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Plasma Phys. Control. Fusion 53 (2011) 093001<br />
Topical Review<br />
Figure 52. A radial streak picture <strong>of</strong> a typical wire array on MAGPIE. Reprinted with permission<br />
from [65]. Copyright 2001, American Institute <strong>of</strong> Physics.<br />
Figure 53. Gated s<strong>of</strong>t x-ray images <strong>of</strong> <strong>the</strong> precursor column in carbon, aluminium and tungsten<br />
taken on MAGPIE. Reprinted with permission from [65]. Copyright 2001, American Institute <strong>of</strong><br />
Physics.<br />
<strong>the</strong> precursor streams impinging on it. Because <strong>of</strong> radiative cooling <strong>of</strong> <strong>the</strong> higher Z plasma<br />
<strong>the</strong>re is a radial contraction <strong>of</strong> <strong>the</strong> column in W; <strong>the</strong> diameters <strong>of</strong> <strong>the</strong> columns in MAGPIE<br />
are 3 mm for C, 1.25 for Al and 0.2 mm for W. Benjamin et al [350] and Aivazov et al [319]<br />
earlier had shown <strong>the</strong> formation <strong>of</strong> a precursor column.<br />
In a hybrid r −θ Monte Carlo treatment <strong>of</strong> <strong>the</strong> Fokker–Planck equation Sherlock et al [351]<br />
show that for tungsten <strong>the</strong> precursor flow is relatively collisionless, while for aluminium it<br />
becomes collisional almost immediately a significant amount <strong>of</strong> plasma arrives on axis. The<br />
precursor column forms after a critical density occurs on axis through convergence, allowing<br />
a nonlinear compression by collisional interaction with <strong>the</strong> incoming streams. The W ions are<br />
more collisionless than Al ions because <strong>the</strong> W ions have a higher kinetic energy (because <strong>of</strong><br />
<strong>the</strong>ir higher atomic mass), causing an increase in <strong>the</strong> mean-free path not compensated by <strong>the</strong><br />
higher Z value. Figure 54 shows <strong>the</strong> evolution <strong>of</strong> ion number density pr<strong>of</strong>ile with time and<br />
also <strong>the</strong> ion–ion mean-free path and ion temperature. In contrast as shown by experimental<br />
end-on laser probing by Lebedev et al [352] in figure 55, <strong>the</strong> Al is more collisional and shock<br />
interactions between individual streams can be seen.<br />
The low magnetic Reynolds number in <strong>the</strong> ablation zone was first shown by Haines [230]<br />
in a 3D analytic model <strong>of</strong> <strong>the</strong> ablation process in <strong>the</strong> presence <strong>of</strong> localized m = 0 necks in which<br />
Joule heating was concentrated. This led to flux limited heat flow to <strong>the</strong> cores, this providing<br />
<strong>the</strong> energy for ionization and ablation. (It should be noted that while radiation transport<br />
is dominant in <strong>the</strong> outer regions, <strong>the</strong> final heat flow to <strong>the</strong> cold cores is <strong>the</strong>rmal transport.)<br />
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