

Operations on the \sc Pegasus Toroidal Experiment are
focusing on the exploration of MHD stability limits at high
normalized current, high \beta_t, and near-unity aspect
ratio. Past plasma behavior was dominated by large resistive
MHD modes and power supply limits. Recent upgrades will
allow access to the I_p/I_tf > 1 regime by suppressing
the resistive MHD. Tools to vary the q-profile and suppress
the MHD activity include significantly increased poloidal
field control, increased, time-variable toroidal field, and
loop voltage programmability. Modeling with the DCON code
has demonstrated that stable equilibria exist with
I_p/I_tf approaching 3. A complete set of magnetics
diagnostics, combined with simple plasma parameter
measurements and eventually an imaging SXR camera system for
poloidal flux surface mapping, provides data for reasonably
accurate equilibrium reconstructions. The present
experimental campaign is focused on the suppression of the
internal tearing modes to allow access to the external kink
limits at high I_N.
[CO3.002] Extending high-beta operation in NSTX through plasma shaping and early H-mode transitions
D. A. Gates, J.E. Menard (PPPL), R. Maingi, M. Wade (ORNL), NSTX National Research Team
The National Spherical Torus Experiment (NSTX) resumed
operation in February 2004 and completed in July a program
of experiments which expanded its operating space and
contributed to resolving issues both for the design of
future ST devices and in toroidal magnetic confinement
physics. Improvements in plasma control have led to the
achievement of higher plasma elongation, \kappa = 2.6 and
normalized current, I_N = I_p/aB_T = 6.9 MA/m \cdot T.
By optimizing the current ramp-up, gas puffing and neutral
beam power waveforms, reliable early transitions to the
H-mode have been obtained, which improved confinement and
broadened the pressure profiles, permitting the achievement
of very high beta, \beta_T = 34%, determined by EFIT
from external magnetic and kinetic profile data and
corroborated by analysis with TRANSP. These improvements
have led to the achievement of 1MA pulses with 1s duration
that were not limited by the available transformer flux.
First measurements have also been obtained with the MSE
diagnostic. The features of the NSTX operating space and
characteristics of the high-\beta plasmas will be
discussed. This work supported by DOE Contract Number
DE-AC02-76CH03073
[CO3.003] Confinement in high-\beta, NB-heated H- and L-mode plasmas in NSTX
M.G. Bell, S.M. Kaye (PPPL), NSTX Research Team
The National Spherical Torus Experiment (NSTX) has completed
a program of experiments which spanned significant ranges
for the dominant engineering variables in the scaling of
energy confinement in conventional tokamaks. The experiments
included well controlled scans in H-mode plasmas of the
plasma current and neutral beam heating power. The energy
confinement time has been determined by equilibrium analysis
based on external magnetic measurements and confirmed for a
subset of discharges by analysis of the kinetic measurements
with the TRANSP code. The variation in the global energy
confinement time with current and heating power matches
quite closely the dependences in the ITER-98pb(y,2) H-mode
scaling both in the single-parameter scans and regression to
the overall database. Nevertheless, for neutral beam heated
H-mode plasmas, the global confinement exceeds the H-mode
scaling predictions by a factor up to 1.6. In L-mode plasmas
the confinement often exceeds the H-mode scaling predictions
as well. These trends and the results of the TRANSP analysis
will be presented.
[CO3.004] Electron Transport in NSTX
W. Horton, H. V. Wong, J.-H. Kim, J. Pratt (IFS University of Texas at Austin), B. LeBlanc (PPPL)
The high harmonic fast wave heated plasmas in NSTX are ideal plasmas for studying electron confinement regimes. Energy confinement times twice that of the ITER-L97 confinement law are produced at high electron plasma pressure-to-magnetic pressure ratios. Peaked density and temperature L-mode type profiles showing good particle confinement with low eta-e values as well as electron ITB discharges in low or weakly reversed magnetic shear profiles are analyzed for transport using standard drift wave transport models. The ETG mode gives the best interpretation of the heat flux versus gradient relationship. Although the trapped electron fraction is high, the trapped electron modes are suppressed by the high plasma pressure and high MHD alpha-factor that produces favorable bounce averaged guiding center drifts among other stabilizing effects. We show nonlinear simulations with specified heating power and edge losses that explain the inverse cascade in the ETG spectrum and produce thermal diffusivity profiles similar to the TRANSP power balance profiles.
Work supported by the Department of Energy Basic Energy
Sciences.
