Spectroscopic study of z-pinch stagnation

POSTER

Abstract

Fast z-pinches provide intense 1-10 keV photon energy radiation sources. Here, we analyze time-, space-, and spectrally- resolved $\sim$2 keV K-shell emissions from Al (5$\%$ Mg) wire array implosions on Sandia$'$s Z machine pulsed power driver. The stagnating plasma is modeled as three separate radial zones, and collisional-radiative modeling with radiation transport calculations are used to constrain the temperatures and densities in these regions, accounting for K-shell line opacity and Doppler effects. We discuss plasma conditions and dynamics at the onset of stagnation, and compare inferences from the atomic modeling to three-dimensional magneto-hydrodynamic simulations.

Authors

  • B. Jones

    Sandia National Laboratories, Sandia Nat. Lab., Sandia National Labs

  • C.A. Jennings

    Sandia National Labs, Sandia National Laboratories

  • E.P. Yu

    Sandia National Labs, Sandia National Laboratories

  • S.B. Hansen

    Sandia National Laboratories

  • Greg Rochau

    Sandia National Laboratories, Sandia National Labs

  • Jim Bailey

    Sandia National Laboratories, Sandia National Labs

  • C.A. Coverdale

    Sandia National Labs, SNL, Sandia National Laboratories, Sandia Nat. Lab., Sandia National Laboratories, Albuquerque

  • D.J. Ampleford

    Sandia National Laboratories

  • M. Cuneo

    Sandia National Labs, Sandia National Laboratories

  • Yitzhak Maron

    Weizmann Institute of Science, Weizmann Institute

  • V. Fisher

    Weizmann Institute

  • V. Bernshtam

    Weizmann Institute

  • A. Starobinets

    Weizmann Institute

  • L. Weingarten

    Weizmann Institute