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A review of the dense Z-pinch

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Plasma Phys. Control. Fusion 53 (2011) 093001<br />

Topical Review<br />

Under pressure balance <strong>the</strong> ratio <strong>of</strong> ion Larmor radius a i to <strong>pinch</strong> radius, a, is<br />

( )<br />

a i<br />

a = 2kB T 1/2 ( )<br />

i m 1/2<br />

i<br />

m i ZeB θ<br />

a = 2πmi 2 1/2<br />

µ o e 2 N Z(1+Z) → 8.08 × 1/2 108 N −1/2 for D +<br />

(3.15)<br />

and depends only on ion line density. The lines a i /a = 0.1 (finite ion Larmor radius or FLR)<br />

and a i /a = 1 (large ion radius or LLR) are shown in figure 16. However, FLR effects only<br />

apply if <strong>the</strong> ions are magnetized, i.e. i τ i > 1 where i is <strong>the</strong> mean ion cyclotron frequency.<br />

In terms <strong>of</strong> I, a and N under pressure balance, i τ i is given in terms <strong>of</strong> I 4 a and N by<br />

i τ i = 3<br />

64 √ 2<br />

εo 2µ5/2<br />

o<br />

m 1/2<br />

2 1/2 I 4 a<br />

i<br />

e 3 ln ii<br />

Z 3 (1+ZT e /T i ) 3/2 N → 3.64 × I 4 a<br />

5/2 1030 for D +<br />

N 5/2 (3.16)<br />

i τ i = 1 is plotted in figure 16, and it is interesting that it passes through <strong>the</strong> wedge-shaped<br />

region in which ideal MHD is applicable, indicating that, strictly, anisotropic viscosity should<br />

be employed in <strong>the</strong> R = 1–10 range. For completeness <strong>the</strong> e τ e = 1 line, with<br />

e τ e = (m i /m e ) 1/2 Z 2 i τ i (3.17)<br />

is plotted in figure 16, showing that magnetized electron transport is important for all but very<br />

resistive plasmas.<br />

We have thus constructed a universal diagram in I 4 a–N space, which determines <strong>the</strong><br />

appropriate <strong>the</strong>oretical model for an equilibrium Z-<strong>pinch</strong>. We now consider <strong>the</strong>ory and<br />

experiments in <strong>the</strong> various regimes.<br />

3.2. Ideal MHD stability<br />

The linear stability problem in ideal MHD has been shown by Bernstein et al [143] tobe<br />

reduced to <strong>the</strong> eigenvalue equation<br />

− ρ o ω 2 ξ = F (ξ), (3.18)<br />

where ρ o is <strong>the</strong> equilibrium mass density, <strong>the</strong> eigenfunction ξ is <strong>the</strong> displacement <strong>of</strong> <strong>the</strong> fluid<br />

plasma from its equilibrium position, ω 2 is <strong>the</strong> eigenvalue for a time dependence <strong>of</strong> ξ on e −iωt<br />

and <strong>the</strong> perturbed force density F is in general<br />

F (ξ) =∇(Ɣp o ∇·ξ + ξ ·∇p o ) + 1 µ o<br />

[(∇ ×B o ) ×∇×(ξ × B o )]<br />

+ 1 µ o<br />

[∇×∇×(ξ × B o )] × B o , (3.19)<br />

where p o and B o (r) are <strong>the</strong> equilibrium pressure and magnetic field, respectively, and Ɣ is<br />

<strong>the</strong> principal ratio <strong>of</strong> <strong>the</strong> specific heats. The operator F has been shown for general boundary<br />

conditions to be self-adjoint [83, 143, 144] and thus <strong>the</strong> eigenvalues ω 2 are real, positive values<br />

corresponding to stable oscillations and negative values to growing instabilities.<br />

For an infinitely long cylinder equation (3.19) can be reduced to a second order ordinary<br />

differential equation [145] <strong>of</strong> <strong>the</strong> Stürm–Liouville form<br />

d<br />

dr<br />

⌊<br />

f(r) d dr (rξ r)<br />

⌋<br />

− g(r)rξ r = 0, (3.20)<br />

where Fourier harmonics in <strong>the</strong> θ- and z-direction are considered for ξ <strong>of</strong> <strong>the</strong> form<br />

34<br />

ξ(r,t)= ξ(r)e i(mθ+kz−ωt) (3.21)

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