2017
DOI: 10.1088/1741-4326/aa66b2
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The inter-ELM tungsten erosion profile in DIII-D H-mode discharges and benchmarking with ERO+OEDGE modeling

Abstract: It is important to develop a predictive capability for the tungsten source rate near the strike points during H-mode operation in ITER and beyond. H-mode deuterium plasma exposures were performed on W-coated graphite and molybdenum substrates in the DIII-D divertor using DiMES. The W-I 400.9 nm spectral line was monitored by fast filtered diagnostics cross calibrated via a high-resolution spectrometer to resolve inter-ELM W erosion. The effective ionization/photon (S/XB) was calibrated using a unique method de… Show more

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Cited by 50 publications
(49 citation statements)
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“…The fraction of Be ions was kept constant in this study whereas it might rise in addition during T plasma operation due to higher sputtering of Be from the main wall due to charge-exchange neutrals [9]. Please note, that the observations in D plasmas are consistent with recent studies in DIII-D [23] where the main impurity (carbon) fraction in the flux to the target plate dominates the W sputtering in the intra-ELM phase over the impinging deuterons.…”
Section: Physical Sputtering Of Tungstensupporting
confidence: 78%
“…The fraction of Be ions was kept constant in this study whereas it might rise in addition during T plasma operation due to higher sputtering of Be from the main wall due to charge-exchange neutrals [9]. Please note, that the observations in D plasmas are consistent with recent studies in DIII-D [23] where the main impurity (carbon) fraction in the flux to the target plate dominates the W sputtering in the intra-ELM phase over the impinging deuterons.…”
Section: Physical Sputtering Of Tungstensupporting
confidence: 78%
“…Tungsten emission lines are among the least intense impurity UV lines present in measured DIII-D spectra, consistent with the low sputtering yield of tungsten [28]; yet, Tungsten emission is more intense compared to the background spectra in the CTH experiment than in DIII-D. Measured tungsten spectral lines in CTH are stronger, due to the greater solid angle of W emission as viewed by the CTH collection optics.…”
Section: Resultssupporting
confidence: 62%
“…The camera was operated in fast line-scan mode with framing rate up to 12 kHz thus able to capture heat flux evolution during ELMs. The inserts near DiMES were imaged with a WI-filtered (400.9 nm) DiMES-TV camera with framing rate 100 Hz and exposure time 10 ms. [13]. Filtered photo multipliers (filterscopes) with sampling rate 5×10 5 Hz have been installed to monitor each of the W rings (two nearby chords with ∅2 cm per ring) and provide background subtracted photon fluxes of neutral W line at 400.9 nm using a recently implemented technique [14].…”
Section: Introductionmentioning
confidence: 99%