2010
DOI: 10.1088/0029-5515/50/2/025012
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Calculation and experimental test of the cooling factor of tungsten

Abstract: Abstract. The cooling factor of W is evaluated using state of the art data for line radiation and an ionization balance which has been benchmarked with experiment. For the calculation of line radiation, level-resolved calculations were performed with the Cowan code to obtain the electronic structure and excitation cross sections (plane-wave Born approximation). The data were processed by a collisional radiative model to obtain electron density dependent emissions. These data were then combined with the radiati… Show more

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Cited by 203 publications
(205 citation statements)
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“…The local impurity density can be estimated from the known relation between the SXR radiation and impurity density as is shown in Refs. 4 and 6. The spatial information about the SXR radiation is provided by several pinhole cameras surrounding the plasma.…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…The local impurity density can be estimated from the known relation between the SXR radiation and impurity density as is shown in Refs. 4 and 6. The spatial information about the SXR radiation is provided by several pinhole cameras surrounding the plasma.…”
Section: Introductionmentioning
confidence: 99%
“…The radiation losses from the partially stripped high-Z ions can be beneficial at the plasma edge because the power exhaust in the divertor is significantly reduced. However, intense radiative cooling in the plasma core leads to a deterioration of the fusion performance 4 . Moreover, unfavorable impurity transport in the plasma core may cause impurity accumulation and, consequently, a radiative collapse of the plasma 5 .…”
Section: Introductionmentioning
confidence: 99%
“…Impurities with higher Z number like Ar and Kr radiate significantly up to high temperatures and can therefore be used as main plasma radiators. Tungsten radiates strongly up to about 10 keV [13]. The local radiation power density is given by the product L z · n 2 e · c z where n e is the electron density and c z the impurity concentration.…”
Section: Theoretical Background and Modelling: Coronal And Non-coronamentioning
confidence: 99%
“…Radiation from excited tungsten ions leads to substantial plasma cooling which has to be well controlled in order to maintain the conditions for nuclear fusion. Thus, a comprehensive knowledge of atomic energy levels and collision cross sections is required for a thorough understanding of the spatial and temporal evolution of the tungsten charge states and emission spectra in fusion plasmas [174].…”
Section: Atomic Data For Fusion Energy Researchmentioning
confidence: 99%
“…TSR at HIE-ISOLDE will allow one to considerably extend the range of charge states up to about 50+ with the currently available charge breeder (REXEBIS) and possibly up to 72 + (Helike) with an upgraded charge breeder. Measurements of absolute rate coefficients for DR and, equally important, for electron-ion impact ionization will thus become possible for all the charge states of tungsten which are relevant for fusion plasma modeling [174]. The dashdotted curve is the calculated merged-beams rate coefficient for radiative recombination (RR) using a hydrogenic approximation.…”
Section: Atomic Data For Fusion Energy Researchmentioning
confidence: 99%