Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session NP11: Poster Session V: Laser-plasma Particle Acceleration; HEDP; Turbulence and Transport; DIII-D Tokamak; Machine Learning, Data Science (9:30am-12:30pm)
Wednesday, November 7, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.NP11.91
Abstract: NP11.00091 : L-H Transition Dynamics in ITER-Similar Plasmas with Applied n=3 Resonant Magnetic Perturbations*
Presenter:
L. Schmitz
(University of California Los Angeles)
Authors:
L. Schmitz
(University of California Los Angeles)
T.L. Rhodes
(University of California Los Angeles)
L. Zeng
(University of California Los Angeles)
M. Kriete
(University of Wisconsin, Madison)
Z. Yan
(University of Wisconsin, Madison)
G. R. McKee
(University of Wisconsin, Madison)
R. Wilcox
(ORNL)
C. Paz-Soldan
(General Atomics)
P. Gohil
(General Atomics)
C. C. Petty
(General Atomics)
A. Marinoni
(MIT)
In ITER-similar plasmas in DIII-D (<ne>=1.5-5x1019m-3, Bt=1.9-2T, Ip=1.5MA, q95~3.6), the L-H threshold power PLH with n=3 Resonant Magnetic Perturbations (RMP) is found to increase with decreasing collisionality [PLH~(nu*)-0.3]. This is a concern for H-mode access in primarily ECH-heated ITER plasmas since RMP may be applied before the L-H transition to safely suppress the first ELM. Non-axisymmetric modifications of the L-mode shear layer with RMP include a substantial local reduction of the Er well and ExB shear (including Er reversal at high RMP field), and spatially modulated low-wavenumber turbulence amplitude, increasing substantially on field lines mapped to high RMP field. Two-fluid M3D-C1 modeling [1,2] shows that the normalized gradients a/L_n, a/L_Te are toroidally modulated and periodically increased on the outboard midplane with RMP. The increase in PLH is atttributed to the combined effects of reduced (and non-axisymmetric) ExB flow / flow shear, and locally enhanced instability drive (via increased kinetic gradients). [1] N.M. Ferraro,Phys. Plasmas 19 056105 (2012); [2] R.S. Wilcox et al. Phys. Plasmas 25 056108 (2018).
**This work supported by the US Department of Energy under DE-FG02-08ER54984, DE-FG02-89ER53296, DE-FG02-08ER 54999, and DE-FC02-04ER54698.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.NP11.91
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