2001
DOI: 10.1134/1.1416202
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Plasma convection near the threshold for MHD instability in nonparaxial magnetic confinement systems

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Cited by 34 publications
(35 citation statements)
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“…For the high power heat source, quasilinear transport was present and large but was quickly replaced by the non-linear stage. A similar finding was reported by Pastukhov [9]. He observed that the quasilinear transport started to smooth the profiles, but was not dominant and was replaced by non-linear global plasma motion.…”
Section: Summary Of Simulation Resultssupporting
confidence: 88%
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“…For the high power heat source, quasilinear transport was present and large but was quickly replaced by the non-linear stage. A similar finding was reported by Pastukhov [9]. He observed that the quasilinear transport started to smooth the profiles, but was not dominant and was replaced by non-linear global plasma motion.…”
Section: Summary Of Simulation Resultssupporting
confidence: 88%
“…This behavior coincides with that seen by Pastukhov [9] in the quasi-stable state, while Makhnin reported smaller scale incoherent turbulence. Also, the development of large-scale convective cells in the nonlinear regime is supported by the theoretical analysis presented by Yoshizawa et.al.…”
Section: Numerical Simulationssupporting
confidence: 89%
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“…Non-linear studies indicate that large-scale convective cells will form when the MHD stability limit is weakly violated, which results in the circulation of plasma between the hot core and the cooler edge region [6]. Studies have also predicted that the confined plasma can be stable to low frequency (drift wave) modes when η=dln Te/d ln ne>2/3 [7].…”
Section: Introductionmentioning
confidence: 99%
“…In fact, Pastukhov and Chudin [23,24] show that this scaling persists even during the nonlinear phase of the evolution of the interchange instability.…”
Section: Cylindrical Resultsmentioning
confidence: 99%