2005 47th Annual Meeting of the Division of Plasma Physics
Monday–Friday, October 24–28, 2005;
Denver, Colorado
Session CI1b: Transport Barrier Physics
3:00 PM–5:00 PM,
Monday, October 24, 2005
Adam's Mark Hotel
Room: Plaza Ballroom ABC
Chair: Charles Bush, Oak Ridge National Laboratory
Abstract ID: BAPS.2005.DPP.CI1b.3
Abstract: CI1b.00003 : Physics and Operational Space of the Small ELM regime in NSTX*
4:00 PM–4:30 PM
Preview Abstract
Abstract
Author:
Rajesh Maingi
(Oak Ridge National Lab)
The search for high performance regimes with small or no periodic
heat
pulses, due e.g. to edge-localized modes (ELMs), has been a focus of
international research, owing to possible erosion damage to
plasma facing
components during large, Type I ELMs as projected...\footnote{A.
Loarte, et. al., 2003 \textit{J. Nucl. Materials}
\textbf{313-316} 962.} for ITER. A
high-performance, small ELM regime is now routinely observed in
the National
Spherical Torus Experiment (NSTX). The ELMS (called \footnote{R.
Maingi, et. al., 2005 \textit{Nuclear Fusion} \textbf{45} 264.}
``type V'') are
consistent with high bootstrap current operation with line
average density
approaching Greenwald scaling. Each individual ELM has no
measurable impact
on stored energy. The ELM perturbation is observed via ultra-soft
X-rays to
typically originate near the lower divertor region and propagate
with a
poloidal component toward the outer midplane. A pre-cursor with
n=1 is
observed on an outboard near-midplane toroidal Mirnov array. The
filament-like structure propagates in the counter plasma current
direction
and persists for \underline {$<$} 1-2 toroidal transit times.
After crossing
the separatrix to the open field lines, the ELM flux is observed
to reach
the outer strike point up to 400 $\mu $sec before the inboard side,
consistent with leakage of ions from the pedestal top $\sim $ 200
eV across
the separatrix on the low field side near the lower X-point, and
sound speed
propagation on the open field lines. In contrast, a large Type I
ELM is
observed to reach the outer strike point only up to 200 $\mu $sec
before the
inboard side, consistent with a ballooning-type perturbation near
the
outboard midplane. To date, the Type V ELM regime without
intervening Type I
ELMs has been obtained with $\beta _{N}$ \underline {$<$ }5, $\nu
_{e,ped}^{\ast } \quad >$ 1, $\beta _{pol}$ \underline {$>$} 0.5 and
$\beta _{ped}$ \underline {$<$ }5{\%}. The differences between
these Type
V ELMs and conventional Types I and III ELMs, which also observed
in NSTX,
will be presented.
*Sponsored by U.S. Dept. of Energy contracts DE-AC05-00OR22725 and DE-AC02-76CH03073.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2005.DPP.CI1b.3