2014
DOI: 10.1063/1.4864603
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ECRH microwave beam broadening in the edge turbulent plasma

Abstract: The influence of turbulent plasma density fluctuations on angular and spatial beam width is treated analytically in the framework of WKB based eikonal method. Reasonable agreement of analytical and numerical treatment results is demonstrated within the domain of quasi-optical approximation validity. Significant broadening of microwave beams is predicted for future ECRH experiments at ITER.

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Cited by 3 publications
(22 citation statements)
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“…Other points have also to be considered in the time-dependent cases, where Maxwell's equation solvers are coupled with J-solvers, the numerical stability and the energy conservation. The both points become problems in the large number of iterations, although they are still below what is required for ITER (da Silva et al 2015). This kind of numerical problems disappears when the time-dependent part is removed under the following assumptions: the launch wave is con-sidered as monochromatic (continuous emission at the same frequency) and the plasma parameters present time-scale evolution much larger than the time of flight of the heating wave.…”
Section: Introductionmentioning
confidence: 99%
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“…Other points have also to be considered in the time-dependent cases, where Maxwell's equation solvers are coupled with J-solvers, the numerical stability and the energy conservation. The both points become problems in the large number of iterations, although they are still below what is required for ITER (da Silva et al 2015). This kind of numerical problems disappears when the time-dependent part is removed under the following assumptions: the launch wave is con-sidered as monochromatic (continuous emission at the same frequency) and the plasma parameters present time-scale evolution much larger than the time of flight of the heating wave.…”
Section: Introductionmentioning
confidence: 99%
“…There are numerical stability problems due to the anisotropy introduced by the external DC magnetic field . One is connected to the very high difference between responses parallel to the magnetic field and those perpendicular to the magnetic field, and another relates to the accumulation of round-off error on the long computation time (more than 10 6 time steps) that drives numerical instabilities as shown in (da Silva et al 2015). On such long runs, the energy conservation should be fulfilled to preserve the statistical properties of the physical system.…”
Section: Heating Simulationmentioning
confidence: 99%
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