1979
DOI: 10.1088/0029-5515/19/9/011
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Anomalous ion loss due to low-frequency instabilities

Abstract: An ambipolarity formula for the cross-field flux of non-uniform plasma in the presence of low-frequency (ω ≪ ion gyrofrequency) electromagnetic fluctuations is presented. It is shown that, owing to ion polarization drift, the ions are pulled out by the diffusing electrons.

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Cited by 19 publications
(16 citation statements)
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“…By virtue of the poloidal momentum conservation, however, the reaction force on electrons F W eh should have the same magnitude of and the opposite direction to F W ih on ions. This implies that the transport induced by this force is the same for electrons and ions, that is, intrinsically ambipolar [28]. On the other hand, if the fluctuations do propagate radially, they may act as a perpendicular viscosity.…”
Section: Forces Induced By Turbulent Fluctuationsmentioning
confidence: 99%
“…By virtue of the poloidal momentum conservation, however, the reaction force on electrons F W eh should have the same magnitude of and the opposite direction to F W ih on ions. This implies that the transport induced by this force is the same for electrons and ions, that is, intrinsically ambipolar [28]. On the other hand, if the fluctuations do propagate radially, they may act as a perpendicular viscosity.…”
Section: Forces Induced By Turbulent Fluctuationsmentioning
confidence: 99%
“…For low-frequency electromagnetic and electrostatic fluctuations ͑ Ӷ ci ͒, where ci is ion gyrofrequency, the total radial flux of ions ͑⌫ i T ͒ and electrons ͑⌫ e T ͒ can be written in the form, 13,15 …”
Section: B Transport and Perpendicular Flowmentioning
confidence: 99%
“…(5a), not shown here, and are estimated to be smaller than hj k b r i=B for MST plasmas]. The first term is an ion polarization drift where V A is the Aflven speed [19], the second term is the charge flux generated only by magnetic fluctuations, and the last term is the classical charge flux arising from the radial flow due to the F B drift, where F is the viscous force within the magnetic surface perpendicular to B [11]. In the last term, is perpendicular viscosity coefficient and V EB ÿE r =B is a fluctuation-induced mean flow.…”
mentioning
confidence: 90%