14.03.2014 Views

A review of the dense Z-pinch

A review of the dense Z-pinch

A review of the dense Z-pinch

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

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 />

79

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!