Phase contrast imaging measurements and numerical simulations of turbulent density fluctuations in gas-fuelled ECRH discharges in Wendelstein 7-X. (28th June 2021)

• Record Type: Journal Article
• Authors: Bähner, J.-P.; Alcusón, J.A.; Hansen, S.K.; von Stechow, A.; Grulke, O.; Windisch, T.; Smith, H.M.; Huang, Z.; Edlund, E.M.; Porkolab, M.; Beurskens, M.N.A.; Bozhenkov, S.A.; Ford, O.P.; Vanó, L.; Langenberg, A.; Pablant, N.; Plunk, G.G.; Bañón Navarro, A.; Jenko, F.
• Other Names: collab.
• Is Part Of: Journal of plasma physics. Volume 87:Number 3(2021)
• Publication Date: 2021-06-28
• Subjects: fusion plasma; Plasma (Ionized gases) -- Periodicals; 530.4405
• DOI: 10.1017/S0022377821000635
• Languages: English
• ISSNs: 0022-3778

Abstract

Abstract : The fundamental nature of turbulent density fluctuations in standard Wendelstein 7-X (W7-X) stellarator discharges is investigated experimentally via phase contrast imaging (PCI) in combination with gyrokinetic simulations with the code GENE. We find that density fluctuations are ion-temperature-gradient-driven and radially localised in the outer half of the plasma. It is shown that the line-integrated PCI measurements cover the right range of wavenumbers and a favourable toroidal and poloidal location to capture some of the strongest density fluctuations in W7-X. Due to the radial localisation of fluctuations, measured wavenumber–frequency spectra exhibit a dominant phase velocity, which can be related to the $\boldsymbol {E\times B}$ rotation velocity at the radial position of a well in the neoclassical radial electric field. The match is robust against variations of heating power and line-integrated density, which is partly due to the localisation of fluctuations and partly due to effects of the radial gradient in the $\boldsymbol {E\times B}$ velocity profile on the wavenumber–frequency spectrum. The latter effect is studied with a newly built synthetic PCI diagnostic and global gyrokinetic simulations with GENE-3D.