$(\mathrm{T}_{1/4}\sim 1\mu \ma"/>

Axial Plasma Jet Characterization on a Microsecond X-Pinch

2018 IEEE International Conference on Plasma Science (ICOPS)(2018)

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Abstract
The jets produced on a microsecond x-pinch $(\mathrm{T}_{1/4}\sim 1\mu \mathrm{s}$ , dl/dt ~ 0.35 kA/ns) have been studied through light-field schlieren imaging and optical framing photographs across 4 different materials: Al, Ti, Mo, and W. The axial velocity of the jets was measured and exhibited no dependence on atomic number (Z) of the wire material. There may be a dependence on another factor(s), namely current rise rate. The average axial jet velocity across all four materials was measured to be 2.9 $\pm 0.5\times 10$ cm/s. The average jet diameter and the average radial jet expansion rate displayed inverse relationships with $\mathrm{Z}$ , which may be attributed to radiative cooling effects. Asymmetry between the anode and cathode jet behavior was observed and is thought to be caused by electron beam activity. The mean divergence angle of the jet was found to vary with wire material and correlated inversely with the thermal conductivity of the cold wire. Optical images indicated a two-layer structure in Al jets which may be caused by standing shocks and resemble phenomena observed in astrophysical jet formation and collimation. Kinks in the jets have also been observed which may be caused by $\mathrm{m}=1$ MHD instability modes or by interaction of the jet with the electrode plasma. Results of recent interferometry and x-ray spectroscopy experiments will also be presented.
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Key words
axial plasma jet characterization,microsecond x-pinch,light-field schlieren imaging,optical framing photographs,axial velocity,wire material,axial jet velocity,jet diameter,radial jet expansion rate,cathode jet behavior,optical images,Al jets,astrophysical jet formation,MHD instability modes
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