Radiative shock experiments on LIL and Gekko

POSTER

Abstract

For more than a decade, we have currently performed laboratory experiments in connection with astrophysical phenomena in order to improve our understanding in the field of radiation hydrodynamics so to validate numerical schemes and assumptions in simulations. Here, recent experimental results on highly radiative shocks generated by high-power lasers such as Gekko (Japan) and LIL (laser integration line) are presented. Many visible diagnostics were implemented (interferometry, self-optical pyrometry, 2D snapshot imagers) providing measurements of the shock and precursor velocities, temperature, electronic density and 2D shock front shape. Results will be compared with 2D radiation hydrodynamic simulations

Authors

  • Michel Koenig

    • Laboratoire LULI - CNRS, France
    • LULI, Ecole Polytechnique
  • Roman Yurchak

    • Laboratoire LULI - CNRS, France
  • Claire Michaut

    • LUTH, France
  • Patrice Barroso

    • LUTH, France
  • Emeric Falize

    • CEA DAM - DIF, France
  • Alexis Casner

    • CEA DAM - DIF, France
    • CEA, DAM, DIF, F-91297 Arpajon Cedex, France
  • Stephane Laffite

    • CEA DAM - DIF, France
    • CEA, DAM, DIF
  • Serge Bouquet

    • CEA DAM - DIF, France
  • Youichi Sakawa

    • ILE, Osaka, Japan
  • Taichi Morita

    • Kyushu University, Japan
  • R. Paul Drake

    • University of Michigan: Ann Arbor
    • University of Michigan
    • Department of Atmospheric, Oceanic, and Space Sciences, U. of Michigan, USA
    • University of Michigan, USA
    • Univ of Michigan - Ann Arbor
  • Alexander Pelka

    • Helmholtz-Zentrum Dresden-Rossendorf, U. Dresden, Germany
  • S. Le Pape

    • LLNL, USA
    • LLNL
    • Lawrence Livermore National Laboratory