Published December 2008 | Version v1
Journal article

Implosion dynamics and K-shell x-ray generation in large diameter stainless steel wire array Z pinches with various nesting configurations

  • 1. Sandia National Laboratories, Albuquerque, New Mexico 87185 (United States)
  • 2. Ktech Corporation, Albuquerque, New Mexico 87123 (United States)
  • 3. Naval Research Laboratory, Washington, D.C. 20375 (United States)
  • 4. Berkeley Scholars, Springfield, Virginia 22150 (United States)
  • 5. Blackett Laboratory, Imperial College, London, SW7 2BW (United Kingdom)

Description

Nested stainless steel wire array variations were investigated on the 20 MA Z machine [R. B. Spielman et al., Phys. Plasmas 5, 2105 (1998)]. In order to reach experimentally observed electron temperatures near 3.8 keV and excite the K shell, these ∼6.7 keV photon energy x-ray sources must be of large initial diameter (45-80 mm) which poses a concern for magnetic Rayleigh-Taylor instability growth. We discuss the implosion dynamics in these large diameter wire arrays, including an analysis of the ablation phase indicating that the prefill material is snowplowed at large radius. Nested array configurations with various mass and radius ratios are compared for instability mitigation and K-shell scaling. Degradation of the K-shell x-ray power and yield was observed for shots that did not have simultaneous implosion of the outer and inner wire arrays. Shots that were designed per this constraint exhibited K-shell yield scaling consistent with the model of J. W. Thornhill et al. [IEEE Trans. Plasma Sci. 34, 2377 (2006)] which had been benchmarked to single array results. This lends confidence to K-shell yield predictions using this model for future shots on the refurbished Z machine. Initial results employing a triple nested wire array to stabilize the large diameter implosion are also reported.

Additional details

Identifiers

Publishing Information

Journal Title
Physics of Plasmas
Journal Volume
15
Journal Issue
12
Journal Page Range
p. 122703-122703.21
ISSN
1070-664X
CODEN
PHPAEN

Optional Information

Notes
(c) 2008 American Institute of Physics