• DocumentCode
    3215664
  • Title

    Current rise-rate scaling for radial wire arrays

  • Author

    Mitchell, M.D. ; Chandler, K.M. ; Bland, S. ; Suzuki, F. ; Hall, G. ; Thomson, A.H. ; Lebedev, S.V. ; Chittenden, J.P. ; McBride, R. ; Pikuz, S.A. ; Shelkovenko, T.A. ; Hammer, D.A. ; Kusse, B.R.

  • Author_Institution
    Idaho State Univ., Pocatello, ID, USA
  • fYear
    2009
  • fDate
    1-5 June 2009
  • Firstpage
    1
  • Lastpage
    1
  • Abstract
    Summary form only given. Radial wire arrays offer the potential for higher energy density of radiated x-rays compared to cylindrical arrays. Higher radiated energy density would allow for more compact hohlraums thus easing power requirements for ICF. In an effort to explore how radiated power scales with the rise-rate of the current we performed experiments on two 1 MA pulsed power generators with very different rise ratesacirceurordquo MAGPIE at Imperial College with about 300 ns rise time and COBRA at Cornell with about 100 ns rise time. Comparisons of radiated power from 16-wire Al and Cu arrays over a range of masses are presented. Results from these initial experiments suggest that radiated power for a given material is similar when implosion times are matched to the current rise time. We also present comparisons of radiated power from modified array geometries such as wire length and cathode diameter. Some results from Ti/Ni and Fe/Ni arrays are also presented.
  • Keywords
    plasma X-ray sources; plasma diagnostics; MAGPIE; current rise-rate scaling; cylindrical arrays; pulsed power generators; radial wire arrays; radiated energy density; radiated x-rays; Cathodes; Educational institutions; Geometry; Iron; Potential energy; Power generation; Pulse generation; US Department of Energy; Wire; X-rays;
  • fLanguage
    English
  • Publisher
    ieee
  • Conference_Titel
    Plasma Science - Abstracts, 2009. ICOPS 2009. IEEE International Conference on
  • Conference_Location
    San Diego, CA
  • ISSN
    0730-9244
  • Print_ISBN
    978-1-4244-2617-1
  • Type

    conf

  • DOI
    10.1109/PLASMA.2009.5227514
  • Filename
    5227514