E D Fredrickson a , J Menard a , D. Stutman b , K. Tritz b a Princeton Plasma Physics Laboratory, NJ b Johns Hopkins University, MD 46 th Annual Meeting of the Division of Plasma Physics, American Physical Society 15 – 19 November 2004 Savannah, Georgia Neoclassical tearing mode onset in NSTX Supported by Columbia U Comp-X General Atomics INEL Johns Hopkins U LANL LLNL Lodestar MIT Nova Photonics NYU ORNL PPPL PSI SNL UC Davis UC Irvine UCLA UCSD U Maryland U Rochester U Washington U Wisconsin Culham Sci Ctr Hiroshima U HIST Kyushu Tokai U Niigata U Tsukuba U U Tokyo JAERI Ioffe Inst TRINITI KBSI KAIST ENEA, Frascati CEA, Cadarache IPP, Jülich IPP, Garching U Quebec
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E D Fredrickson a, J Menard a, D. Stutman b, K. Tritz b a Princeton Plasma Physics Laboratory, NJ b Johns Hopkins University, MD 46 th Annual Meeting of.
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E D Fredricksona, J Menarda,
D. Stutmanb, K. Tritzb
a Princeton Plasma Physics Laboratory, NJb Johns Hopkins University, MD
46th Annual Meeting of the Division of Plasma Physics, American Physical Society
15 – 19 November 2004Savannah, Georgia
Neoclassical tearing mode onset in NSTX
Supported by
Columbia UComp-X
General AtomicsINEL
Johns Hopkins ULANLLLNL
LodestarMIT
Nova PhotonicsNYU
ORNLPPPL
PSISNL
UC DavisUC Irvine
UCLAUCSD
U MarylandU Rochester
U WashingtonU Wisconsin
Culham Sci CtrHiroshima U
HISTKyushu Tokai U
Niigata UTsukuba U
U TokyoJAERI
Ioffe InstTRINITI
KBSIKAIST
ENEA, FrascatiCEA, Cadarache
IPP, JülichIPP, Garching
U Quebec
Sawtooth crashes often trigger modes which appear similar to NTMs
• Toroidal mode number of n = 2 suggests NTM.
• Strong interaction with sawtooth instability, drop in amplitude at sawtooth.
• Can amplitude evolution be modeled with extended Rutherford equation?
• "Spontaneous" n = 2 modes are also seen.
Amplitude drop at sawteeth not predicted by Rutherford equation
• Amplitude evolution of 3/2 modeled with Rutherford equation, TRANSP.
• "NTM" coefficients adjusted to match Mirnov amplitude.
• Local parameters not affected by sawtooth crash - island width should evolve on resistive time scale.
• Need internal measurements.
Early in sawtooth period n=2 is kink-like, strong n=1 mode
• Weakly phase locked with 3:2 frequency match.
• n=2 not triggered through non-linear coupling to n=1.
• Are core oscillations a chord-integral effect?
• Sawtooth crash triggers n=2 kink?
• Insufficient data for tomography, use simulations.
Equilibrium J, q profiles are used to simulate 3/2 tearing mode
• Soft x-ray data Abel inverted on EFIT grid to find local emissivity.
• Emissivity remapped on island flux plot and chord integrated.
• Comparison to fluctuation amplitude in experimental data is used to constrain island size, eigenmode structure.
-10101Major Radius (m)111383_0.45s
Simulation suggests 2/2 persists in core, as at high aspect ratio
• Core oscillation's phase pattern, amplitude differs from simulation.
• Coupling to 2/2 mode may reduce classic ' of 3/2 mode.
• Or is this a 2/2 island? • q profile is not measured, adjusted
to match phase inversion.
The inferred q=1 radius is comparable to the inferred q=1.5 radius
• The q=1.5 radius was inferred from simulating the island inversion radius.
• Could these n = 2 modes be 2/2 kinks evolving to 2/2 islands?
• Radius of q=1 surface is ≈1.2 times the chord integrated inversion radius
Summary
• Studies of NTM onset in NSTX raise more questions than are answered.
• NTMs interact much more strongly with sawteeth than should be expected.
• SXI implies islands near q = 1 surface, i.e., islands are not 3/2 modes.
• Routine current profile measurements expected for next campaign; are key to progress.