Bulletin of the American Physical Society
66th Annual Meeting of the APS Division of Plasma Physics
Monday–Friday, October 7–11, 2024; Atlanta, Georgia
Session BP12: Poster Session I:
DIII-D and Conventional Tokamaks 1
HBT-EP and TCV
Space Plasmas
ICF1: Analytical and Computational Techniques; Machine learning and data science techniques in inertially confined plasmas; Z-pinch, X-pinch, exploding wire plasma, and dense plasma focus; Compression and burn; Magneto-inertial fusion
High Energy Density Physics
9:30 AM - 12:30 PM
Monday, October 7, 2024
Hyatt Regency
Room: Grand Hall West
Abstract: BP12.00137 : Kinetic simulations of magnetized collisionless shock experiments on the Z Machine*
Presenter:
David Schneidinger
(University of California, Los Angeles)
Authors:
David Schneidinger
(University of California, Los Angeles)
Matthew R Trantham
(University of Michigan)
Mirielle H Wong
(University of Michigan)
Carolyn C Kuranz
(University of Michigan)
Frank S. Tsung
(University of California, Los Angeles)
Paulo Alves
(University of California, Los Angeles)
Derek B Schaeffer
(University of California, Los Angeles)
Magnetized collisionless shocks are formed when a super-magnetosonic flow encounters a magnetic obstacle, and the resulting shockwave forms on length scales much shorter than the particle mean free path. Recent laboratory experiments have demonstrated the ability to drive magnetized collisionless shocks [1-2], but the exact mechanisms of particle heating and non-stationary shock behavior remain open questions due to the limited domain sizes of previous experiments. A new experimental platform, MagShockZ, has been developed to study high-Mach-number magnetized collisonless shocks over large domains on the Z Machine at Sandia National Laboratories by combining a pulsed-power-driven exploding wire array and a laser-driven magnetic piston. We present results from quasi-1D and 2D simulations that modeled the experiments using the particle-in-cell (PIC) code OSIRIS and radiative MHD code FLASH. The initial conditions for the PIC simulations were extracted from FLASH simulations of the laser-target interaction. The resulting shock formation and propagation were then modeled with OSIRIS. We use synthetic diagnostics to compare the OSIRIS results directly to experimental results.
*This work is supported by the NNSA Center of Excellence under cooperative agreement number DE-NA0004146. Simulations were conducted through the Oak Ridge Leadership Computing Facility, which is a DOE Office of Science User Facility supported under Contract DE-AC05-00OR22725.
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