2016
DOI: 10.1016/j.fusengdes.2016.02.025
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Design of the ITER VUV edge imaging spectrometer and R&D for the rotary motional vacuum feed-through

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Cited by 9 publications
(8 citation statements)
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“…Whereas radiation induced luminescence mainly affects those diagnostics with very weak signals, radiation induced attenuation affects all diagnostics using refractive optics and optical fibres. Even for radiation hardened optical fibres an attenuation of several dB/m can be expected at the end of ITER life in the interspace [13] (see figure 5). Measures such as providing extra shielding around optical fibres, providing heating for annealing the radiation damage and foreseeing the possibility of periodic replacement of the fibres in the interspace are to be taken into account in the design of spectroscopy diagnostics that plan on using optical fibres.…”
Section: Effects Of Radiation On Optical and Electronic Componentsmentioning
confidence: 99%
“…Whereas radiation induced luminescence mainly affects those diagnostics with very weak signals, radiation induced attenuation affects all diagnostics using refractive optics and optical fibres. Even for radiation hardened optical fibres an attenuation of several dB/m can be expected at the end of ITER life in the interspace [13] (see figure 5). Measures such as providing extra shielding around optical fibres, providing heating for annealing the radiation damage and foreseeing the possibility of periodic replacement of the fibres in the interspace are to be taken into account in the design of spectroscopy diagnostics that plan on using optical fibres.…”
Section: Effects Of Radiation On Optical and Electronic Componentsmentioning
confidence: 99%
“…In KSTAR, several imaging diagnostics with tomographic reconstruction algorithms have been developed for impurity transport study [8][9][10][11], including the tungsten powder injection experiment. However, both the vacuum (VUV) and extreme ultraviolet (EUV) spectrometers [10,12] on KSTAR and the one planned for ITER [13], which have a capability of resolving the spatial distribution of line emissions, suffer from a limited viewing angle due to the narrow allocated space, which makes it difficult to accurately reconstruct the local emissivity profile of each line radiation from the chordintegrated data. The ITER VUV spectrometers are expected to employ 5 channels having different fields of view (FoVs) with different wavelengths [12][13][14].…”
Section: Local Profiles Of Line Emission Of Impurity Ions In Rotating...mentioning
confidence: 99%
“…However, both the vacuum (VUV) and extreme ultraviolet (EUV) spectrometers [10,12] on KSTAR and the one planned for ITER [13], which have a capability of resolving the spatial distribution of line emissions, suffer from a limited viewing angle due to the narrow allocated space, which makes it difficult to accurately reconstruct the local emissivity profile of each line radiation from the chordintegrated data. The ITER VUV spectrometers are expected to employ 5 channels having different fields of view (FoVs) with different wavelengths [12][13][14]. Therefore, inadequate lines of sight (LoSs) may lead to the inaccurate local profiles by using the conventional tomographic methods.…”
Section: Local Profiles Of Line Emission Of Impurity Ions In Rotating...mentioning
confidence: 99%
“…The VUV edge imaging spectrometer in upper port #18 consists of one field mirror with cylindrical geometry, one collimating mirror with ellipsoidal geometry, and a VUV imaging spectrometer. 12 The equatorial system in equatorial port #11 employs a VUV survey spectrometer with five channels for wideband coverage and having high spectral and time resolution. The divertor VUV spectrometer is also located at equatorial port #11 with relay optics consisting of a field mirror and a collimating mirror.…”
Section: Iter Vuv Core Survey Spectrometermentioning
confidence: 99%