Relationship Between Edge Zonal Flows and L-H Transitions in NSTX S. J. Zweben 1, T. Munsat 2, Y. Sechrest 2, D. Battaglia 3, S.M. Kaye 1, S. Kubota 4.

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Relationship Between Edge Zonal Flows and L-H Transitions in NSTX S. J. Zweben 1, T. Munsat 2, Y. Sechrest 2, D. Battaglia 3, S.M. Kaye 1, S. Kubota 4 and the NSTX Team 1 Princeton Plasma Physics Laboratory, 2 University of Colorado 3 ORNL, Oak Ridge 4 UCLA, Los Angeles EFTSOMP Workshop, Strasbourg July 6-7, 2011

What Causes the L-H Transition ? Theoretical ideas: Shearing of edge turbulence by mean (steady) flows Shearing of edge turbulence by zonal (fluctuating) flows Stabilization of L-mode instability without flow shearing ? Experimental evidence: Clear evidence of improved confinement due to biasing Clear evidence of turbulence reduction at L-H transition But transition ‘trigger’ is still an open issue (Wagner ‘07) We don’t have a good answer yet !

Outline of this Talk Latest fast camera movies of L-H transition on NSTX Edge zonal flow spectra derived from these movies Relationship between edge zonal flow and transition Comparison with preliminary result from Alcator C-Mod

4 Gas Puff Imaging (GPI) Diagnostic Optics view along B toward D  emission from D 2 gas puff Oriented to view 2-D radial vs. poloidal plane at gas puff 4 GPI in NSTX GPI

5 Movie of L-H Transition in NSTX Viewing area ~ 25 cm radially x 25 cm poloidally This movie 285,000 frames/sec for ~ 3.5 msec sep. radial (outward) poloidal (z) 5 50 µsec/sec (EDD) # B=4.5 kG I=0.92 MA P=2.6 MW NBI L-H sec

6 What Are We Seeing in GPI ? Seeing local emission of D  ~ n o f(n e,T e ) within window where D  is emitted in plasma edge, where T e ~ eV Can measure 2-D turbulence structure and motion even if response of D  is nonlinear (like contrast knob on a TV) Can not directly measure fluid (ion) flow or ExB flow, but measures turbulence flow velocity, as done previously* * McKee et al, PoP ’03 using BES on DIII-D Conway et al, PPCF ’05 using Doppler reflectometry on AUG 6

L-H Transition NBI-Heated Case # B=4.4 kG I=0.91 MA P=1.3 MW NBI L-H sec radial (outward) poloidal (z) (EDD) Viewing area ~ 25 cm radially x 31 cm poloidally This movie 400,000 frames/sec for ~ 2 msec 40 µsec/sec

L-H Transition RF-Heated Case # B=4.4 kG I=0.91 MA P=0.7 MW RF L-H sec radial (outward) poloidal (z) (EDD) Viewing area ~ 25 cm radially x 31 cm poloidally This movie 400,000 frames/sec for ~ 2 msec 40 µsec/sec

# B=3.6 kG I=0.80 MA Ohmic L-H sec L-H Transition in Ohmic Case radial (outward) poloidal (z) (EDD) Viewing area ~ 25 cm radially x 31 cm poloidally This movie 400,000 frames/sec for ~ 2 msec 40 µsec/sec

10 Method to Calculate Zonal Flows - for each pixel in each frame, make a short time series of the normalized GPI signal at that pixel over a ~ 40 µs interval - find highest cross-correlation to this time series in pixels of the next frame and get 2-D velocity from the displacement - average ~25 cm poloidally to get “zonal flow” velocity one frame

L H V pol spectrum just inside separatrix Zonal Flow Spectrum in NBI Case See near-coherent peak at ~ 3 kHz preceding transition

L H + dithering Zonal Flow Spectrum in RF Case See broadband, intermittent spectrum preceding transition Dithering of H to L to H etc. in D  starts at 243 msec 12 V pol spectrum just inside separatrix

13 Ohmic H-mode Zonal Flow Spectrum in Ohmic Case V pol spectrum just inside separatrix See near-coherent peak at ~ 3 kHz preceding transition

Radial Profile of ZF- NBI Case L-H transition at 253 msec V pol spectrum vs. time

Radial Profile of ZF - RF Case L-H transition at 238 msec V pol spectrum vs. time

Radial Profile of ZF– OH Case L-H transition at 235 msec V pol spectrum vs. time

HL time (sec) Fsol Vpol (km/s)  (µs) Lpol (cm) Lrad (cm) S=(dV pol /dr) (L r /L p )  Look at changes in V pol and turbulence before L-H transition No obvious ‘trigger event’, e.g. at  ~ 0.4 cm in NBI transition* Relationship of ZF and Transition ? *Zweben et al, POP ‘10 ; Sechrest et al, POP ‘11

Shear Flow Preceding Transition *Zweben et al, POP ’10 Evaluate S = (dV pol /dr)(L r /L p )  for 9 similar NBI transitions* No clear, systematic increase in S just before transition L H

Summary of NSTX Results See clear reduction in edge turbulence at L-H transition Often see coherent zonal flow preceding L-H transition But sometimes see broadband, intermittent flow instead No clear increase in zonal flow or shear before transition Causal relationship between zonal flow and L-H transition not yet clear !

Comparison with Alcator C-Mod w/ J. Terry, D. Pace, T. Golfinopolos and the Alcator Group Coherent V ~ 6.5 kHz before RF-induced L-H transition Good correlation of V pol with Bdot (probably n=0) - EGAM ? L H correlation of Vpol with Bdot

Questions for Discussion ? How can we identify cause of L-H transition experimentally ? How can we establish quantitative connection with theory ?