MHD Equations for a Plasma:
Define the total mass density , the average flow velocity u, the current
density j as following: (In fully ionized plasma)
(1)
(2)
(3)
Equations of motion for ions and electrons are:
(4)
(5)
Equations of continuity for mass of ions and electrons are:
(6)
(7)
Equations of continuity for charge of ions and electrons are:
(8)
(9)
Where momentum transfer and
. They are dissipation terms related to friction and thermal force.
([2], pp.37).
The set of MHD equations can be derived by playing with above equations for ions and
electrons. They are:
Equation of motion: (10)
Equation of continuity: (11);
(12)
Generalized Ohm's law: (13)
Equation of state (adiabatic relation):
(14)
Where , is adiabatic index.
The system of equations is closed by including with Maxwell's equations:
Farady's law:
(15)
Ampere's law:
(16)
(17)
Coulomb's law:
U (18)
Usually, term is neglected.
Magnetohydrodynamics
1. The quasi-neutrality Approximation: , but
2. The "small Larmor Radius" Approximation:[9]-120
Assume that the ion Larmor radius is very small compared to the scale-length of the
fluid motion, i.e. . This is called "finite Larmor radius" treatment.
The Ohm's law becomes simple:
(19)
3. Ideal MHD approximation:
Assume that the conductivity of the plasma is infinite, which means that the plasma is
tied to the magnetic field lines. Ohm's law is simply:
(20)
4. Conservation of Magnetic Flux:
If assume plasma is a perfect conductor, the magnetic flux through any closed contour
that moves with the plasma is constant:
(21)
5. Magnetic Reynolds Number:[9]-127~128
How good must a plasma's conductivity be that ideal MHD is valid? This is decided by
the magnetic Reynolds number: (22)
where L is characteristic scale-length, and u a characteristic plasma velocity.
If is high enough, the perfect conductor assumption is valid. For fully
developed magnetohydrodynamic motion, the characteristic velocities are very large,
and magnetic Reynolds number in low-resistivity plasmas can range up to
, or
higher.[9]