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Juno Jupiter image

Greg Colyer

Visitor

Research theme

  • Climate physics
  • Exoplanets and planetary physics
  • Plasma physics

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Geophysical and Astrophysical Fluid Dynamics
Telephone: 01865 (2)82436
Atmospheric Physics Clarendon Laboratory, room 209E
  • About
  • Publications

Plasma rotation and transport in MAST spherical tokamak

Nuclear Fusion 51:6 (2011)

Authors:

AR Field, C Michael, RJ Akers, J Candy, G Colyer, W Guttenfelder, YC Ghim, CM Roach, S Saarelma

Abstract:

The formation of internal transport barriers (ITBs) is investigated in MAST spherical tokamak plasmas. The relative importance of equilibrium flow shear and magnetic shear in their formation and evolution is investigated using data from high-resolution kinetic- and q-profile diagnostics. In L-mode plasmas, with co-current directed NBI heating, ITBs in the momentum and ion thermal channels form in the negative shear region just inside qmin. In the ITB region the anomalous ion thermal transport is suppressed, with ion thermal transport close to the neo-classical level, although the electron transport remains anomalous. Linear stability analysis with the gyro-kinetic code GS2 shows that all electrostatic micro-instabilities are stable in the negative magnetic shear region in the core, both with and without flow shear. Outside the ITB, in the region of positive magnetic shear and relatively weak flow shear, electrostatic micro-instabilities become unstable over a wide range of wave numbers. Flow shear reduces the linear growth rates of low-k modes but suppression of ITG modes is incomplete, which is consistent with the observed anomalous ion transport in this region; however, flow shear has little impact on growth rates of high-k, electron-scale modes. With counter-NBI ITBs of greater radial extent form outside qmin due to the broader profile of E 脳 B flow shear produced by the greater prompt fast-ion loss torque. 漏 2011 IAEA, Vienna.

Global gyrokinetic ITG turbulence simulations of MAST plasmas

37th EPS Conference on Plasma Physics 2010, EPS 2010 1 (2010) 521-524

Authors:

S Saarelma, A Bottino, J Candy, G Colyer, A Field, W Gutenfelder, P Hill, A Peeters, CM Roach

Gyrokinetic simulations of spherical tokamaks

Plasma Physics and Controlled Fusion 51:12 (2009)

Authors:

CM Roach, IG Abel, RJ Akers, W Arter, M Barnes, Y Camenen, FJ Casson, G Colyer, JW Connor, SC Cowley, D Dickinson, W Dorland, AR Field, W Guttenfelder, GW Hammett, RJ Hastie, E Highcock, NF Loureiro, AG Peeters, M Reshko, S Saarelma, AA Schekochihin, M Valovic, HR Wilson

Abstract:

This paper reviews transport and confinement in spherical tokamaks (STs) and our current physics understanding of this that is partly based on gyrokinetic simulations. Equilibrium flow shear plays an important role, and we show how this is consistently included in the gyrokinetic framework for flows that greatly exceed the diamagnetic velocity. The key geometry factors that influence the effectiveness of turbulence suppression by flow shear are discussed, and we show that toroidal equilibrium flow shear can sometimes entirely suppress ion scale turbulence in today's STs. Advanced nonlinear simulations of electron temperature gradient (ETG) driven turbulence, including kinetic ion physics, collisions and equilibrium flow shear, support the model that ETG turbulence can explain electron heat transport in many ST discharges. 漏 2009 IOP Publishing Ltd.

Testing the Trapped Gyro-Landau Fluid Transport Model with Data from Tokamaks and Spherical Tori

Proc. 22nd IAEA FEC (2008)

Authors:

GM Staebler, G Colyer, S Kaye, JE Kinsey, RE Waltz

Collisionality scaling of the electron heat flux in ETG turbulence

Plasma Physics and Controlled Fusion IOP Publishing: Hybrid Open Access

Authors:

GJ Colyer, AA Schekochihin, FI Parra, CM Roach, MA Barnes, Y-C Ghim, W Dorland

Abstract:

In electrostatic simulations of MAST plasma at electron-gyroradius scales, using the local flux-tube gyrokinetic code GS2 with adiabatic ions, we find that the long-time saturated electron heat flux (the level most relevant to energy transport) decreases as the electron collisionality decreases. At early simulation times, the heat flux "quasi-saturates" without any strong dependence on collisionality, and with the turbulence dominated by streamer-like radially elongated structures. However, the zonal fluctuation component continues to grow slowly until much later times, eventually leading to a new saturated state dominated by zonal modes and with the heat flux proportional to the collision rate, in approximate agreement with the experimentally observed collisionality scaling of the energy confinement in MAST. We outline an explanation of this effect based on a model of ETG turbulence dominated by zonal-nonzonal interactions and on an analytically derived scaling of the zonal-mode damping rate with the electron-ion collisionality. Improved energy confinement with decreasing collisionality is favourable towards the performance of future, hotter devices.

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