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.TP11.101
Abstract: TP11.00101 : Simultaneous High-k Scattering and Microwave Imaging Reflectometry on NSTX-U*
Presenter:
N.C. Luhmann, Jr.
(UC Davis)
Authors:
N.C. Luhmann, Jr.
(UC Davis)
Robert Barchfeld
(UC Davis)
Yang Ren
(PPPL)
Robert Ellis
(PPPL)
Nicole Allen
(PPPL)
Robert Kaita
(PPPL)
Brent Stratton
(PPPL)
Jon Dannenberg
(UC Davis)
Yilun Zhu
(UC Davis)
Calvin Domier
(UC Davis)
An 8-channel 693 GHz poloidal high-k scattering system is under development, replacing a 5-channel 280 GHz toroidal scattering system, to study high-k density fluctuations on NSTX-U. The far-infrared probe beam is launched from Bay G towards Bay L, where large aperture optics collect radiation at 8 simultaneous scattering angles ranging from 2 to 15°. This yields measurement of poloidal wavenumbers from 7 cm-1 to >40 cm-1, while translatable optics allow placement of the scattering volume from r/a = 0.1 out to the pedestal region (r/a ~ 0.99). A microwave imaging reflectometry (MIR) system will co-exist with the High-k Scattering system on Bay L, with MIR optics positioned above that of the scattering system, to monitor low-kθ (< 3 cm-1) density fluctuations. Details of the 5×4 channel (5 poloidal, 4 radial) MIR system, spanning frequencies of 51 to 75 GHz, will be presented together with that of the High-k Scattering system.
*Work supported in part by U.S. DOE Grant DE-FG02-99ER54518 and DE-AC02-09CH1146.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.TP11.101
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