e d fredrickson a, j menard a, d. stutman b, k. tritz b a princeton plasma physics laboratory, nj b...

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 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

Page 2: 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

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.

Page 3: 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

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.

Page 4: 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

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.

Page 5: 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

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

Page 6: 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

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.

Page 7: 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 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

Page 8: 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

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.

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