Study of instabilities in wire-array Z pinches at stagnation

ORAL

Abstract

Stagnation of the wire array Z pinches was studied at a 1 MA generator with imaging UV and x-ray diagnostics. Cylindrical, linear, and star wire-array Z pinches present different sets of instabilities seeded to the pinch during implosion. Compact cylindrical wire arrays implode to Z-pinches with $m=$0 necks associated with bright spots on x-ray images. The electron temperature of bright spots measured with K-shell spectroscopy is higher by 20-40{\%} compared to cold areas. Maximum x-ray power is generated by Z pinches with strong instabilities. Fast plasma motion with a velocity $>$100 km/s was observed in the Z pinch at stagnation with two-frame shadowgraphy. Plasma instabilities may present a mechanism for conversion of magnetic energy to kinetic energy. Comparison of the implosions in small-diameter cylindrical and star wire array shows that the secondary implosion of non-imploded peripheral plasma prolongs the stagnation stage and provides the enhanced x-ray production. Development of instabilities in wire arrays is in agreement with 3D MHD Gorgon simulations.

*This work was supported by DOE/NNSA under the UNR grant DE-FC52-06NA27616.

Authors

  • V.V. Ivanov

    • University of Nevada, Reno, USA
  • J.P. Chittenden

    • Imperial College, London, UK
  • R.C. Mancini

    • University of Nevada, Reno, USA
  • D. Papp

    • University of Nevada, Reno, USA
  • N. Niasse

    • Imperial College, London, UK
  • S.D. Altemara

    • University of Nevada, Reno, USA
  • A.A. Anderson

    • University of Nevada, Reno, USA