2003
DOI: 10.1088/0741-3335/45/12a/025
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Computation of electromagnetic turbulence and anomalous transport mechanisms in tokamak plasmas

Abstract: The basic scales of motion and computational requirements for low frequency fluid drift turbulence are summarised in tutorial fashion. Basic signatures for each of the competing eigenmode types are given, some of which are accessible experimentally. The emphasis is on edge turbulence since it is less intuitive. The difference in physical mechanism between linear instabilities and fully developed turbulence at the same parameters is shown. The difference in physical character from more familiar MHD models is al… Show more

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Cited by 98 publications
(165 citation statements)
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“…[21][22][23][24][25] Furthermore, the periodic axial boundary conditions used in the LAPD turbulence simulation are obviously unphysical, and more realistic boundary conditions may change the parallel dynamics disallowing an exact n 6 ¼ 0 $ n ¼ 0 path.…”
Section: Linear Versus Nonlinear Instability Drivementioning
confidence: 99%
See 2 more Smart Citations
“…[21][22][23][24][25] Furthermore, the periodic axial boundary conditions used in the LAPD turbulence simulation are obviously unphysical, and more realistic boundary conditions may change the parallel dynamics disallowing an exact n 6 ¼ 0 $ n ¼ 0 path.…”
Section: Linear Versus Nonlinear Instability Drivementioning
confidence: 99%
“…They are after all, not essential to the otherwise similar nonlinear drift-like instabilities in the tokamak edge simulations. [21][22][23][24][25] Now, there are a few ways to eliminate the flute modes in the simulation, such as eliminating one of the nonlinearities that is essential to the nonlinear instability process described in Fig. 5.…”
Section: Linear Versus Nonlinear Instability Drivementioning
confidence: 99%
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“…It can be regarded as one of the most intriguing results of half a century in physics of hot magnetized plasmas, that in macroscopically stable equilibria the confinement is nevertheless determined by micro-scale instabilities and fluctuations, with transport of energy and particles across magnetic flux surfaces being dominated by ubiquitous turbulence on small (gyro radius) scales and low (drift) frequencies [1,2,3,4,5,6,7]. This turbulence is regulated by the formation of mesoscopic zonal structures out of the turbulent flows [8,9,10,11,12,13].…”
Section: Introductionmentioning
confidence: 99%
“…[44]. A single gyro-fluid microtearing simulation has also previously been reported [47], but with little discussion of the resulting turbulence characteristics and transport dependencies.…”
Section: Introductionmentioning
confidence: 99%