First High-Power Helicon Results From DIII-D

Abstract More than 0.6 MW of rf power at 476 MHz has been coupled to DIII-D plasmas by launching helicon (whistler) waves with a traveling-wave antenna (comb-line) in the fast-wave polarization which resulted in the observation of electron heating of the core plasma with single-pass absorption based...

Full description

Saved in:
Bibliographic Details
Published inNuclear fusion
Main Authors Pinsker, Robert I., Van Compernolle, Bart, Tang, Shawn X., Lestz, Jeff, Moeller, Charles P., Petty, Craig, Dupuy, Alexandre, Squire, Jared P., Garofalo, Andrea M., Porkolab, Miklos, Rost, J. C., Baek, Seung-Gyou, Nagy, Alexander, Chowdhury, Satyajit, Crocker, Neal A., DeGrandchamp, Genevieve, McLean, Adam G., Gage, Kenneth Ryan, Marinoni, Alessandro, Martin, Elijah Henry, Ronchi, Gilson
Format Journal Article
LanguageEnglish
Published United States IOP Science 10.09.2024
Online AccessGet full text

Cover

Loading…
More Information
Summary:Abstract More than 0.6 MW of rf power at 476 MHz has been coupled to DIII-D plasmas by launching helicon (whistler) waves with a traveling-wave antenna (comb-line) in the fast-wave polarization which resulted in the observation of electron heating of the core plasma with single-pass absorption based on ray-tracing in L-mode discharges. The coupling performance of the wide 30-element comb-line traveling-wave antenna has been consistent with expectations based on the 2015-2016 experiments on DIII-D with a low-power 12-element prototype. The conditioning process that was necessary to carry out high-power experiments is discussed; rf-specific impurities have not been observed. Parametric decay instabilities (PDI) have been observed and are being investigated as a potential edge absorption mechanism.
Bibliography:USDOE Office of Science (SC), Basic Energy Sciences (BES). Scientific User Facilities (SUF)
USDOE Office of Science (SC), Fusion Energy Sciences (FES)
FC02-04ER54698; SC0016154; SC0020649; AC52-07NA27344; SC0020337; FG02-07ER54917; AC05-00OR22725; AC02-09CH11466
ISSN:0029-5515