[CO3.005] High Performance Regime with Small ELMs in NSTX
Rajesh Maingi (Oak Ridge National Lab), NSTX Team
A high performance regime with small edge-localized modes
(ELMs) has been observed in the National Spherical Torus
Experiment (NSTX). The ELMS (“type V”) are consistent with
high bootstrap current operation with line average density
approaching Greenwald scaling, and provide enhanced edge
particle transport compared with ELM-free discharges. Each
individual ELM has no measurable impact on stored energy,
The ELM perturbation is observed via ultra-soft X-rays
(USXR) to typically originate near the lower divertor region
and propagate with a poloidal component toward the outer
midplane and often to the top of the machine. An
electromagnetic signature is observed before the USXR
perturbation on separate poloidal and toroidal Mirnov
arrays, indicating a toroidal mode number of n=1,
propagation counter to the plasma current, and persistence
for up to two toroidal transit times. These type V ELMs are
distinct from both type I and type III ELMs, which have also
been observed in NSTX, and can co-exist with type I ELMs.
When the type V ELMS are present, there is no evidence of an
edge harmonic oscillation as observed in DIII-D quiescent
H-mode discharges, or of an edge quasi-coherent mode
observed in the PDX forced density rise scenario and the
C-MOD Enhanced D-alpha H-mode scenario.
[CO3.006] Solenoid free plasma start-up in NSTX by Coaxial Helicity Injection
R. Raman, T.R. Jarboe, B.A. Nelson (Univ. of Wash.), M. Bell, D. Mueller (PPPL), M. Schaffer (GA), NSTX Research Team
A new method recently developed on HIT-II, referred to as
transient CHI, has unambiguously demonstrated the presence
of a robust closed flux equilibrium and central transformer
volt-seconds savings when coupled to induction, showing that
the CHI produced plasmas are not only compatible with
conventionally produced inductive plasmas but that they also
improve the performance of these inductive plasmas [R.Raman
et al., Phys. Rev. Lett. 90, 075005 (2003)]. In this method
the plasma is rapidly grown through the use of an
appropriately sized capacitor bank. The initial static
magnetic flux is chosen such that this rapidly expanding
plasma has a tendency to detach from the lower divertor
electrodes. Rapidly reducing the injector current during
this phase eases the detachment process, which results in
the production of a robust closed field line equilibrium.
Results from these experiments on NSTX will be reported. DOE
Contract No. DE-AC02-76CH03073 and DE-FG03-99ER54519
supports this work.
[CO3.007] Plasma formation without a central solenoid in a Spherical Tokamak
A. Sykes, G. Cunningham, M. Gryaznevich, M. Hood, G. McArdle (EURATOM/UKAEA Fusion Association, Culham Science Centre, Abingdon, Oxfordshire OX14 3DB, UK), F. Alladio, P. Costa, A. Mancuso, P. Micozzi (ENEA Frascati, Italy), A. Dnestrovskij (Kurchatov Institute, Moscow, Russia)
Obtaining the plasma current in any ST is a challenge as
there is limited space for the central solenoid; indeed this
is absent in most proposed ST fusion devices due to the high
neutron flux, there being no space for an effective shield.
A range of start-up techniques will be described, with
special emphasis on the Merging-Compression (M-C) method of
plasma formation used on START and MAST, and a `Double Null
Merging' scheme whereby two initial plasmas formed in
low-order nulls between Poloidal Field coils are merged.
Results from M-C confirm that high temperature plasmas are
obtained from merging. Results and/or modelling indicate
that both techniques can produce hot initial plasmas of
0.5MA in MAST without use of the central solenoid, in
readiness for subsequent ramp-up using high power NBI and
the associated input of flux (significant in an ST) from the
increasing vertical field
[CO3.008] Toroidal Rotation Damping Physics in NSTX
W. Zhu, S.A. Sabbagh, A.G. Sontag, J. Bialek (Columbia University), R.E. Bell, J.E. Menard, D.A. Gates, B.P. LeBlanc (PPPL, and the NSTX Research Team)
Spherical torus and tokamak experiments show that the
combination of sufficient plasma rotation and a resistive
wall can stabilize ideal kink/ballooning modes. However,
toroidal rotation damping has been observed at sufficiently
high plasma beta, eliminating passive stabilization. Rapid
and global damping at high beta above the ideal MHD no-wall
limit experimentally expedites mode locking and plasma beta
collapse. ELMs lead to edge rotation damping that is
typically insignificant. Resonant electromagnetic drag may
explain rotation damping for resistive modes with small
island width, while non-resonant neo-classical toroidal
viscous drag is in quantitative agreement with measured
global damping in resistive wall mode, 1/1 mode, and local
damping in ELMing plasmas. A pair of non-axisymmetric coils
was used to generate an n=1 magnetic field perturbation
which allowed greater rotation control. Quantitative
comparison is made between theory and experiment to
determine the physics and parameter dependence of the
damping evolution for the observed instabilities.
