Initialising ...
Initialising ...
Initialising ...
Initialising ...
Initialising ...
Initialising ...
Initialising ...
Onuki, Yoshichika; Settai, Rikio*; Haga, Yoshinori; Machida, Yo*; Izawa, Koichi*; Honda, Fuminori*; Aoki, Dai*
Comptes Rendus Physique, 15(7), p.616 - 629, 2014/08
Times Cited Count:6 Percentile:44.73(Astronomy & Astrophysics)Aoki, Dai*; Hardy, F.*; Miyake, Atsushi*; Taufour, V.*; Matsuda, Tatsuma; Flouquet, J.*
Comptes Rendus Physique, 12(5-6), p.573 - 583, 2011/06
Times Cited Count:34 Percentile:80.8(Astronomy & Astrophysics)Bulanov, S. V.; Esirkepov, T. Z.; Pegoraro, F.*; Borghesi, M.*
Comptes Rendus Physique, 10(2-3), p.216 - 226, 2009/03
Times Cited Count:20 Percentile:70.62(Astronomy & Astrophysics)Idomura, Yasuhiro; Watanabe, Tomohiko*; Sugama, Hideo*
Comptes Rendus Physique, 7(6), p.650 - 669, 2006/07
Times Cited Count:23 Percentile:39.33(Astronomy & Astrophysics)In contrast to neutral fluid turbulence described in three-dimensional (3D) configuration space, collisionless magnetised plasma turbulence has been studied using the gyrokinetic model, which is a reduced kinetic model of a plasma in 5D phase space. Recent advances in computer technology and simulation models enabled a direct numerical simulation of plasma turbulence in a toroidal configuration with experimentally relevant parameters. Such kinetic simulations have been established as an essential tool for studying turbulent transport in a fusion plasma. This overview summarises progress in kinetic simulations of turbulent fusion plasmas focusing on physical and numerical models and physical findings obtained from 5D gyrokinetic simulations.