About the speaker:
Dr Bhavin Patel is a senior turbulence and transport modeller working at UKAEA with a focus on spherical tokamaks and high β turbulence. His major areas of focus are designing experiments on MAST-Upgrade to examine turbulence, modelling turbulence in spherical tokamaks using gyrokinetics and performing predictive simulations of transport for the STEP power plant design. He has been working at UKAEA there since 2021, before which he did his PhD with the Fusion CDT at the University of York where he examined some of the challenges of designing a conceptual spherical tokamak power plant that could produce net electricity and the type of turbulence expected to form in such a regime.
Abstract:
Gyrokinetic analysis of the core plasma in MAST-U
Understanding the core confinement of spherical tokamaks is critical for achieving high-performance plasmas. MAST-Upgrade provides a valuable opportunity to benchmark first-principles-based model predictions against experimental results, given the high-quality diagnostic data available.
This study examines the nature of core turbulence that develops across different operational regimes in MAST-U. Transport analysis indicates that in both L-mode and H-mode regimes, there is significant anomalous electron heat transport, whereas ion heat transport remains at neoclassical levels. Furthermore, core performance in MAST-U often deteriorates due to the onset of an MHD-driven locked mode, which significantly reduces plasma rotation. The impact of this reduction on turbulence is explored here.
An L-mode and an H-mode discharge, corresponding to low and high achieved plasma β respectively, are analysed using gyrokinetic modelling. In the L-mode discharge, a range of instabilities are identified at both electron and ion scales, highlighting the multiscale nature of turbulence in MAST-U. At higher β, electron-scale turbulence is stabilized, with electromagnetic instabilities forming at the ion scale. In both scenarios, fast ions are found to have a much more significant impact deeper with the core plasma. Nonlinear analysis further reveals the stiff nature of turbulence in both regimes and the strong influence of rotation shear.
Environmental Statement Modern Slavery Act Accessibility Disclaimer Terms & Conditions Privacy Policy Code of Conduct About IOP
© 2021 IOP All rights reserved.
The Institute is a charity registered in England and Wales (no. 293851) and Scotland (no. SC040092)