2013
DOI: 10.1088/0029-5515/54/1/013008
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Compressible impurity flow in the TJ-II stellarator

Abstract: Abstract. Fully-ionised carbon impurity flow is studied in ion-root, neutral beam heated plasmas by means of Charge Exchange Recombination Spectroscopy (CXRS) in the TJ-II stellarator. Perpendicular flows are found to be in reasonable agreement with neoclassical calculations of the radial electric field. The parallel flow of the impurity is obtained at two locations of the same flux surface after subtraction of the calculated Pfirsch-Schlüter parallel velocity. For the medium density plasmas studied,ne ∈ (1.2−… Show more

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Cited by 15 publications
(29 citation statements)
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“…In that reference the asymmetry of the impurity density was assessed by comparing the inboard and outboard parallel velocities of C 6+ . Whereas the model was not able to explain the sign of the measured flow variation, the predicted density asymmetry is qualitatively consistent with the 2D emissivity pattern shown here (see figures 5 and 6 and figure 7 in reference [20]). …”
Section: Summary and Discussionsupporting
confidence: 83%
“…In that reference the asymmetry of the impurity density was assessed by comparing the inboard and outboard parallel velocities of C 6+ . Whereas the model was not able to explain the sign of the measured flow variation, the predicted density asymmetry is qualitatively consistent with the 2D emissivity pattern shown here (see figures 5 and 6 and figure 7 in reference [20]). …”
Section: Summary and Discussionsupporting
confidence: 83%
“…At higher densities, systematic variations of flow were observed within a magnetic surface (figure 2), which are interpreted as being due to particle number conservation in the presence of impurity density variations along the surface. Modelling based on the above-mentioned mechanisms (see [9] and references therein) resulted in density variations of 20-30% for these higher density NBI plasmas, and return parallel flows of the correct size (∼5 km s −1 ). However, the calculated flow correction had the opposite sign of the observations.…”
Section: Particle Energy and Impurity Transportmentioning
confidence: 95%
“…It is well-known (Galeev & Sagdeev 1979;Ho & Kulsrud 1987) that, for sufficiently low ion collisionality, tangential drifts have to be kept in the stellarator drift-kinetic equation. If the radial electric field is not small and the aspect ratio is large, one can show that the drift-kinetic equation is radially local and that the tangential magnetic drift † As a matter of fact, this has brought up the relevance of the measurement ofφ (Pedrosa et al 2015) and its impact on impurity density inhomogeneities (Arévalo et al 2014;Alonso et al 2016).…”
Section: Introductionmentioning
confidence: 99%