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Plasma Phys. Control. Fusion 53 (2011) 093001<br />
Topical Review<br />
Figure 51. A side-on laser shadowgram <strong>of</strong> a 16 × 15 µm Al wire array on MAGPIE at 180 ns after<br />
<strong>the</strong> start <strong>of</strong> <strong>the</strong> current [65]. On <strong>the</strong> right is a similar result from a tungsten 16 × 7.5 µm array.<br />
Reprinted with permission from [65]. Copyright 2001, American Institute <strong>of</strong> Physics.<br />
between wires so that inside <strong>the</strong> current-carrying region, <strong>the</strong> closed line integral ∮ B · dl is<br />
zero. Yu [338] found that <strong>the</strong> ablation process was confined to an almost azimuthally symmetric<br />
private flux region with R m < 1, and, as described above, developed a <strong>the</strong>ory for <strong>the</strong> mass<br />
ablation rate.<br />
The mass ablation rate ṁ was very successfully modelled phenomenologically by Lebedev<br />
et al [65] in a rocket model. Assuming R m ≪ 1 and that all <strong>the</strong> current flows in a narrow<br />
shell-like region, <strong>the</strong> magnetomotive force leads to ejection <strong>of</strong> <strong>the</strong> precursor plasma with an<br />
ablation velocity V a which experimentally is found to be a constant for each material during a<br />
discharge, <strong>the</strong> rocket equation gives<br />
ṁ =− µ 0I 2<br />
4πRV a<br />
(kg m −1 s −1 ). (5.1)<br />
Knowing all <strong>the</strong> terms on <strong>the</strong> rhs from experiment ṁ can be found and integrated in time to<br />
find <strong>the</strong> mass that has been ablated up to any time t. V a is typically 10 5 ms −1 .<br />
A model developed by <strong>the</strong> Angara group [339] gave a slightly modified equation for<br />
tungsten<br />
ṁ ∗ =−0.4π I 1.8 (MA)<br />
R 0.8 (cm) (µgcm−1 ns −1 ), (5.2)<br />
where <strong>the</strong> ablation velocity is implicitly included. Cuneo et al [323] claim that both formulae<br />
agree with experiment within <strong>the</strong> accuracy <strong>of</strong> measurement. Yu et al [338] also provide scaling<br />
laws but in terms <strong>of</strong> current and wire core radius and wire number.<br />
A side-on laser shadowgram, figure 51, clearly shows both <strong>the</strong> inward filamentary<br />
precursor flow with a wavelength <strong>of</strong> ∼0.5 mm in Al and <strong>the</strong> accumulated precursor cylinder<br />
on axis. As can be seen from <strong>the</strong> radial streak picture in figure 52, <strong>the</strong> precursor arrives on axis<br />
in MAGPIE at approximately half <strong>the</strong> time to full implosion, and is a bright emitter. Figure 53<br />
shows gated s<strong>of</strong>t x-ray images <strong>of</strong> precursor in carbon, aluminium and tungsten. In all cases<br />
<strong>the</strong> cylindrical column is straight with no sign <strong>of</strong> MHD instabilities, consistent with it carrying<br />
negligible current. The confinement <strong>of</strong> <strong>the</strong> column is because <strong>of</strong> <strong>the</strong> ρVa<br />
2 kinetic pressure <strong>of</strong><br />
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