Resistive diffusion and radiative cooling effects in magnetized oblique shocks
R. Datta, E. Neill, E. Freeman, E. S. Lavine, S. Chowdhry, L. Horan IV, W. M. Potter, D. A. Hammer, B.R. Kusse, and J.D. Hare

TL;DR
This study investigates magnetized oblique shocks in plasmas, demonstrating how resistive diffusion and radiative cooling influence shock structure and behavior through experiments on a pulsed power facility.
Contribution
It provides the first experimental analysis of perpendicular-type oblique shocks considering both resistive diffusion and radiative cooling effects.
Findings
Shocks show shallower angles and higher density compression than Rankine-Hugoniot predictions.
Experimental results align with a model including resistive diffusion and radiative cooling.
Oblique shocks can support magnetic field compression in plasma systems.
Abstract
Magnetized oblique shocks are of interest in various plasmas, including in astrophysical systems, magneto-inertial confinement fusion experiments, and in aerospace applications. Through experiments on the COBRA pulsed power facility (Cornell University, 1~MA peak current, 100~ns rise time), we investigate oblique shock formation in a system with a magnetic field, and where both radiative cooling and resistive diffusion are important. Compared to previous pulsed power experiments, which have investigated quasi-parallel oblique shocks, here we consider perpendicular-type shocks, which can support magnetic field compression. In our experiments, supersonic, super-Alfv\'enic, collisional plasma flows, generated using an aluminum exploding wire array, are deflected by angled obstacles to generate oblique shocks. The shocks are imaged using laser shadowgraphy and Mach-Zehnder interferometry,…
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