1987
DOI: 10.1063/1.866146
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The anomalous Doppler instability during lower-hybrid current drive

Abstract: The anomalous Doppler instability is investigated for two-dimensional velocity distributions f(v∥,v⊥) appropriate for lower-hybrid current drive. In this case, in contrast to the runaway electron problem, this mode becomes unstable at high density when the ratio ω2pe/ ω2ce is sufficiently large. Increasing the maximum velocity v2 of the rf (radio-frequency) plateau, v1≤v∥ ≤v2, is also a destabilizing influence. In this paper expressions are given for the growth rate of the electrostatic waves obeying the dispe… Show more

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Cited by 15 publications
(10 citation statements)
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“…The low-density discharge regime is characterized by a large energetic-electron population. When the ratio of the electron plasma frequency to electron cyclotron frequency ω pe /ω ce < 0.3, according to the empirical values in a number of devices, an anomalous Doppler instability (ADI) can be excited [21][22][23][24]. For discharge #10580 with toroidal field B t = 1.3 T, the ADI is excited when the density is less than the critical density n ec ≈ 0.14 × 10 19 m −3 .…”
Section: Baes Excited By Energetic Electronsmentioning
confidence: 99%
“…The low-density discharge regime is characterized by a large energetic-electron population. When the ratio of the electron plasma frequency to electron cyclotron frequency ω pe /ω ce < 0.3, according to the empirical values in a number of devices, an anomalous Doppler instability (ADI) can be excited [21][22][23][24]. For discharge #10580 with toroidal field B t = 1.3 T, the ADI is excited when the density is less than the critical density n ec ≈ 0.14 × 10 19 m −3 .…”
Section: Baes Excited By Energetic Electronsmentioning
confidence: 99%
“…pe =! ce < 0:3 according to the empirical values in several machines, the anomalous Doppler instability (ADI) can be excited [16][17][18][19]. For no.…”
mentioning
confidence: 99%
“…Many studies report observational signatures of this plateau-like electron distribution in Alcator tokamak 3,4 as well as use it extensively to explain radiation patterns and heating observed in experiments. 5,6 The agreement between the predicted and measured profiles is usually good, but on the other hand, even some recent works report discrepancies between the measured and simulated hard x-ray spectra that may be explained by neglected or underestimated electron diffusion physics. 4 In the type III radio burst problem, the solar burst electrons are accelerated and eventually the-bump-on-tail distribution is formed on the electron distribution function.…”
Section: Introductionmentioning
confidence: 95%
“…8 and 9 that the electron distribution with a tail of energetic electrons that have a plateau-like or even decreasing power-like distribution function is unstable with respect to excitation of waves at anomalous Doppler resonance (ADR). 6 x ð2Þ k À k ð2Þ z v z þ x ce ¼ 0; where x ð2Þ k and k ð2Þ z are the frequency and parallel wave number for excited waves. This is so-called fan instability that is an effective mechanism of pitch angle diffusion of the tail electrons.…”
Section: Introductionmentioning
confidence: 99%