50th Annual Meeting of the Division of Plasma Physics 
Volume 53, Number 14
Monday–Friday, November 17–21, 2008;
Dallas, Texas
Session BI2: Rotation in Tokamaks
9:45 AM–12:45 PM, 
Monday, November 17, 2008
Room: Landmark B
Chair: John de Grassie, General Atomics
Abstract ID: BAPS.2008.DPP.BI2.6
Abstract: BI2.00006 : Observation of ICRF Mode Conversion Plasma Flow Drive on Alcator C-Mod*
12:15 PM–12:45 PM
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 Abstract
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Author:
Yijun Lin
(MIT Plasma Science and Fusion Center)
Plasma flow driven by externally launched rf waves could be important in 
stabilizing micro- and macro-instabilities in tokamaks. We report the first 
observation of both toroidal (V$_{\phi })$ and poloidal (V$_{\theta })$ 
flows driven via an ICRF mode conversion (MC) process in D($^{3}$He) 
plasmas. At modest $^{3}$He levels (n$_{3He}$/n$_{e}\sim $ 8{\%}), in 
relatively low density plasmas, $<$n$_{e}>\le $ 1.3$\times 
$10$^{20}$m$^{-3}$, heated with 50 MHz rf power (B$_{t0}\sim $ 5.1 T), 
strong V$_{\phi }$ in the co-current direction is observed by 
high-resolution x-ray spectroscopy. The central V$_{\phi }$ scales with the 
applied rf power ($\le $ 30 km/s per MW), and is at least a factor of 2 more 
than the empirically determined intrinsic plasma rotation [1]. The rotation 
near the plasma center (r/a $<$ 0.3) responds more quickly to the applied rf 
power than the outer region, indicative of a local flow drive source. 
Localized poloidal rotation (0.3 $\le $ r/a $\le $ 0.5) in the ion 
diamagnetic drift direction is observed when P$_{rf }\ge $ 1.5 MW and 
increases with power ($\sim $ 2 km/s at 3 MW). Turbulence spectrum 
broadening seen by a phase contrast imaging (PCI) system indicates strong 
flow also exists in the main ions. The mode converted ion cyclotron wave (MC 
ICW) is observed by PCI and confirmed by 2-D full wave TORIC code 
simulation. The simulation result shows that due to the up-shifted k$_{\vert 
\vert }$,$_{ }$the MC ICW is strongly damped on $^{3}$He ions in the 
vicinity of the MC layer, approximately on the same flux surfaces where 
poloidal flow is observed. The involvement of ion heating and 
short-wavelength slow wave is consistent with theoretical considerations for 
efficient rf flow drive. Our experimental results are comparable to the 
predictions [2], assuming similar ion interaction mechanism for the MC ICW 
and direct launch ion Bernstein wave. The feasibility of ICRF flow drive on 
ITER will be discussed.
[1] J. E. Rice, et al, Nucl. Fusion \textbf{47}, 1618 (2007). 
[2] J. R. Myra and D. A. D'Ippolito, Phys. Plasmas \textbf{9}, 3867 (2002).
*Work supported by US DoE Coop. Agreement No. DE-FC02-99ER54512.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2008.DPP.BI2.6