13:15 〜 13:40
[HEDS13-01(Invited)] Structure of Reverse Shocks and Radiative Cooling Effects in High Energy Density Plasma Experiments
Accretion shocks, common in many astrophysical systems, can be significantly influenced by radiative cooling effects, resulting in instabilities and turbulence. This study investigates accretion shock experiments at the MAGPIE pulsed power facility using two different approaches. The first approach examines reverse shocks resulting from the collision of supersonic, magnetized plasma flows produced by an inverse wire array interacting with a planar conducting obstacle. The second approach involves the ablation of solid targets by X-ray radiation from a Z-pinch wire array.
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