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• W2336449130 abstract "The impact of rotating magnetic islands on background radial profiles in a the presence of strong turbulent transport is analysed, with particular a emphasis on island widths of the order of 6-10 ion Larmor radii. Only a the case of ion temperature gradient (ITG) turbulence is considered. A a significant reduction of fluctuations is found when island and a turbulence co-rotate and the island width is of the order of the radial a correlation length of turbulence. This reduction is not due to a a flattening of ion temperature, suggesting an additional mechanism. A a nonlinear transfer of energy from small to large scale structures might a be responsible for the stabilization at a scale close to the radial a correlation length of turbulence. It is shown that in the presence of a intermediate magnetic islands rotating in the ion diamagnetic direction a the density flattening survives the radial turbulent transport, a representing a destabilizing effect for a magnetic island in terms of a bootstrap current. However, this flattening is not necessarily due to an a adiabatic response of trapped ions. Owing to the fast parallel motion of a electrons, their temperature is always flattened. Finally, when the a island width is large enough (island width greater than 18 ion Larmor a radii), the standard profile flattening leading to a linear a stabilization of turbulence dominates over the other mechanisms." @default.
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• W2336449130 date "2015-09-01" @default.
• W2336449130 modified "2023-09-26" @default.
• W2336449130 title "Impact of rotating magnetic islands on density profile flattening and turbulent transport" @default.
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• W2336449130 doi "https://doi.org/10.1088/0029-5515/55/11/113018" @default.
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