Challenges to understanding radiative shocks

ORAL

Abstract

Shock waves driven above a threshold velocity near 100 km/s become strongly radiative, converting most of the incoming energy flux into radiation. We produce such shock waves in Xe or Ar by using a laser to shock, ionize, and accelerate a Be plate into a gas-filled shock tube. Structure develops in these systems due to both radiative energy transfer and hydrodynamic instability. We are conducting such experiments, implementing a code to model them, and implementing software to assess the predictive capability of the code in our Center for Radiative Shock Hydrodynamics. This presentation will discuss the challenges and show our progress.

*Supported by the DOE NNSA under the Predictive Sci. Academic Alliance Program by grant DE-FC52-08NA28616, the Stewardship Sci. Academic Alliances program by grant DE-FG52-04NA00064, and the Nat. Laser User Facility by grant DE-FG03-00SF22021.

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Authors

  • Paul Drake

    • University of Michigan

  • F.W. Doss

    • University of Michigan

  • B. Fryxell

    • University of Michigan

  • M.J. Grosskopf

    • University of Michigan
    • Univeristy of Michigan

  • J.P. Holloway

    • University of Michigan

  • B. van der Holst

    • University of Michigan

  • C. Huntington

    • University of Michigan

  • C.C. Kuranz

    • University of Michigan

  • E.S. Myra

    • University of Michigan

  • K.G. Powell

    • University of Michigan

  • I.V. Sokolov

    • University of Michigan

  • Q.F. Stout

    • University of Michigan

  • G. Toth

    • University of Michigan

  • A.J. Visco

    • University of Michigan