Simulation of K-$\alpha$ Emission from Highly Charged Cu ions for Pinches on ZR

POSTER

Abstract

Recent spectral data of Cu shots Z1975 and Z2122 from Sandia's ZR machine are believed to show strong K-$\alpha $ emissions. As these K-$\alpha $ lines provide good diagnostics, a detailed spectral model will be developed to investigate these line emissions for analyzing the data. In a Z pinch plasma, K-$\alpha $ emission can occur due to e-beams, hot electrons at the tail of a Maxwellian and also pumping from hot photons emitted near the axis. K-$\alpha $ emission that originates from collisional processes involving hot electrons in the final phase of the pinching plasmas are associated with radiationless electron capture, inner-shell electron collisional excitation and ionization. K-$\alpha $ lines from various ionization stages of various materials such as Fe, Cr, Ni, and Mn were also observed in the ZR data. Contributions from ions with strong K-$\alpha $ transitions will be included for this study which is a preliminary attempt to investigate Cu K-$\alpha $ lines due to hot electrons and photons. Photo-pumped K-$\alpha $ emission from an outer shell is spatially distinguishable from that produced by e-beam on axis.

*Work supported by DOE/NNSA. Sandia is a multi-program laboratory operated by Sandia Corporation, a Lockheed Martin Company, for the United States Department of Energy's National Nuclear Security Administration under contract DE-AC04-94AL85000.

Authors

  • A. Dasgupta

    • Naval Research Laboratory, Washington, DC
  • J.L. Giuliani

    • Naval Research Laboratory, Washington, DC
  • R.W. Clark

    • Berkeley Scholars Inc., Springfield, VA
  • N.D. Ouart

    • NRC/NRL Post Doc
  • B. Jones

    • Sandia National Laboratories, Albuquerque, NM
  • D.J. Ampleford

    • Sandia National Laboratories, Albuquerque, NM