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 BP11: Poster Session I: HEDP; General Stellarator; Wendelstein 7-X; Heating, Current Drive, and Energetic Ions (9:30am-12:30pm)
Monday, November 5, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.BP11.91
Abstract: BP11.00091 : Interaction between high-power ICRF waves and drift-wave turbulence in LAPD*
Presenter:
Troy Carter
(Univ of California - Los Angeles)
Authors:
Troy Carter
(Univ of California - Los Angeles)
Bart G.P. Van Compernolle
(Univ of California - Los Angeles)
Rory James Perkins
(Princeton Plasma Phys Lab)
Patrick Pribyl
(University of California, Los Angeles)
An experimental campaign on the physics of ICRF waves has recently begun using the Large
Plasma Device (LAPD) at UCLA. A new high-power (∼150 kW) RF system and antenna have been developed for excitation of large amplitude fast waves in LAPD. The source runs at a
frequency of 1-5 MHz, corresponding to ∼ 1-10 fci, depending on plasma parameters. Recent work has focused on the structure and scaling of RF sheaths and convection cells near the antenna [1]. In these same experiments, strong low-frequency modulation of coupled fast wave power is observed via direct measurement of the magnetic signals associated with the fast waves in the core plasma. This modulation is well correlated with low-frequency edge
density fluctuations associated with drift waves. Suprisingly, the amplitude of the RF modulation and the amplitude of edge density fluctuations in the drift wave frenquency range both grow with increasing RF power, suggesting some nonlinear coupling between the edge drift waves and large amplitude fast waves in the core region.
[1] Martin, et al., PRL 119, 205002 (2017)
*This work was performed at the Basic Plasma Science Facility supported by DOE and NSF, with major facility instrumentation developed via an NSF award AGS-9724366.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.BP11.91
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