Grad-Shafranov equation

Grad-Shafranov equation

!MHD
!Plasma

The Grad-Shafranov equation (H. Grad and H. Rubin (1958) Shafranov (1966) ) is the equilibrium equation in ideal magnetohydrodynamics (MHD) for a two dimensional plasma, for example the axisymmetric toroidal plasma in a tokamak. This equation is a two-dimensional, nonlinear, elliptic partial differential equation obtained from the reduction of the ideal MHD equations to two dimensions, often for the case of toroidal axisymmetry (the case relevant in a tokamak). Interestingly the flux function psi is both a dependent and an independent variable in this equation:

Delta^{*}psi = -mu_{0}R^{2}frac{dp}{dpsi}-Ffrac{dF}{dpsi}

where mu_0 is the magnetic permeability, p(psi) is the pressure, F(psi)=RB_{phi}

and the magnetic field and current are given by

vec{B}=frac{1}{R} ablapsi imes hat{e_{phi+frac{F}{R}hat{e}_{phi}

mu_0vec{J}=frac{1}{R}frac{dF}{dpsi} ablapsi imes hat{e_{phi-frac{1}{R}Delta^{*}psi hat{e}_{phi}

The elliptic operator

:Delta^{*} is given byDelta^{*}psi = Rfrac{partial}{partial R}left(frac{1}{R}frac{partial psi}{partial R} ight)+frac{partial^2 psi}{partial Z^2}.

The nature of the equilibrium, whether it be a tokamak, reversed field pinch, etc. is largely determined by the choices of the two functions F(psi) and p(psi) as well as the boundary conditions.

Derivation:
To begin we assume that the system is 2-dimensional with z as the invariant axis, i.e. partial /partial z = 0 for all quantities.Then the magnetic field can be written in cartesian coordinates as

: old{B} = (partial A/partial y,-partial A /partial x,B_z(x,y))

or more compactly,

: old{B} = abla A imes hat{old{z + hat{old{z B_z,

where A(x,y)hat{old{z is the vector potential for the in-plane (x and y components) magnetic field. Note that based on this form for B we can see that "A" is constant along any given magnetic field line, since abla A is everywhere perpendicular to B. (Also note that -A is the flux function psi mentioned above.)

Two dimensional, stationary, magnetic structures are described by the balance of pressure forces and magnetic forces, i.e.:

: abla p = old{j} imes old{B},

where "p" is the plasma pressure and j is the electric current. Note from the form of this equation that we also know "p" is a constant along any field line, (again since abla p is everywhere perpendicular to B. Additionally, the two-dimensional assumption (partial / partial z ) means that the z- component of the left hand side must be zero, so the z-component of the magnetic force on the right hand side must also be zero. This means that old{j}_perp imes old{B}_perp = 0, i.e. old{j}_perp is parallel to old{B}_perp.

We can break the right hand side of the previous equation into two parts::old{j} imes old{B} = j_z (hat{old{z imes old{B_perp}) +old{j_perp} imes hat{old{zB_z ,

where the perp subscript denotes the component in the plane perpendicular to the z-axis. The z component of the current in the above equation can be written in terms of the one dimensional vector potential asj_z = - abla^2 A/mu_0. . The in plane field is
:old{B}_perp = abla A imes hat{old{z ,
and using Ampère's Law the in plane current is given by
:old{j}_perp = (1/mu_0) abla B_z imes hat{old{z.
In order for this vector to be parallel to old{B}_perp as required, the vector abla B_z must be perpendicular to old{j}_perp, and B_z must therefore, like p be a field like invariant.

Rearranging the cross products above, we see that that
:hat{old{z imes old{B}_perp = abla A ,
and
:old{j}_perp imes B_zold{hat{z = -(1/mu_0)B_z abla B_z
These results can be substituted into the expression for abla p to yield:
: abla p = - [(1/mu_0) abla^2 A] abla A-(1/mu_0)B_z abla B_z.

Now, since p and B_perp are constants along a field line, and functions only of A, we note that abla p = (d p /dA) abla A and abla B_z = (d B_z/dA) abla A. Thus, factoring out abla A and rearraging terms we arrive at the Grad Shafranov equation:
: abla^2 A = -mu_0 frac{d}{dA}(p + frac{B_z^2}{2mu_0})

References

* Grad.H, and Rubin, H. (1958) "Hydromagnetic Equilibria and Force-Free Fields". Proceedings of the 2nd UN Conf. on the Peaceful Uses of Atomic Energy, Vol. 31, Geneva: IAEA p.190.
* Shafranov, V.D. (1966) Plasma equilibrum in a magnetic field, "Reviews of Plasma Physics", Vol. 2, New York: Consultants Bureau, p. 103.


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