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

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

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

Topical Review<br />

Figure 40. Experimental implosion trajectory <strong>of</strong> a 32 × 4 µm A1 wire array on MAGPIE and<br />

implosion trajectories calculated from a model <strong>of</strong> snowplough implosion taking into account<br />

<strong>the</strong> precursor mass distribution for several cases <strong>of</strong> initial mass in <strong>the</strong> snowplough piston. The<br />

0D trajectory is also shown. Reprinted with permission from [322, figure 5]. Copyright 2002,<br />

American Institute <strong>of</strong> Physics.<br />

Figure 41. Side-on laser probing image <strong>of</strong> a 32 × 4 µm W wire array showing implosion <strong>of</strong> <strong>the</strong><br />

plasma piston onto <strong>the</strong> precursor plasma column. Reprinted with permission from [322]. Copyright<br />

2002, American Institute <strong>of</strong> Physics.<br />

implosion commences. Figure 41 is a laser probing snap-shot <strong>of</strong> an implosion at 93% <strong>of</strong> <strong>the</strong><br />

time to peak x-ray power. This implosion trajectory corresponds to a snowplough as shown by<br />

Lebedev et al [322] in <strong>the</strong> radially distributed precursor plasma. Thus it is conjectured from<br />

<strong>the</strong> trajectories and confirmed by Cuneo et al [323] at higher currents that about 40–50% <strong>of</strong><br />

<strong>the</strong> original mass is in <strong>the</strong> precursor plasma, 10–30% in <strong>the</strong> piston <strong>of</strong> <strong>the</strong> main implosion and<br />

30–40% is left behind as ‘trailing mass’. This trailing mass can be seen in figure 41 as blobs<br />

<strong>of</strong> density between azimuthally correlated gaps. 3D simulations by Chittenden et al [324]<br />

70

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

Saved successfully!

Ooh no, something went wrong!