + curlB B 4

This form can often be more useful.

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Displacement current
Let L be a characteristic length, T a characteristic time and V = L/T a characteristic velocity in the system The equation for the current is:
Ji c = ilm 4 cB O L vV =O c2 @ Bm @ xl O 1 1 @ Ei 4 @ t E vB = T cT

Displacement Current ) Curl B current

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Displacement current (cont'd)
In the MHD approximation we always put
Ji i.e. J = = c @ Bm ilm 4 @ xl c curl B 4

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Energy equation
The total electromagnetic energy density is
EM

E since

E

2

E2 + B2 B2 = 8 8 2 v 2 =O B 2 c

In order to derive the total energy equation for a magnetised gas, we add the electromagnetic energy to the total energy and the Poynting flux to the energy flux

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Energy equation (cont'd)
The final result is 2 @12 B v + + + @t 2 8
+ = h S
i

= = =

where

? vi

=

@ 12 v +h+ vi + Si @ xj 2 ds kT dt +p c ij k Ej Bk 4 2 B2 ? 1 B vi Bj vj Bi = vi 4 4 Component of velocity perpendicular to magnetic field
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The induction equation
The final equation to consider is the induction equation, which describes the evolution of the magnetic field. We have the following two equations:
Faraday's Law: Infinite conductivity: 1 @B r E + =0 c @t v E= B c

Together these imply the induction equation
@B = curl(v B) @t
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