2017
DOI: 10.1051/epjconf/201715703066
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Plasma edge modelling with ICRF coupling

Abstract: Abstract. The physics of Radio-Frequency (RF) wave heating in the Ion Cyclotron Range of Frequencies (ICRF) in the core plasmas of fusion devices are relatively well understood while those in the Scrape-Off Layer (SOL) remain still unresolved. This paper is dedicated to study the ICRF interactions with the plasma edge, mainly from the theoretical and numerical point of view, in particular with the 3D edge plasma fluid and neutral transport code EMC3-EIRENE and various wave codes. Here emphasis is given to the … Show more

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Cited by 4 publications
(3 citation statements)
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“…The simulation results are in qualitative agreement with the experimental ones, as shown in figure 6. As pointed out in references [35,145], the results indicate that convective cells are developed where high potential blobs exist. The E × B drifts near the center of convective cells are usually highest (on the order of 1 km s −1 ), and the drifts near the boundary of convective cells can go from one convective cell to the other.…”
Section: Icrf-induced Convectionsupporting
confidence: 55%
“…The simulation results are in qualitative agreement with the experimental ones, as shown in figure 6. As pointed out in references [35,145], the results indicate that convective cells are developed where high potential blobs exist. The E × B drifts near the center of convective cells are usually highest (on the order of 1 km s −1 ), and the drifts near the boundary of convective cells can go from one convective cell to the other.…”
Section: Icrf-induced Convectionsupporting
confidence: 55%
“…Theoretical approaches [24][25][26] to model sheaths are being developed and will be validated against measurements on ASDEX Upgrade [11,27] and on IShTAR [28,29]. Theoretical insight of experimental results will provide key guidelines to design antennas with reduced sheaths and RF-induced impurities.…”
Section: Discussionmentioning
confidence: 99%
“…In a steady state, the ionized particles (ions and electrons) leave this ionization zone mainly via convection along the field lines. The associated convective energy flux and the power losses into the ionization processes provide an energy sink to the background plasma and thereby lower the plasma temperatures in the ionization region due to the finite classical heat conductivity, resulting in a local density rise as a consequence of the parallel pressure conservation [31]. Figure 8.…”
Section: Power Flux To the Main Chamber Wallmentioning
confidence: 99%