Gravitational wave heating of stars and accretion discs

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 425:4 (2012) 2407-2412

Authors:

Gongjie Li, Bence Kocsis, Abraham Loeb

Multiscale Gyrokinetics for Rotating Tokamak Plasmas: Fluctuations, Transport and Energy Flows

(2012)

Authors:

IG Abel, GG Plunk, E Wang, M Barnes, SC Cowley, W Dorland, AA Schekochihin

Orbital evolution of a planet on an inclined orbit interacting with a disc

(2012)

Authors:

Jean Teyssandier, Caroline Terquem, John CB Papaloizou

Experimental Signatures of Critically Balanced Turbulence in MAST

(2012)

Authors:

Y-C Ghim, AA Schekochihin, AR Field, IG Abel, M Barnes, G Colyer, SC Cowley, FI Parra, D Dunai, S Zoletnik, the MAST Team

Experimental Signatures of Critically Balanced Turbulence in MAST

ArXiv 1208.597 (2012)

Authors:

Y-C Ghim, AA Schekochihin, AR Field, IG Abel, M Barnes, G Colyer, SC Cowley, FI Parra, D Dunai, S Zoletnik, the MAST Team

Abstract:

Beam Emission Spectroscopy (BES) measurements of ion-scale density fluctuations in the MAST tokamak are used to show that the turbulence correlation time, the drift time associated with ion temperature or density gradients, the particle (ion) streaming time along the magnetic field and the magnetic drift time are consistently comparable, suggesting a "critically balanced" turbulence determined by the local equilibrium. The resulting scalings of the poloidal and radial correlation lengths are derived and tested. The nonlinear time inferred from the density fluctuations is longer than the other times; its ratio to the correlation time scales as $\nu_{*i}^{-0.8\pm0.1}$, where $\nu_{*i}=$ ion collision rate/streaming rate. This is consistent with turbulent decorrelation being controlled by a zonal component, invisible to the BES, with an amplitude exceeding the drift waves' by $\sim \nu_{*i}^{-0.8}$.