Zero-Turbulence Manifold in a Toroidal Plasma

ArXiv 1203.6455 (2012)

Authors:

EG Highcock, AA Schekochihin, SC Cowley, M Barnes, FI Parra, CM Roach, W Dorland

Abstract:

Sheared toroidal flows can cause bifurcations to zero-turbulent-transport states in tokamak plasmas. The maximum temperature gradients that can be reached are limited by subcritical turbulence driven by the parallel velocity gradient. Here it is shown that q/\epsilon (magnetic field pitch/inverse aspect ratio) is a critical control parameter for sheared tokamak turbulence. By reducing q/\epsilon, far higher temperature gradients can be achieved without triggering turbulence, in some instances comparable to those found experimentally in transport barriers. The zero-turbulence manifold is mapped out, in the zero-magnetic-shear limit, over the parameter space (\gamma_E, q/\epsilon, R/L_T), where \gamma_E is the perpendicular flow shear and R/L_T is the normalised inverse temperature gradient scale. The extent to which it can be constructed from linear theory is discussed.

Zero-Turbulence Manifold in a Toroidal Plasma

(2012)

Authors:

EG Highcock, AA Schekochihin, SC Cowley, M Barnes, FI Parra, CM Roach, W Dorland

Intrinsic rotation with gyrokinetic models

ArXiv 1203.4958 (2012)

Authors:

Felix I Parra, Michael Barnes, Ivan Calvo, Peter J Catto

Abstract:

The generation of intrinsic rotation by turbulence and neoclassical effects in tokamaks is considered. To obtain the complex dependences observed in experiments, it is necessary to have a model of the radial flux of momentum that redistributes the momentum within the tokamak in the absence of a preexisting velocity. When the lowest order gyrokinetic formulation is used, a symmetry of the model precludes this possibility, making small effects in the gyroradius over scale length expansion necessary. These effects that are usually small become important for momentum transport because the symmetry of the lowest order gyrokinetic formulation leads to the cancellation of the lowest order momentum flux. The accuracy to which the gyrokinetic equation needs to be obtained to retain all the physically relevant effects is discussed.

Intrinsic rotation with gyrokinetic models

(2012)

Authors:

Felix I Parra, Michael Barnes, Ivan Calvo, Peter J Catto

Gravitational Wave Heating of Stars and Accretion Disks

(2012)

Authors:

Gongjie Li, Bence Kocsis, Abraham Loeb