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Mining experimental magnetized liner inertial fusion data: Trends in stagnation morphology

Physics of Plasmas

Laros, James H.; Yager-Elorriaga, David A.; Jennings, Christopher A.; Fein, Jeffrey R.; Shipley, Gabriel A.; Porwitzky, Andrew J.; Awe, Thomas J.; Gomez, Matthew R.; Harding, Eric H.; Harvey-Thompson, Adam J.; Knapp, Patrick F.; Mannion, Owen M.; Ruiz, Daniel E.; Schaeuble, Marc-Andre S.; Slutz, Stephen A.; Weis, Matthew R.; Woolstrum, Jeffrey M.; Ampleford, David A.; Shulenburger, Luke N.

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Hall interchange instability as a seed for helical magneto-Rayleigh–Taylor instabilities in magnetized liner inertial fusion Z-Pinches scaled from Z-Machine parameters to a next generation pulsed power facility

Physics of Plasmas

Woolstrum, Jeffrey M.; Ruiz, Daniel E.; Hamlin, Nathaniel D.; Beckwith, Kristian B.; Martin, Matthew

Magnetized liner inertial fusion (MagLIF) is a magneto-inertial-fusion concept that is studied on the 20-MA, 100-ns rise time Z Pulsed Power Facility at Sandia National Laboratories. Given the relative success of the platform, there is a wide interest in studying the scaled performance of this concept at a next-generation pulsed-power facility that may produce peak currents upward of 60 MA. An important aspect that requires more research is the instability dynamics of the imploding MagLIF liner, specifically how instabilities are initially seeded. It has been shown in magnetized 1-MA thin-foil liner Z-pinch implosion simulations that a Hall interchange instability (HII) effect can provide an independent seeding mechanism for helical magneto-Rayleigh–Taylor instabilities. Here in this paper, we explore this instability at higher peak currents for MagLIF using 2D discontinuous Galerkin PERSEUS simulations, an extended magneto-hydrodynamics code, which includes Hall physics. Our simulations of scaled MagLIF loads show that the growth rate of the HII is invariant to the peak current, suggesting that studies at 20-MA are directly relevant to 60-MA class machines.

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5 Results
5 Results