This title appears in the Scientific Report :
2018
Please use the identifier:
http://dx.doi.org/10.1088/1402-4896/aa8a45 in citations.
Spectroscopic determination of inverse photon efficiencies of W atoms in the scrape-off layer of TEXTOR
Spectroscopic determination of inverse photon efficiencies of W atoms in the scrape-off layer of TEXTOR
Optical emission spectroscopy can be applied to determine in situ tungsten particle fluxes from erosion processes at plasma-facing materials. Inverse photon efficiencies convert photon fluxes of WI and WII line transitions into W and ${{\rm{W}}}^{+}$ particle fluxes, respectively, dependening on the...
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Personal Name(s): | Brezinsek, S. (Corresponding author) |
---|---|
Laengner, M. / Coenen, J. W. / O’Mullane, M. G. / Pospieszczyk, A. / Sergienko, G. / Samm, U. | |
Contributing Institute: |
Plasmaphysik; IEK-4 |
Published in: | Physica scripta, T170 (2017) S. 014052 - |
Imprint: |
Bristol
IoP Publ.
2017
|
DOI: |
10.1088/1402-4896/aa8a45 |
Document Type: |
Journal Article |
Research Program: |
Plasma-Wall-Interaction |
Publikationsportal JuSER |
Optical emission spectroscopy can be applied to determine in situ tungsten particle fluxes from erosion processes at plasma-facing materials. Inverse photon efficiencies convert photon fluxes of WI and WII line transitions into W and ${{\rm{W}}}^{+}$ particle fluxes, respectively, dependening on the local plasma conditions. Experiments in TEXTOR were carried out to determine effective conversion factors for different WI and WII transitions with the aid of WF6 injection into deuterium scrape-off layer plasmas in the electron temperature T e range between ${T}_{{e}}=20\,\mathrm{eV}$ and ${T}_{{e}}=82\,\mathrm{eV}$. The inverse photon efficiencies or so-called effective $\tfrac{S}{{XB}}$-values have been determined for WI lines at $\lambda =400.9\,\mathrm{nm}$, 429.5 nm, 488.7 nm, 498.3 nm, and 522.5 nm as well as for WII at $\lambda =434.6\,\mathrm{nm}$ and compared with theoretical calculations from the ADAS data base. Moreover, a multi-machine scaling for the $\tfrac{S}{{XB}}$-value in the range of T e between $2...100\,\mathrm{eV}$ has been determined for the most prominent WI line at $\lambda =400.9\,\mathrm{nm}$ to $\tfrac{S}{{XB}}({T}_{{e}})=53.63-56.07\times {e}^{(0.045\times {T}_{{e}}[\mathrm{eV}])}$ considering experimental data from TEXTOR, ASDEX Upgrade, PSI and PISCES. Comparison with ADAS calculations for the same transition reveal a good qualitative agreement with the dependence on T e , but an underestimation of ADAS calculations of less than 25% over the full covered range of experimentally accessible T e in the multi-machine scaling. A good agreement within the experimental uncertainties is found between TEXTOR and ADAS $\tfrac{S}{{XB}}$-values for WI at $\lambda =429.5\,\mathrm{nm}$ and $\lambda =488.7\,\mathrm{nm}$ whereas an underestimation of up to a factor two of ADAS values for WI at $\lambda =522.5\,\mathrm{nm}$ and $\lambda =498.3\,\mathrm{nm}$ was measured. Potentially, reasons for the discrepancy are an overestimation of applied ionisation rate coefficients in ADAS for neutral W and a stronger electron dependence n e for these transitions. |