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A review of the dense Z-pinch

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

Topical Review<br />

was always in <strong>the</strong> direction from cathode to anode. No attempt was made to remove perturbing<br />

fields such as <strong>the</strong> Earth’s field [557], and it also was not possible to reverse <strong>the</strong> polarity <strong>of</strong><br />

<strong>the</strong> <strong>pinch</strong>. In [53] <strong>the</strong> accretion problem was addressed, and it was suggested that by current<br />

programming to have a larger rate <strong>of</strong> rise, compression <strong>of</strong> <strong>the</strong> hot <strong>pinch</strong> will occur.<br />

A variant <strong>of</strong> this was explored by Soto et al [54] who employed two stainless-steel conical<br />

hollow electrodes with 2 mm diameter with edges <strong>of</strong> 50 µm radius <strong>of</strong> curvature. A microdischarge<br />

was set up between <strong>the</strong>se. Then a few nanoseconds before <strong>the</strong> application <strong>of</strong> <strong>the</strong><br />

main current a pulsed laser was focused through <strong>the</strong> anode on to <strong>the</strong> cathode. Thus two parallel<br />

conductive paths for <strong>the</strong> current were set up. With a peak current <strong>of</strong> 130 kA, interferograms<br />

showed a peak electron density <strong>of</strong> 3 × 10 25 m −3 on axis. The outer annular hydrogen plasma<br />

coalesced with <strong>the</strong> central column and <strong>the</strong>re was a compression <strong>of</strong> <strong>the</strong> <strong>pinch</strong> from 1 mm to an<br />

equilibrium radius <strong>of</strong> 50 µm. The Alfvén transit time was estimated to be 14 ns, and <strong>the</strong> line<br />

density grew to 1.3 × 10 19 m −1 . This early increase in N is not maintained, inferring that <strong>the</strong><br />

neutral gas does not cross <strong>the</strong> <strong>pinch</strong> boundary. The <strong>pinch</strong> appeared to be stable at a temperature<br />

<strong>of</strong> 150 eV. The enhanced stability is proposed to be due to resistivity at early times, and later<br />

due to FLR because a i /a is about 0.1. It could be worthwhile to extend this compressional gasembedded<br />

<strong>pinch</strong> to higher currents. So far with no observations <strong>of</strong> neutrons or x-rays, <strong>the</strong>re are<br />

no disruptions, <strong>the</strong> achievable temperatures by Joule heating alone are ra<strong>the</strong>r modest. This idea<br />

<strong>of</strong> employing compression both to insulate <strong>the</strong> plasma from accretion from <strong>the</strong> neutrals outside,<br />

and to have more heating has been followed up by Veloso et al [558] using a laser-initiated<br />

hollow gas-embedded Z-<strong>pinch</strong>. The peak current <strong>of</strong> 150 kA led to an implosion velocity <strong>of</strong><br />

5kms −1 , and <strong>the</strong> plasma column remained hollow and stable for 10 Alfvén transit times at a<br />

Bennett temperature <strong>of</strong> 150 eV.<br />

7.5. Single wire and frozen deuterium fibre <strong>pinch</strong>es<br />

For single fibres distinction between insulating and conducting materials should be made at<br />

<strong>the</strong> earliest stage <strong>of</strong> electrical breakdown and plasma formation. As found by Beg et al [254],<br />

for insulators breakdown was observed to proceed from <strong>the</strong> cathode, coincident with a pulse <strong>of</strong><br />

hard x-rays associated with an electron beam <strong>of</strong> about 4 kA and >50 keV. This was consistent<br />

with a magnetron type <strong>of</strong> condition,<br />

√<br />

2me V<br />

I = 2πr 0<br />

(7.15)<br />

µ 0 d e<br />

in a radius r 0 ≫ a, <strong>the</strong> fibre radius. This is r 0 /d times <strong>the</strong> Alfvén-Lawson limiting current [95],<br />

(see section 2.2). Carbon and frozen hydrogen or deuterium are examples <strong>of</strong> insulators used,<br />

while conductors such as aluminium, tungsten, copper and nickel have been widely explored.<br />

The subject <strong>of</strong> exploding wires has a ra<strong>the</strong>r different motivation, but indeed it characterizes<br />

that all fibres initially explode with a typical velocity <strong>of</strong> 10 4 ms. This is illustrated in figure 81<br />

in an optical radial streak <strong>of</strong> images <strong>of</strong> a 25 µm aluminium fibre taken on <strong>the</strong> IMP generator<br />

in which <strong>the</strong> current rises to 80 kA in 60 ns. The exploding plasma around <strong>the</strong> fibre carries <strong>the</strong><br />

rising current, but at this stage <strong>the</strong> J × B <strong>pinch</strong> force is insufficient to overcome <strong>the</strong> plasma<br />

pressure, rising under Joule heating. Thus here is ano<strong>the</strong>r example <strong>of</strong> <strong>the</strong> current being less than<br />

that given by <strong>the</strong> Haines–Hammel curve [103–105]. As <strong>the</strong> current increases fur<strong>the</strong>r, however,<br />

simulations [197] show that a re-compression occurs accompanied by <strong>the</strong> onset <strong>of</strong> <strong>the</strong> m = 0<br />

MHD instability. The experimental data and simulation are shown in figure 82. It is interesting<br />

that here <strong>the</strong> simulation reproduces from noise <strong>the</strong> same wavelength <strong>of</strong> instability as occurs<br />

in <strong>the</strong> experiment, i.e. <strong>the</strong> resistive MHD approximation is adequate. Thus <strong>the</strong> fibre <strong>pinch</strong><br />

is dominated at <strong>the</strong> stage <strong>of</strong> confinement by <strong>the</strong> m = 0 instability. Fur<strong>the</strong>rmore, Chittenden<br />

122

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