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 UO5: Research in Support of ITER
2:00 PM–5:00 PM,
Thursday, November 8, 2018
OCC
Room: B113-114
Chair: Francesca Turco, Columbia University
Abstract ID: BAPS.2018.DPP.UO5.7
Abstract: UO5.00007 : Advancement of Wide Pedestal Quiescent H-mode Scenario at Zero Torque to ITER-like Shape*
3:12 PM–3:24 PM
Presenter:
Theresa M Wilks
(Massachusetts Inst of Tech-MIT)
Authors:
Theresa M Wilks
(Massachusetts Inst of Tech-MIT)
Carlos Alberto Paz-Soldan
(General Atomics - San Diego)
Jerry W Hughes
(Massachusetts Inst of Tech-MIT)
Kshitish Kumar Barada
(Univ of California - Los Angeles)
Keith Burrell
(General Atomics)
Xi Chen
(General Atomics - San Diego)
Andrea MV Garofalo
(General Atomics - San Diego)
Darin R Ernst
(Massachusetts Inst of Tech-MIT)
Philip B Snyder
(General Atomics - San Diego)
Recent experiments on DIII-D have advanced the operational limits of wide pedestal QH-mode plasmas towards increased ITER relevance by demonstrating well-matched plasma shape and net zero injected torque simultaneously. Quiescent H-modes (QH-modes) are a candidate regime for ITER and future reactors because they maintain a stationary pedestal without ELMs via additional edge transport generated by either an edge harmonic oscillation (EHO), broadband turbulence, a limit cycle oscillation (LCO), or some combination thereof. Comparing to the traditional double null shape, the ITER-like shape is shown to have 1) a narrower pedestal width, 2) lower frequency LCOs, yet larger density fluctuations, and 3) larger ExB shear in the inner Er well pedestal region. In the peeling-ballooning stability space, the ITER-like shape operates far from the kink/peeling boundary, suggesting much higher power and possibly wider pedestal operation can be achieved in future experiments. The H98y2 confinement factor was shown to increase with pedestal width, suggesting a favorable scaling for ITER in this regime.
*Work supported by the U.S. DOE under DE-FC02-04ER54698 and DE-SC0014264.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.UO5.7
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