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Theoretical physicists working at a blackboard collaboration pod in the Beecroft building.
Credit: Jack Hobhouse

Prof Michael Barnes

Professor in Theoretical Physics

Sub department

  • Rudolf Peierls Centre for Theoretical Physics

Research groups

  • Theoretical astrophysics and plasma physics at RPC
michael.barnes@physics.ox.ac.uk
Telephone: 01865 (2)73960
Rudolf Peierls Centre for Theoretical Physics, room 50.10
  • About
  • Publications

Gyrokinetic simulations in stellarators using different computational domains

(2021)

Authors:

E Sánchez, JM García-Regaña, A Bañón Navarro, JHE Proll, C Mora Moreno, A González-Jerez, I Calvo, R Kleiber, J Riemann, J Smoniewski, M Barnes, FI Parra
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Details from ArXiV

Continuous-in-time approach to flow shear in a linearly implicit local δf gyrokinetic code

Journal of Plasma Physics Cambridge University Press 87:2 (2021) 905870230

Authors:

Nicolas Christen, Michael Barnes, Felix I Parra

Abstract:

A new algorithm for toroidal flow shear in a linearly implicit, local δf gyrokinetic code is described. Unlike the current approach followed by a number of codes, it treats flow shear continuously in time. In the linear gyrokinetic equation, time-dependences arising from the presence of flow shear are decomposed in such a way that they can be treated explicitly in time with no stringent constraint on the time step. Flow shear related time dependences in the nonlinear term are taken into account exactly, and time dependences in the quasineutrality equation are interpolated. Test cases validating the continuous-in-time implementation in the code GS2 are presented. Lastly, nonlinear gyrokinetic simulations of a JET discharge illustrate the differences observed in turbulent transport compared with the usual, discrete-in-time approach. The continuous-in-time approach is shown, in some cases, to produce fluxes that converge to a different value than with the discrete approach. The new approach can also lead to substantial computational savings by requiring radially narrower boxes. At fixed box size, the continuous implementation is only modestly slower than the previous, discrete approach.
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Impact of shaping on microstability in high-performance tokamak plasmas

Nuclear Fusion IOP Publishing 61:6 (2021) 66020

Authors:

O Beeke, M Barnes, M Romanelli, M Nakata, M Yoshida

Abstract:

We have used the local-δf gyrokinetic code GS2 to perform studies of the effect of flux-surface shaping on two highly-shaped, low- and high-β JT-60SA-relevant equilibria, including a successful benchmark with the GKV code. We find that for a high-performance plasma, i.e. one with high plasma beta and steep pressure gradients, the turbulent outwards radial fluxes may be reduced by minimizing the elongation. We explain the results as a competition between the local magnetic shear and finite-Larmor-radius (FLR) stabilization. Electromagnetic studies indicate that kinetic ballooning modes are stabilized by increased shaping due to an increased sensitivity to FLR effects, relative to the ion-temperature-gradient instability. Nevertheless, at high enough β, increased elongation degrades the local magnetic shear stabilization that enables access to the region of ballooning second-stability.
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Turbulent impurity transport simulations in Wendelstein 7-X plasmas

Journal of Plasma Physics Cambridge University Press 87:1 (2021) 855870103

Authors:

Jm Garcia-Regana, M Barnes, I Calvo, Fi Parra, Ja Alcuson, R Davies, A Gonzalez-Jerez, A Mollen, E Sanchez, Jl Velasco, A Zocco

Abstract:

A study of turbulent impurity transport by means of quasilinear and nonlinear gyrokinetic simulations is presented for Wendelstein 7-X (W7-X). The calculations have been carried out with the recently developed gyrokinetic code stella. Different impurity species are considered in the presence of various types of background instabilities: ion temperature gradient (ITG), trapped electron mode (TEM) and electron temperature gradient (ETG) modes for the quasilinear part of the work; ITG and TEM for the nonlinear results. While the quasilinear approach allows one to draw qualitative conclusions about the sign or relative importance of the various contributions to the flux, the nonlinear simulations quantitatively determine the size of the turbulent flux and check the extent to which the quasilinear conclusions hold. Although the bulk of the nonlinear simulations are performed at trace impurity concentration, nonlinear simulations are also carried out at realistic effective charge values, in order to know to what degree the conclusions based on the simulations performed for trace impurities can be extrapolated to realistic impurity concentrations. The presented results conclude that the turbulent radial impurity transport in W7-X is mainly dominated by ordinary diffusion, which is close to that measured during the recent W7-X experimental campaigns. It is also confirmed that thermodiffusion adds a weak inward flux contribution and that, in the absence of impurity temperature and density gradients, ITG- and TEM-driven turbulence push the impurities inwards and outwards, respectively.
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Details from ArXiV

Preparing for first diverted plasma operation in the ST40 high-field spherical tokamak

47th EPS Conference on Plasma Physics, EPS 2021 2021-June (2021) 681-684

Authors:

M Romanelli, S McNamara, P Buxton, O Asunta, J Varje, J Wood, C Marsden, J Bland, V Nemytov, P Thomas, M Gryaznevich, M Sertoli, B Vincent, S Sridhar, A Dnestrovsky, S Medvedev, V Drozdov, S Janhunen, J Sinha, T Bogaarts, G Rubino, P Innocenti, G Calabro, M Scarpari, P Fanelli, F Giorgetti, R Lombroni, S Kaye, A Diallo, W Guttenfelder, M Barnes, Y Zhang

Abstract:

The ST40 tokamak [1], built and operated by Tokamak Energy, has recently been upgraded with upper and lower divertors to enable double null diverted operations with up to 1MA plasma current and 2MW neutral beam heating. ST40 is a high field spherical tokamak (ST), BT=3T at R0=0.4m with a goal to extend the high field spherical tokamak physics basis. Crucially, transport and confinement in high field, high temperature STs will be explored in support to the design of next step STs [2]. Extensive modelling activities have been undertaken to prepare for the exploitation of ST40. A range of plasma equilibrium in double-null configuration have been designed along with detailed scenario modelling, including 1.5D transport simulations and 2D SOL modelling. Gyrokinetic analysis has been performed to assess the level of expected turbulent transport. Building upon the NSTX pedestal database the pedestal width and height in the high performance ST40 scenarios have been predicted. MHD stability analysis and beta limit have been assessed. ST40 will be initially operated in hydrogen with up to 1.5 MW NBI (0.8MW at 55kV and 0.7MW at 25kV). The heating systems will be upgraded in view of the follow up campaign in deuterium, with 2MW, 55kV NBI and around 1.6MW 105/140GHz ECRH. Careful analysis of the power deposited in the divertor during high performance operation has also been carried out.

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