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 PO7: Magnetized HED Plasmas and Laborary Astrophysics
2:00 PM–5:00 PM,
Wednesday, November 7, 2018
OCC
Room: B117-119
Chair: Will Fox, Princeton Plasma Physics Lab
Abstract ID: BAPS.2018.DPP.PO7.5
Abstract: PO7.00005 : Self-Generated Magnetic Fields in High Energy Density Laboratory Experiments*
2:48 PM–3:00 PM
Presenter:
Kirk A. Flippo
(Los Alamos National Laboratory)
Authors:
Kirk A. Flippo
(Los Alamos National Laboratory)
Hui Li
(Los Alamos National Laboratory)
Shengtai Li
(Los Alamos National Laboratory)
Carlos Di Stefano
(Los Alamos National Laboratory)
Alexander Rasmus
(Los Alamos National Laboratory)
Daniel H Barnak
(Los Alamos National Laboratory)
Codie Y Fiedler Kawaguchi
(Los Alamos National Laboratory)
Kwyntero V Kelso
(Los Alamos National Laboratory)
Andy Liao
(Los Alamos National Laboratory)
Yingchao Lu
(Rice University, Los Alamos National Laboratory)
Jordon T. Laune
(University of Chicago)
High Energy Density (HED) laboratory experiments to study hydrodynamic instabilities have been developed over the last several years on Omega and NIF. We model these experiments with multi-physics hydro-dynamic codes under the assumption that any magnetic fields produced in these plasmas will not affect the bulk hydro. In many cases this is likely a valid assumption; however, as we try to ever focus our understanding on smaller and smaller scale phenomena in HED experiments we begin to see more and more discrepancies with our pure hydro models. Our project aims to create and diagnose self-generated fields in platforms similar to our HED hydro experiments to quantify how large these fields can become and how these fields can affect the small scale hydro evolution of these platforms. Namely, when the energy density of phenomena are on par with the magnetic energy density, as can be in turbulence, how are small vortices affected, how do B fields change the dissipation scales, and how do changes in heat conduction change the distribution of modes?
*This work was supported by the LDRD Office at Los Alamos National Laboratory operated by Los Alamos National Security, LLC for the U.S. DOE NNSA.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.PO7.5
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