000282884 001__ 282884 000282884 005__ 20240711113858.0 000282884 0247_ $$2doi$$a10.1088/0029-5515/56/2/026014 000282884 0247_ $$2ISSN$$a0029-5515 000282884 0247_ $$2ISSN$$a1741-4326 000282884 0247_ $$2WOS$$aWOS:000372332500006 000282884 037__ $$aFZJ-2016-01631 000282884 082__ $$a530 000282884 1001_ $$0P:(DE-HGF)0$$aDen Harder, N.$$b0 000282884 245__ $$aELM-resolved divertor erosion in the JET ITER-Like Wall 000282884 260__ $$aVienna$$bIAEA$$c2016 000282884 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1455541174_27521 000282884 3367_ $$2DataCite$$aOutput Types/Journal article 000282884 3367_ $$00$$2EndNote$$aJournal Article 000282884 3367_ $$2BibTeX$$aARTICLE 000282884 3367_ $$2ORCID$$aJOURNAL_ARTICLE 000282884 3367_ $$2DRIVER$$aarticle 000282884 520__ $$aTungsten erosion in H-mode plasmas is quantified in the outer divertor of the JET ITER-Like Wall environment with optical emission spectroscopy on the 400.9 nm atomic neutral tungsten line. A novel cross-calibration procedure is developed to link slow, high spectral resolution spectroscopy and fast photomultiplier tube measurements in order to obtain ELM-resolved photon fluxes. Inter-ELM W erosion is exclusively impurity sputtering by beryllium because of the high sputter threshold for deuterons. Low beryllium concentrations resulted in low inter-ELM sputter yields of around 10−4 with respect to the total flux.Intra-ELM W sources, which dominate the total W tungsten source, vary independently from the inter-ELM source. The amount of W erosion could only be partly explained by beryllium sputtering, indicating that during ELMs sputtering by fuel species is important. The total W outer divertor source is found to linearly increase with the power crossing the separatrix, whilst excessive divertor fueling can break this trend.The influence of the W source rate on the tungsten content of the core plasma is investigated using soft x-ray emission to determine the tungsten content. At low source rates the content is determined by the source, but at higher source rates, other phenomena determine the total tungsten content. Indications of impurity flushing by ELMs is seen at ELM frequencies above approximately 40 Hz. The inner/outer divertor asymmetry of the W source during ELMs is investigated, and the outer divertor W source is larger by a factor of $1.8\pm 0.7$ . 000282884 536__ $$0G:(DE-HGF)POF3-174$$a174 - Plasma-Wall-Interaction (POF3-174)$$cPOF3-174$$fPOF III$$x0 000282884 588__ $$aDataset connected to CrossRef 000282884 7001_ $$0P:(DE-Juel1)129976$$aBrezinsek, S.$$b1$$eCorresponding author$$ufzj 000282884 7001_ $$0P:(DE-HGF)0$$aPütterich, T.$$b2 000282884 7001_ $$0P:(DE-HGF)0$$aFedorczak, N.$$b3 000282884 7001_ $$0P:(DE-HGF)0$$aMatthews, G. F.$$b4 000282884 7001_ $$0P:(DE-HGF)0$$aMeigs, A.$$b5 000282884 7001_ $$0P:(DE-HGF)0$$aStamp, M. F.$$b6 000282884 7001_ $$0P:(DE-HGF)0$$avan de Sanden, M. C. M.$$b7 000282884 7001_ $$0P:(DE-HGF)0$$aVan Rooij, G. J.$$b8 000282884 773__ $$0PERI:(DE-600)2037980-8$$a10.1088/0029-5515/56/2/026014$$gVol. 56, no. 2, p. 026014 -$$n2$$p026014 -$$tNuclear fusion$$v56$$x1741-4326$$y2016 000282884 8564_ $$uhttps://juser.fz-juelich.de/record/282884/files/pdf-1.pdf$$yRestricted 000282884 8564_ $$uhttps://juser.fz-juelich.de/record/282884/files/pdf-1.pdf?subformat=pdfa$$xpdfa$$yRestricted 000282884 909CO $$ooai:juser.fz-juelich.de:282884$$pVDB 000282884 9101_ $$0I:(DE-588b)5008462-8$$6P:(DE-Juel1)129976$$aForschungszentrum Jülich GmbH$$b1$$kFZJ 000282884 9131_ $$0G:(DE-HGF)POF3-174$$1G:(DE-HGF)POF3-170$$2G:(DE-HGF)POF3-100$$3G:(DE-HGF)POF3$$4G:(DE-HGF)POF$$aDE-HGF$$bEnergie$$lKernfusion$$vPlasma-Wall-Interaction$$x0 000282884 9141_ $$y2016 000282884 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS 000282884 915__ $$0StatID:(DE-HGF)0100$$2StatID$$aJCR$$bNUCL FUSION : 2014 000282884 915__ $$0StatID:(DE-HGF)0150$$2StatID$$aDBCoverage$$bWeb of Science Core Collection 000282884 915__ $$0StatID:(DE-HGF)0110$$2StatID$$aWoS$$bScience Citation Index 000282884 915__ $$0StatID:(DE-HGF)0111$$2StatID$$aWoS$$bScience Citation Index Expanded 000282884 915__ $$0StatID:(DE-HGF)9900$$2StatID$$aIF < 5 000282884 915__ $$0StatID:(DE-HGF)0550$$2StatID$$aNo Authors Fulltext 000282884 915__ $$0StatID:(DE-HGF)1150$$2StatID$$aDBCoverage$$bCurrent Contents - Physical, Chemical and Earth Sciences 000282884 915__ $$0StatID:(DE-HGF)0430$$2StatID$$aNational-Konsortium 000282884 915__ $$0StatID:(DE-HGF)0420$$2StatID$$aNationallizenz 000282884 915__ $$0StatID:(DE-HGF)0199$$2StatID$$aDBCoverage$$bThomson Reuters Master Journal List 000282884 9201_ $$0I:(DE-Juel1)IEK-4-20101013$$kIEK-4$$lPlasmaphysik$$x0 000282884 980__ $$ajournal 000282884 980__ $$aVDB 000282884 980__ $$aUNRESTRICTED 000282884 980__ $$aI:(DE-Juel1)IEK-4-20101013 000282884 981__ $$aI:(DE-Juel1)IFN-1-20101013