55th Annual Meeting of the APS Division of Plasma Physics
Volume 58, Number 16
Monday–Friday, November 11–15, 2013;
Denver, Colorado
Session NI2: Energetic Particles, 3D Physics
9:30 AM–12:30 PM,
Wednesday, November 13, 2013
Room: Plaza E
Chair: Nikolai Gorelenkov, Princeton Plasma Physics Laboratory
Abstract ID: BAPS.2013.DPP.NI2.4
Abstract: NI2.00004 : Unified parametric dependence, control, and reconstruction of 3D equilibria in the RFP*
11:00 AM–11:30 AM
Preview Abstract
Abstract
Author:
Brett Chapman
(University of Wisconsin-Madison)
A helical, stellarator-like equilibrium emerges in the core of RFP plasmas
when the normally broad tearing mode spectrum spontaneously condenses -- the
innermost resonant mode grows to large amplitude, while the other, secondary
mode amplitudes are reduced. This quasi-single-helicity (QSH) transition is
not fully understood, but it likely hinges on the nonlinear MHD that governs
the tearing mode spectrum. Here we report (1) progress in understanding the
transition in terms of the Lundquist number, S, a key dimensionless
parameter in nonlinear MHD, (2) improved energy confinement in MST with QSH
and inductive current profile control, and (3) progress in developing 3D
equilibrium reconstructions for QSH plasmas. In MST, the likelihood and
duration of QSH spectra increase strongly with the plasma current, Ip,
similar to the trend in RFX-mod, but the Ip at which QSH emerges in MST is
3x smaller. However, given that MST can, for a given Ip, access lower
density and higher Te, the two devices share a common range of S, which
varies as Ip*Te$^{\mathrm{1.5}}$n$^{\mathrm{-0.5}}$, and the tearing spectra
from the two devices exhibit a common dependence on S. The above results
accrued in plasmas with largely Maxwellian electrons and ions. With the
addition of neutral-beam-injected fast (25 keV) ions in MST, the likelihood
of QSH in low-S plasmas decreases further. In high-S plasmas, the likelihood
of QSH is largely unaffected by the fast ions. The dominant mode in MST can
reach 8{\%} of the equilibrium field. This, combined with the reduced
secondary modes, leads to a locally enhanced Te in the core and a 50{\%}
improvement in energy confinement. The secondary modes are further reduced
by slowly ramping down Ip, a form of current profile control. This leads to
a larger Te \textgreater 1 keV and a tripling of the energy confinement.
These results were achieved with zero applied Bt (infinite toroidal beta).
The 3D magnetic topology was measured directly for the first time in MST via
Faraday rotation. This and other advanced diagnostics are being included in
the V3FIT equilibrium reconstruction code through a multi-institution
collaboration. The varying orientation of the 3D structure relative to the
diagnostics will help in V3FIT optimization.
*Work supported by US DOE.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2013.DPP.NI2.4