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- W4296699993 abstract "Abstract The mean E <?CDATA $ times $?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:mo>×</mml:mo> </mml:math> B shear in a stochastic magnetic field is calculated, using the radial force balance relation and transport equations. This analysis is relevant to the L → H transition with resonant magnetic perturbations, and special focus is placed upon the physics of non-ambipolar transport and radial current. The key physical process is the flow of fluctuating currents along wandering magnetic fields. The increments in poloidal and toroidal rotation, density and ion pressure are calculated. The radial envelope of the magnetic perturbations inside the plasma defines a new scale <?CDATA ${ell _{{text{env}}}}$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:mrow> <mml:msub> <mml:mi>ℓ</mml:mi> <mml:mrow> <mml:mrow> <mml:mtext>env</mml:mtext> </mml:mrow> </mml:mrow> </mml:msub> </mml:mrow> </mml:math> , which is the characteristic scale of the magnetic fluctuation intensity profile. The net particle outflow due to stochastic magnetic fields is calculated and is determined by the net radial current through the separatrix. Implications for the L → H transition are discussed." @default.
- W4296699993 created "2022-09-23" @default.
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- W4296699993 date "2022-10-18" @default.
- W4296699993 modified "2023-10-14" @default.
- W4296699993 title "Theory of mean E × B shear in a stochastic magnetic field: ambipolarity breaking and radial current" @default.
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- W4296699993 doi "https://doi.org/10.1088/1361-6587/ac93b0" @default.
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