Bulletin of the American Physical Society
65th Annual Meeting of the APS Division of Plasma Physics
Monday–Friday, October 30–November 3 2023; Denver, Colorado
Session BO06: Magneto-Inertial Fusion, Z-pinches, X-pinches & Pulsed Power-Driven Plasmas
9:30 AM–12:30 PM,
Monday, October 30, 2023
Room: Governor's Square 15
Chair: David Strozzi, Lawrence Livermore Natl Lab
Abstract: BO06.00004 : Proton Radiography of Bounded, Magnetized Plasma relevant to MagLIF*
10:06 AM–10:18 AM
Presenter:
Sophia Malko
(Princeton Plasma Physics Laboratory)
Authors:
Sophia Malko
(Princeton Plasma Physics Laboratory)
Chris A Walsh
(Lawrence Livermore National Laboratory)
Jeffrey Fein
(Sandia National Laboratories)
Adam Harvey-Thompson
(Sandia National Laboratories)
Daniel E Ruiz
(Sandia National Laboratories)
Matt Weis
(Sandia National Laboratories)
Jesse Griff-McMahon
(Princeton University)
Vicente Valenzuela-Villaseca
(Princeton University)
Derek B Schaeffer
(University of California, Los Angeles)
Gennady Fiksel
(University of Michigan)
Cameron A Frank
(University of Delaware)
Arijit Bose
(University of Delaware)
William R Fox
(Princeton Plasma Physics Laboratory)
Here we report on a new experimental platform at OMEGA to study blast wave dynamics and subsequent physics of confinement of magnetic field and plasma energy in a laser-heated gas liner. The experimental parameters were scaled to study the preheating phase physics of MagLIF. The geometry consists of a laser-heated cylindrical gas cell with a thin wall (liner), applied magnetic field parallel to the liner axis, and laser heating parallel to the axis and magnetic field produced by MIFEDS. Proton radiography with 3 and 15 MeV monoenergetic protons produced from a DHe3 implosion was be used to measure the magnetic fields at several times [2], while the conditions of the plasma in liner were characterized by collecting X-ray emission using X-ray Framing Camera.
We have observed the Nernst advection of magnetic field in liner at early expansion times and the interaction of the blast wave with the liner walls at later times, which led to fluctuation of magnetic flux. These results are compared with HYDRA and GORGON simulations.
[1] M. R. Gomez et al., Phys. Rev. Lett., 125, 155002 (2020)
[2] S. Malko, C. Johnson, W. Fox, D. Schaeffer et al. , Applied Optics 61(6) (2021).
*The work was supported by Laboratory Basic Science (LBS) Program. This work is also funded by PPPL Laboratory Directed Research and Development (DE-AC02- 09CH11466).
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