Investigating small-scale edge turbulence with GPI Noah Mandell, Stewart Zweben, Walter Guttenfelder, Yang Ren, Steve Sabbagh NSTX T&T Forum 2015 2/25/2015.

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Presentation transcript:

Investigating small-scale edge turbulence with GPI Noah Mandell, Stewart Zweben, Walter Guttenfelder, Yang Ren, Steve Sabbagh NSTX T&T Forum /25/2015

Motivation & GPI Optics Upgrades ●2010 GPI data included shots that showed small-scale (sub-cm) structure → consistent with ETG turbulence ●Zoom optics upgrade will allow 2-3x zoom to enhance spatial resolution of optics so that ~2-3mm structure can be resolved ●Other upgrades to fiber bundle, etc will allow better signal-to-noise ratio, possibly faster frame rate for movies Shot , t= ms (80 frames)

Experiment Goals ●Measure fluctuation (w,k) spectra of edge turbulence from GPI movies made using new magnifying zoom lens ●Examine how edge turbulence changes with ∇ T e, ∇ n e near separatrix ●Compare with theory (Guttenfelder) and other diagnostics (e.g. high-k scattering, Ren) to assess whether observed fluctuations are characteristic of ETG turbulence or other theorized modes ●Determine role of turbulence in stiff T e profiles near separatrix (as suggested by Canik et al, 2011)

Plasma Conditions ●Calibration: Require scans of B T or I P to align local B field with GPI optical view to optimize small-scale resolution, guided by EFIT (Sabbagh) ●This will require 5-10 dedicated shots (~2 hours), with GPI gas puffing. Could be an XMP. ●Main experiment: H-mode, with and without Lithium wall conditioning ●With lithium, density gradient is weakened and ETG is predicted to be more unstable in pedestal (Canik et al) ●Can piggy-back on other XPs for additional data as allowed