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100 1 _ |a Mertens, Philippe
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245 _ _ |a On the use of rhodium mirrors for optical diagnostics in ITER
260 _ _ |a New York, NY [u.a.]
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520 _ _ |a The first mirrors of optical diagnostics in ITER are exposed to high radiation and fluxes of particles which escape the plasma, in the order of $10^{20} m^{−2}s^{−1}$. At the position of the mirror, the flux may still reach about $10^{18} m^{−2}s^{−1}$. First mirrors are thus the most vulnerable in-vessel optical components, being subject to erosion, esp. by fast charge-exchange neutrals, or to deposition of impurities at flux rates which can reach 0.05 nm/s. The material selected for the reflecting surface must combine a high optical reflectivity in a wide spectral range and a sufficient resistance to physical sputtering during normal operation and during mirror cleaning discharges, if any is installed. Rhodium ($^{103}Rh$) was identified early as a possible or even promising candidate. It combines several attractive properties, for instance a mass which leads in most cases to low sputtering yields together with an optical reflectance ($\mathscr{R}_{Rh}≈75\%$) which is much higher than of some other options. $\mathscr{R}_{Rh}$is insensitive to large temperature changes. Rhodium is fairly inert and its low oxidation is an appreciable advantage in case of steam ingress events.The core-plasma CXRS diagnostic in ITER (UPP 3) have now turned to Rh as a baseline. The aim is to procure monocrystalline rhodium (SC-Rh) to mitigate the increase of the diffuse reflection with the damage due to physical sputtering.
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700 1 _ |a Boman, Romain
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700 1 _ |a Dickheuer, Sven
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700 1 _ |a Krasikov, Yury
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700 1 _ |a Krimmer, Andreas
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700 1 _ |a Leichtle, Dieter
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700 1 _ |a Liegeois, Kim
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700 1 _ |a Linsmeier, Christian
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700 1 _ |a Litnovsky, Andrey
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700 1 _ |a Marchuk, Oleksander
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700 1 _ |a Rasinski, Marcin
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700 1 _ |a De Bock, Maarten
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856 4 _ |u https://juser.fz-juelich.de/record/862421/files/W1503625.pdf
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