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.TP11.95
Abstract: TP11.00095 : High harmonic fast wave propagation in the scrape-off layer of NSTX and NSTX-U*
Presenter:
Eun-Hwa Kim
(Princeton Plasma Physics Laboratory, Princeton University)
Authors:
Eun-Hwa Kim
(Princeton Plasma Physics Laboratory, Princeton University)
Nicola Bertelli
(Princeton Plasma Physics Laboratory, Princeton University)
Joel C. Hosea
(Princeton Plasma Physics Laboratory, Princeton University)
Ernest Valeo
(Princeton Plasma Physics Laboratory, Princeton University)
Rory J. Perkins
(Princeton Plasma Physics Laboratory, Princeton University)
Syun'ichi Shiraiwa
(Plasma Science and Fusion Center, Massachusetts Institute of Technology)
John Wright
(Plasma Science and Fusion Center, Massachusetts Institute of Technology)
We perform simulations using a 2D full-wave (FW2D) code for high harmonic fast wave (HHFW) in the scrape-off layer (SOL), the region of the plasma between the last closed flux surface (LCFS) and the tokamak vacuum vessel, of NSTX and NSTX-U. The SOL is important for HHFW heating because up to 60% of the coupled power can be lost in the SOL. In this presentation, we examine the collisional power losses in the SOL (Pabs) by adopting various values of the electron density in front of antenna (Nant), the magnetic field strength (B0) as well as the distance between the LCFS and the antenna (Δ). The results clearly show that Pabs increases with increasing Nant, and/or weaker B0, showing consistency with NSTX experiments. We also found that vessel shape strongly affects the power lost to the SOL, hence Pabs increases when Δ increases. We also examine the HHFW in the NSTX/NSTX-U using recently developed Petra-M code and compare with the results from FW2D.
*This work is supported by U.S. Department of Energy, Office of Science, Office of Fusion Energy Sciences under contract number DE-AC02-09CH11466 and SciDAC grant AT1030200.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.TP11.95
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