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 TP11: Poster Session VII: Basic Plasma Physics: Pure Electron Plasma, Strongly Coupled Plasmas, Self-Organization, Elementary Processes, Dusty Plasmas, Sheaths, Shocks, and Sources; Mini-conference on Nonlinear Waves and Processes in Space Plasmas - Posters; MHD and Stability, Transients (2), Runaway Electrons; NSTX-U; Spherical Tokamaks; Analytical and Computational Techniques; Diagnostics (9:30am-12:30pm)
Thursday, November 8, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.TP11.28
Abstract: TP11.00028 : Studies of plasma sheaths and plasma-wall interaction using continuum kinetic simulations*
Presenter:
Petr Cagas
(Virginia Tech)
Authors:
Petr Cagas
(Virginia Tech)
Ammar Hakim
(Princeton Plasma Phys Lab)
Bhuvana Srinivasan
(Virginia Tech)
A continuum kinetic plasma model is used to study plasma sheaths by directly evolving the ion and electron distribution functions using the Vlasov equation along with Maxwell's equations.
With the inclusion of an emitting boundary, the plasma sheath simulations become relevant for a wide range of applications, for example, space propulsion or fusion. However, such boundary conditions can significantly alter the results; theoretically up to point when the electric field potential is reversed. Therefore, these boundary conditions need to be physics-based and self-consistent.
In this work, a novel method is presented which allows for both self-consistent and efficient implementation of the emitting boundary conditions and its application to magnetized plasma sheath simulations.
*This research was supported by the Air Force Office of Scientific Research under Grant No. FA9550-15-1-0193. The work of Ammar Hakim was supported by the U.S. Department of Energy under Contract No. DE-AC02-09CH11466.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.TP11.28
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