TY - JOUR
T1 - Plasma impurities observed by a pulse height analysis diagnostic during the divertor campaign of the Wendelstein 7-X stellarator
AU - W7-X Team
AU - Kubkowska, M.
AU - Czarnecka, A.
AU - Fornal, T.
AU - Gruca, M.
AU - Jabłoński, S.
AU - Krawczyk, N.
AU - Ryć, L.
AU - Burhenn, R.
AU - Buttenschön, B.
AU - Geiger, B.
AU - Grulke, O.
AU - Langenberg, A.
AU - Marchuk, O.
AU - McCarthy, K. J.
AU - Neuner, U.
AU - Nicolai, D.
AU - Pablant, N.
AU - Schweer, B.
AU - Thomsen, H.
AU - Wegner, Th
AU - Drews, P.
AU - Hollfeld, K. P.
AU - Killer, C.
AU - Krings, Th
AU - Offermanns, G.
AU - Satheeswaran, G.
AU - Kunkel, F.
N1 - Publisher Copyright:
© 2018 EURATOM.
PY - 2018/10/1
Y1 - 2018/10/1
N2 - The paper reports on the optimization process of the soft X-ray pulse height analyzer installed on the Wendelstein 7-X (W7-X) stellarator. It is a 3-channel system that records X-ray spectra in the range from 0.6 to 19.6 keV. X-ray spectra, with a temporal and spatial resolution of 100 ms and 2.5 cm (depending on selected slit sizes), respectively, are line integrated along a line-of-sight that crosses near to the plasma center. In the second W7-X operation phase with a carbon test divertor unit, light impurities, e.g., carbon and oxygen, were observed as well as mid- to high-Z elements, e.g., sulfur, chlorine, chromium, manganese, iron, and nickel. In addition, X-ray lines from several tracer elements have been observed after the laser blow-off injection of different impurities, e.g., silicon, titanium, and iron, and during discharges with prefill or a gas puff of neon or argon. These measurements were achieved by optimizing light absorber-foil selection, which defines the detected energy range, and remotely controlled pinhole size, which defines photon flux. The identification of X-ray lines was confirmed by other spectroscopic diagnostics, e.g., by the High-Efficiency XUV Overview Spectrometer, HEXOS, and high-resolution X-ray imaging spectrometer, HR-XIS.
AB - The paper reports on the optimization process of the soft X-ray pulse height analyzer installed on the Wendelstein 7-X (W7-X) stellarator. It is a 3-channel system that records X-ray spectra in the range from 0.6 to 19.6 keV. X-ray spectra, with a temporal and spatial resolution of 100 ms and 2.5 cm (depending on selected slit sizes), respectively, are line integrated along a line-of-sight that crosses near to the plasma center. In the second W7-X operation phase with a carbon test divertor unit, light impurities, e.g., carbon and oxygen, were observed as well as mid- to high-Z elements, e.g., sulfur, chlorine, chromium, manganese, iron, and nickel. In addition, X-ray lines from several tracer elements have been observed after the laser blow-off injection of different impurities, e.g., silicon, titanium, and iron, and during discharges with prefill or a gas puff of neon or argon. These measurements were achieved by optimizing light absorber-foil selection, which defines the detected energy range, and remotely controlled pinhole size, which defines photon flux. The identification of X-ray lines was confirmed by other spectroscopic diagnostics, e.g., by the High-Efficiency XUV Overview Spectrometer, HEXOS, and high-resolution X-ray imaging spectrometer, HR-XIS.
UR - https://www.scopus.com/pages/publications/85054320126
UR - https://www.scopus.com/inward/citedby.url?scp=85054320126&partnerID=8YFLogxK
U2 - 10.1063/1.5038850
DO - 10.1063/1.5038850
M3 - Review article
C2 - 30399723
AN - SCOPUS:85054320126
SN - 0034-6748
VL - 89
JO - Review of Scientific Instruments
JF - Review of Scientific Instruments
IS - 10
M1 - 10F111
ER -