[CO3.009] Neoclassical tearing mode onset in NSTX
E.D. Fredrickson, J. Menard (Princeton Plasma Physics Laboratory), K. Tritz, D. Stutman (Johns Hopkins University)
Neoclassical theory predicts well the time evolution of
experimentally observed saturated tearing modes. The
theory also predicts that many more modes are non-linearly
unstable than are seen. The theory does less well in
predicting which modes are either linearly unstable or
triggered by other events in the plasma. Experiments have
been performed in NSTX to identify the parametric
dependences of NTM onset. In the first experiment,
repetitive sawteeth were generated in plasmas with different
beta and plasma current and the growth (damping) rate for
the NTMs was determined. In the second. Similar, experiment,
repetitive fast ion driven chirping modes (fishbones) were
used as the NTM trigger. For all shots, the NTM parameters
were evaluated using TRANSP, including the calculation of
the neoclassical (bootstrap) current fraction. Diagnostics
for mode detection included soft x-ray cameras and Mirnov
coils.
[CO3.010] Edge/SOL characterization in the NSTX spherical tokamak
Jose Boedo, Dmitry Rudakov (UCSD), Henry Kugel (PPPL), Neal Crocker (UCLA), Alexander Pigarov (UCSD), Stewart Zweben (PPPL), Ricardo Maqueda (Nova Photonics), NSTX Team
The edge/SOL of NSTX has been investigated with a high
temporal (1 ?s) and spatial (1.5 mm) resolution probe array
in L-mode and H-mode discharges. The decay lengths of the
density and temperature profiles in the SOL in L-mode are 4
cm and 12 cm respectively, independently of power. In H-mode
the profile decay lengths are reduced considerably to 1-2
cm. The profile decay lengths shorten significantly to ~2 cm
in H-mode. Features of interest are: 1) The Te SOL profile
is flat at \sim20 eV and highly fluctuating and, 2) the Te
pedestal is shifted inwards from the Ne pedestal by \sim3 cm,
indicating decoupled energy and particle transport. Strong
intermittency in the edge/SOL has been observed and
quantified using conditional averaging. UEDGE modeling is in
progress.
[CO3.011] Edge Turbulence Imaging During L-H Transitions in NSTX
S.J. Zweben, T. Munsat (PPPL), R.J. Maqueda (Nova Photonics), T.M. Biewer (PPPL), C.E. Bush, R. Maingi, D.P. Stotler (ORNL), N.A. Crocker, S. Kubota, X.V. Nguyen, W.A. Peebles (UCLA), NSTX
High speed movies of the radial vs. poloidal structure of
edge turbulence during L-H and H-L transitions in NSTX will
be shown and discussed. These images were made in D-alpha
light at up to 250,000 frames/sec with a 300 frame, 64x64
pixel ultra-high speed PSI-5 camera . Transitions from
L-mode to H-mode appear as a continuous evolution from a
turbulent state to a quiescent state over about 0.1 ms,
apparently without any new spatial features or flows.
Transitions from H-L generally appear as high-n poloidal
perturbations which evolve into radially moving blobs.
Analysis of this data is being done to extract local
velocity fields to estimate shear and zonal flows.
Comparison of these images with data from the UCLA
reflectometers will be discussed. Movies of ELMs and other
MHD effects will also be shown if time allows.
[CO3.012] High Harmonic Fast Wave Heating on NSTX- I
J. R. Wilson, S. Bernabei, T. Biewer, S. Diem, J. Hosea, B. LeBlanc, C. K. Phillips (PPPL), P. Ryan, D. W. Swain (ORNL)
Previous experiments on NSTX have demonstrated that HHFW
heats electrons and drives current as expected from theory.
