1998
DOI: 10.1063/1.872772
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Role of ponderomotive density expulsion in ion Bernstein wave coupling to the core plasma

Abstract: When the density at the ion Bernstein wave ͑IBW͒ antenna is relatively low, mode transformation of the electron plasma wave to the IBW is sensitive to the density gradient scale length, and hence to ponderomotive effects. A second-order nonlinear ordinary differential equation that describes mode transformation at the lower-hybrid layer, including self-consistent ponderomotive density profile modification, is solved for the rf electrostatic potential in front of the IBW antenna, for the particular case of heat… Show more

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Cited by 9 publications
(13 citation statements)
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“…Non-linear interactions of the RF power with the plasma edge, such as RF sheaths and parametric instabilities, can produce poor IBW penetration in the bulk and impurity influxes. This is what inhibited the reproducibility of successful IBW results obtained in previous experiments [24,25,26]. Non-linear edge phenomena occur as a consequence of the onset of a strong turbulence regime.…”
Section: Introductionmentioning
confidence: 90%
“…Non-linear interactions of the RF power with the plasma edge, such as RF sheaths and parametric instabilities, can produce poor IBW penetration in the bulk and impurity influxes. This is what inhibited the reproducibility of successful IBW results obtained in previous experiments [24,25,26]. Non-linear edge phenomena occur as a consequence of the onset of a strong turbulence regime.…”
Section: Introductionmentioning
confidence: 90%
“…The code, which is limited to the k y = 0 case, has been described in detail elsewhere. 7 In this code, the CM geometry is a bit different than in Sec. IV because a vacuum region rather than a low density halo plasma is assumed beyond the Faraday screen.…”
Section: Diffuse Profile Calculations With Self-consistent Ponderomentioning
confidence: 99%
“…This feature and the role of ponderomotive steepening and induced reflection have been treated elsewhere. 7 The TFTR experimental observation that loading depends on poloidal (y) phasing (0-0-0-0 or 0-0-π-π) is suggestive of the notion that the CM propagates only at low k y . In this paper, we explore this dependence and the dependence of the power split P out /P rf on dissipation in the halo plasma, where P out = P rf − P halo .…”
Section: Introductionmentioning
confidence: 99%
“…This feature, was not expected from traditional direct launch IBW theory, but could be explained by a linear theory model 40 which assumed ponderomotive depletion of density in front of the antenna, and allowed the energy to be absorbed at the ensuing lower hybrid resonance (LHR). A related 1-D nonlinear model, 41 which explicitly included ponderomotive profile steepening, showed enhanced wave reflection near the LHR that effectively channeled energy into a coaxial mode propagating in the halo plasma. Furthermore, the phasing properties of this mode were consistent with loading and heating efficiency measurements on TFTR.…”
Section: Ibw Edge Interactionsmentioning
confidence: 99%