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 JP11: Poster Session IV: Education and Outreach; Undergraduate or High School Research; Plasma technology, Fusion reactor Nuclear and Materials Science; Propulsion; Materials Interfaces (2:00pm-5:00pm)
Tuesday, November 6, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.JP11.59
Abstract: JP11.00059 : Data analysis of wave propagation and boundary interactions in the ion cyclotron range of frequencies at LaPD *
Presenter:
Parker John Roberts
(Princeton Plasma Physics Laboratory)
Authors:
Parker John Roberts
(Princeton Plasma Physics Laboratory)
Rory James Perkins
(Princeton Plasma Physics Laboratory)
Troy Carter
(Univ of California - Los Angeles)
Bart G.P. Van Compernolle
(Univ of California - Los Angeles)
Walter N Gekelman
(Univ of California - Los Angeles)
Patrick Pribyl
(Univ of California - Los Angeles)
John B Caughman
(Oak Ridge National Lab)
Cornwall H. Lau
(Oak Ridge National Lab)
Elijah Henry Martin
(Oak Ridge National Lab)
Shreekrishna Tripathi
(Univ of California - Los Angeles)
Steve Vincena
(Univ of California - Los Angeles)
Plasma heating using waves in the ion cyclotron range of frequencies is common in fusion experiments but frequently causes an unacceptable rise in metallic impurities. This is attributed to RF rectification, a nonlinear sheath phenomenon that can increase both electron current and plasma voltage across the sheath. Experiments to study this phenomenon have been performed at the Large Plasma Device located at UCLA using a single-strap antenna with about 100 kW of power and include measurements from floating and emissive probes. We develop Python code to visualize the spatially-dense two-dimensional data sets to resolve differences in the rectified response between the field lines connecting to the antenna at low plasma densities (below 1e18 m-3) and field lines with longer connection lengths (of order 10 m) in a denser plasma (around 5e18 m-3). This will help determine the penetration depth of the rectified effects into the central plasma and how their nature changes at different densities and magnetic-connection lengths.
*This work was supported by the DOE SULI program and was performed at the Basic Plasma Science Facility supported by DOE and NSF, with major facility instrumentation developed via NSF award AGS-9724366.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.JP11.59
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