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Plasma Phys. Control. Fusion 53 (2011) 093001<br />
Topical Review<br />
Figure 56. Contour plots <strong>of</strong> ln ρ, T e , j z and pressure ρ at 130 ns from a 2D simulation <strong>of</strong> 1 <strong>of</strong><br />
32 × 15 µm Al wires in an array on MAGPIE. Reprinted with permission from [358]. Copyright<br />
2004, American Institute <strong>of</strong> Physics.<br />
For typical precursor plasma conditions, V a ∼ 10 5 ms −1 , σ ∼ 2.5 × 10 5 , <strong>the</strong> value <strong>of</strong> k −1 is<br />
not sensitive to <strong>the</strong> value <strong>of</strong> σ or V a but gives 1.3 mm to 5 mm for γ = (8–2) × 10 7 s −1 .<br />
Thus <strong>the</strong> effective skin depth for fast rising currents appears to dominate even though<br />
γ ≪ µ 0 σVa 2/4.<br />
If <strong>the</strong> wires are preheated Beg et al [362] has shown that using a linear ramp current 500 ns<br />
long <strong>of</strong> 1 kA per wire a low density precursor plasma column (n e ∼ 2 × 10 17 cm −3 ) is formed<br />
on <strong>the</strong> array axis before <strong>the</strong> start <strong>of</strong> <strong>the</strong> main current. After <strong>the</strong> main current pulse <strong>the</strong> s<strong>of</strong>t<br />
x-ray emission shows <strong>the</strong> growth <strong>of</strong> an m = 1 helical instability; without a prepulse current<br />
<strong>the</strong> precursor plasma shows no instability. The x-ray pulse at stagnation on axis is at least 30<br />
times smaller. Similar results <strong>of</strong> onset <strong>of</strong> a helical instability and reduced x-ray power was<br />
found by Lebedev et al [363] in an experiment in which additional current could be diverted<br />
into <strong>the</strong> precursor column on axis. Recent studies by Sarkisov suggest that <strong>the</strong>re is an optimum<br />
prepulse condition on current, and also a polarity issue [364]. This is developed fur<strong>the</strong>r in<br />
section 6.4 where improvements in long pulse performance is reported.<br />
In [363] <strong>the</strong>re is a study <strong>of</strong> how <strong>the</strong> ablation velocity V a varies with gap/core size, x.<br />
The mean core size was measured by x-ray radiography as 250 µm approximately when <strong>the</strong><br />
final implosion begins. The experimental results shown in figure 57 are compared with <strong>the</strong><br />
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