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M. Greenwald, et al., APS-DPP 2006 Density Peaking At Low Collisionality on Alcator C-Mod APS-DPP Meeting Philadelphia, 10/31/2006 M. Greenwald, D. Ernst,

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Presentation on theme: "M. Greenwald, et al., APS-DPP 2006 Density Peaking At Low Collisionality on Alcator C-Mod APS-DPP Meeting Philadelphia, 10/31/2006 M. Greenwald, D. Ernst,"— Presentation transcript:

1 M. Greenwald, et al., APS-DPP 2006 Density Peaking At Low Collisionality on Alcator C-Mod APS-DPP Meeting Philadelphia, 10/31/2006 M. Greenwald, D. Ernst, A. Hubbard, J.W. Hughes, Y. Lin, J. Terry, S. Wukitch, K. Zhurovich, Alcator Group

2 M. Greenwald, et al., APS-DPP 2006 ● ITER interest – better fusion performance with moderate density peaking ● Results from ASDEX, JET suggest increase in density peaking at low * (note plots use eff = ei / De not *) ● Much of the previous work has significant beam fueling (C-Mod uses RF only) ● Until recently, C-Mod density was too high to enter the very low * regime. Collisionality Effects on Density Profile ASDEX-U: C. Angioni et al., PRL (2003) JET: H. Weisen, et al., NF (2005) ASDEX-U H-Modes Typical C-Mod H-modes

3 M. Greenwald, et al., APS-DPP 2006 With this shape, large ELMs appear in C-Mod for first time (Terry APS GI1.00004) n/n G = 0.3, eff = 0.33, ei  E ~ 10 Low Density H-Modes Accessible With “Unusual” Shape

4 M. Greenwald, et al., APS-DPP 2006 EDA (QC mode) and small ELMs n/n G = 0.66, eff = 1.5, ei  E ~ 40 (2x, 5x, 4x lower density H-mode respectively) H-Mode In Standard C-Mod Shape

5 M. Greenwald, et al., APS-DPP 2006 ● We don’t know why these shapes allow operational H-mode at lower target densities –Lower L-H threshold density –ELMs seem to reduce rate of density rise in H-mode ● Whatever the cause: –Standard H-mode n e0 / = 1.1-1.2 L n >> a, R/L n ~ 0, R/L T ~ 6-7 –Low-Density H-mode n e0 / = 1.5 R/L n ~ 3-4, R/L T ~ 6-7 Lower Density H-Modes Show More Profile Peaking

6 M. Greenwald, et al., APS-DPP 2006 ● Peaking is seen over outer 60% of plasma radius ● H-mode profiles evolve quickly;  << a/V WARE ● Transport in center of plasma may be affected by sawteeth –These are of large amplitude;  T e /T e ~ 25% ● Radii chosen to characterize peaking in ASDEX-U are appropriate for C-Mod profiles ● So, collect a database and plot results…. Difference In Profile Shape Is Notable Sawtooth Inversion Radius r/a = 0.4r/a = 0.8

7 M. Greenwald, et al., APS-DPP 2006 Trend Of Increased Density Peaking At Low Collisionality Is Observed For ICRF Heated H-Modes In C-Mod “Standard” Shape “New Shape” LHCD (L-Mode with V S ~ 0; V Ware very small)

8 M. Greenwald, et al., APS-DPP 2006 C-Mod Data Overlays ASDEX-U C-Mod Angioni PRL 2003

9 M. Greenwald, et al., APS-DPP 2006 Same With Respect To JET Data…. C-Mod Weisen NF 2005 ITER

10 M. Greenwald, et al., APS-DPP 2006 n/n G Is Apparently Not A Good Scaling Parameter For Comparing C-Mod and JET Peaking n/n G C-Mod Note horizontal separation of data sets JET data from Weisen PPCF 2006 ITER

11 M. Greenwald, et al., APS-DPP 2006 ● ITG/TEM turbulence can predict inward particle flux in the collisionless limit (Quasi-linear calculations: Angioni, Phys. Plasmas 12, 112310, 2005) –Thermodiffusion mechanism (Coppi, PRL 41, 551,1978) –Driven by  T i, for R/L T > R/L n –“Pinch” disappears at higher collisionality –Depends on relative strength of ITG and TEM (L T, ,, T e /T i ) ● However: collisionality range with density peaking is predicted to be about 30 x smaller than what is seen in experiments ● Nonlinear GK simulations see pinch at experimentally realistic eff, but only by lowering L n /L T (Estrada-Milna, Phys. Plasmas 12 022305, 2005) State Of Theory Is Not Yet Adequate To Explain These Results

12 M. Greenwald, et al., APS-DPP 2006 ● Significant density profile peaking seen at low collisionality ● Trend and values match data from ASDEX-U and JET –Lack of NBI fueling does not affect result –Lack of Ware pinch does not affect result –Result holds for Ti ~ Te –Work extended to higher neutral opacity (ITER-like) –Addition of C-Mod data suggest that eff is appropriate scaling variable rather than n/n G (These are strongly correlated, especially on any given machine) – Good news for ITER ● Effect of shaping? ● Installation of cryopump and increased LH power will allow substantial extension of this work. Summary


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