Some anomalies have been observed, including edge ion
heating and apparent reduced heating and current drive under
some conditions. A series of detailed experiments to
quantify these observations has been undertaken. The edge
heating is believed to be due to parametric decay of the
applied fast wave into ion Bernstein waves. Peaks in the
frequency spectrum of an edge langmuir probe corresponding
to these waves have been observed. The number of peaks and
their magnitude increases with rf power. The incremental
energy confinement time and percent of rf power absorbed as
well as the radial power deposition profile for a variety of
plasmas and antenna phasing has been explored utilizing
amplitude modulated rf power waveforms. Differences in these
quantities between deuterium and helium plasmas and with
varying applied wave spectra have been found and will be
compared to macroscopic plasma parameters and theory.
[CO3.013] High Harmonic Fast Wave Heating on NSTX- II
P. Ryan, D. Swain (ORNL), J. R. Wilson, S. Bernabei, T. Biewer, S. Diem, J. Hosea, B. LeBlanc, C. K. Phillips (PPPL)
HHFW experiments have been carried out in both RF-heated
plasmas and RF+NBI-heated plasmas. In RF-only plasmas, the
heating efficiency was greatest for 14 m^-1, decreased
as the wavenumber was decreased to 7 m^-1, and was
minimal for 3 m^-1 operation. The decrease in heating
efficiency follows increasingly centralized power
deposition. H-mode was obtained for double-null diverted
(DND) plasmas for symmetric spectra at both 14 m^-1 and
7 m^-1. Current drive measurements were obtained from
the differences in loop voltages for co- and counter-current
directions for the same plasma conditions. The normalized CD
efficiency obtained at wavenumbers of ±7 m^-1 in DND He
plasmas was similar to those previously obtained in D and He
lower single-null diverted plasmas at lower densities. CD
attempted at –3 m^-1 (after preheating the plasma to
Te(0) = 2 keV with 3 MW at 7 m^-1) was unsuccessful due
to rapid collapse of the temperature and stored energy. A
fraction of the HHFW power is absorbed by fast particles
during combined operation with NBI.
[CO3.014] Progress in EBW Current Drive Research Towards Enabling Sustained High Beta, Solenoid-Free Operation on NSTX
G. Taylor, P.C. Efthimion, C.E. Kessel (Princeton U.), G.L. Bell, T.S. Bigelow, M.D. Carter, J.B. Caughman, F. Jaeger, D.A. Rasmussen, J.B. Wilgen (ORNL), R.W. Harvey (CompX), C.B. Forest (U. of Wisconsin)
Off-axis rf-driven current can play a critical role in
sustaining high beta spherical torus (ST) plasmas without a
central solenoid. Numerical modeling of electron Bernstein
wave current drive (EBWCD) for a beta \sim 40% ST plasma
predicts efficient, EBWCD at r/a > 0.5 where the large
trapped electron fraction provides favorable conditions for
Ohkawa EBWCD. Normalized EBWCD efficiency increases with r/a
and is a factor of two higher at r/a = 0.7 than has been
obtained with ECCD near the axis of large aspect ratio
Tokamaks. Calculations predict 3-4 MW of 28 GHz RF power
would maintain the \sim 100 kA off-axis current needed to
stabilize a beta \sim 40% plasma. Modeling shows that
efficient coupling to EBWs can be readily accomplished using
near-circularly polarized electromagnetic waves via an
``O-X-B" oblique launch to the confining magnetic field.
Initial measurements of EBW emission support pursuing this
approach.
[CO3.015] Ideal MHD stability of the Component Test Facility and Culham Spherical Tokamak Power Plant
O. Keating, H. R. Wilson (EURATOM/UKAEA Fusion Association, Culham Science Centre, OX14 3DB, UK.), M. J. Hole (School of Physics, University of Sydney 2006, NSW, Australia.)
As well as complementing the physics base for ITER, theory and progress in Spherical Tokamak (ST) experiments have prompted design studies into next step ST devices such as the Component Test Facility (CTF) [1], and ST power plants such as the 3GW (fusion) / 1GW (electric) Culham ST Power Plant (STPP) [2]. In this study, low toroidal wave number (n=0,1,2,3) and ballooning (n=\infty) ideal MHD stability of the CTF and STPP concepts is addressed: for low n modes scans of growth rate with conformal wall radius and on-axis safety factor q_0 are performed, whilst for ballooning modes the proximity to the marginally stable pressure-driven boundaries assessed. Stable equilibria are reported in both configurations, consolidating the viability of the ST line. Time permitting, the effects of toroidal flow will be qualitatively investigated, and the role of fast particles discussed.
[1] H. R. Wilson et al, EPS Conf. Plasma Phs., P4-196. 2004. [2] H. R. Wilson et al, in-press, Nuc. Fus. 2004.