Bulletin of the American Physical Society
66th Annual Meeting of the APS Division of Plasma Physics
Monday–Friday, October 7–11, 2024; Atlanta, Georgia
Session JP12: Poster Session IV:
Stellarators: W7-X, LHD, HSX, CTH, Others
Low Aspect Ratio Tokamaks
Particle acceleration, beams and relativistic plasmas: Laser-plasma ion acceleration
Plasma-based wakefield accelerators and Analytical and computational techniques
Astrophysical Plasmas
2:00 PM - 5:00 PM
Tuesday, October 8, 2024
Hyatt Regency
Room: Grand Hall West
Abstract: JP12.00101 : Investigation of Micro-Tearing Modes on MAST-U*
Presenter:
Mate Lampert
(Princeton Plasma Physics Laboratory)
Authors:
Mate Lampert
(Princeton Plasma Physics Laboratory)
Steven Thomas
(University of York)
Jason F Parisi
(Princeton Plasma Physics Laboratory, Princeton University)
Jack W Berkery
(Princeton Plasma Physics Laboratory)
Sam Blackmore
(UKAEA - United Kingdom Atomic Energy Authority)
Daniel Dunai
(HUN-REN Centre for Energy Research, Budapest, Hungary)
Sarah Elmore
(UKAEA - United Kingdom Atomic Energy Authority)
Clive Alvin Michael
(University of California)
David Ryan
(UKAEA - United Kingdom Atomic Energy Authority)
Rory Scannell
(UKAEA - United Kingdom Atomic Energy Authority)
Collaboration:
MAST-U
MTMs were investigated in the previous two measurement campaigns in dedicated experiments on the MAST-U spherical tokamak. Rapid vertical displacements were introduced to high beta type 1 ELMy H-mode plasmas to align a rational magnetic surface with the peak of the omega* profile. Collisionality was kept low by heating the plasma with all available neutral beam heating power. The spectrograms of magnetic and density fluctuations were calculated and the origins of the coherent frequency bands were investigated to identify MTMs amongst other coherent fluctuations. The growth rate and the expected frequency of the MTMs were calculated with gyrokinetic simulations and were compared to the experimental findings.
*This work was supported by U.S. DOE Contract No. DE-AC02-09CH11466 (PPPL).
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