Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session GP11: Poster Session III: Basic Plasma Physics: General; Space and Astrophysical Plasmas; ICF Measurement and Computational Techniques, Direct and Indirect Drive; MIF Science and Technology (9:30am-12:30pm)
Tuesday, November 6, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.GP11.123
Abstract: GP11.00123 : Assessment of High-β Magnetized Target Formation and Plasma-Liner Nonuniformities in Plasma-Jet-Driven Magneto-Inertial Fusion using the FLASH Code*
Presenter:
Tom Byvank
(Los Alamos National Laboratory)
Authors:
Tom Byvank
(Los Alamos National Laboratory)
Samuel Langendorf
(Los Alamos National Laboratory)
Scott C Hsu
(Los Alamos National Laboratory)
Petros Tzeferacos
(Univ of Chicago)
Y C Francis Thio
(US Dept of Energy-Germantown)
The Plasma Liner Experiment (PLX) is being used to explore a potentially lower-cost fusion-energy concept by which an imploding spherical plasma liner will compress a magnetized plasma target to fusion conditions [1,2], a concept known as plasma-jet-driven magneto-inertial fusion (PJMIF). The liner is produced by merging of supersonic plasma jets, and each jet is generated by a coaxial plasma gun. Using the FLASH code, we study possible formation of a high-β magnetized target (β > 1, ωiτi > 1) by merging pre-magnetized jets [3]. Furthermore, we characterize how liner nonuniformities degrade the implosion during target compression. Adaptive mesh refinement in FLASH permits study of shock structures formed by the merging jets and their consequences in 2D and 3D. We compare FLASH results for target compression with recent relevant 1D simulation results [4,5]. The FLASH results will help guide experiments and continued assessment of the PJMIF concept.
[1] S. C. Hsu et al., IEEE Trans. Plasma Sci. 40, 1287 (2012); [2] S. C. Hsu et al., ibid 46, 1951 (2018); [3] S. C. Hsu and S. J. Langendorf, J. Fusion Energy, Accepted (2018); [4] C. E. Knapp and R. C. Kirkpatrick, Phys. Plasmas 21, 070701 (2014); [5] S. J. Langendorf and S. C. Hsu, ibid 24, 032704 (2017).
*LANL LDRD Program
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.GP11.123
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