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 UP11: Poster Session VIII: MST; DIII-D Tokamak; SPARC, C-Mod, and High Field Tokamaks; HBT-EP; Transport and LPI in ICF Plasmas, Hydrodynamic Instability; HEDP Posters; Space and Astrophysical Plasmas (2:00pm-5:00pm)
Thursday, November 8, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.UP11.56
Abstract: UP11.00056 : Creation and Sustainment of Quiescent H-mode Plasmas in DIII-D with Zero Net NBI Torque*
Presenter:
K.H. Burrell
(General Atomics)
Authors:
K.H. Burrell
(General Atomics)
Xi Chen
(General Atomics)
T.H. Osborne
(General Atomics)
C. Paz-Soldan
(General Atomics)
T.M. Wilks
(PSFC-MIT)
Recent experiments have demonstrated both creation and sustainment of wide pedestal QH-mode with zero net neutral beam injected (NBI) torque. QH-mode is an attractive operating regime for future devices since it has excellent energy confinement time and can operate without ELMs at zero net NBI torque. Wide pedestal QH-mode exhibits an increase in the pedestal pressure height and width and increased global energy confinement associated with a bipolar change in the edge ExB shear [1]. Previous low torque QH-mode shots utilized a startup phase with significant NBI torque which was reduced to zero later in the shot. Since future devices will not have appreciable NBI torque, creation and sustainment of QH-mode at zero NBI torque is an important step towards using QH-mode in those devices. These recent shots have plasma conditions relevant for future devices: βN = 1.75, ITER H98y2 = 1.25, ν*ePED = 0.3-0.4 and stationary conditions for at least 20 energy confinement times, limited only by hardware constraints. Unlike the rapid transition to wide pedestal conditions seen previously [1], the wide pedestal state forms gradually over a period of roughly 100 ms in the present cases
[1] K.H. Burrell et al, Phys. Plasmas 23, 056103 (2016)
*Supported by US DOE under DE-FC02-04ER54698
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.UP11.56
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