Design, justification, and prototyping of the visible and infrared wide angle viewing system diagnostic for ITER equatorial port 12

The ITER equatorial visible and infrared Wide Angle Viewing System (WAVS) will play a major role in the protection of plasma facing components by providing surface temperature measurements of these components. It will also image the plasma emission in the visible range. The WAVS is composed of 15 lines of sight located in four Equatorial Ports (EPs) 3, 9, 12, and 17. Its development is being carried out by the Consortium constituted by CEA, CIEMAT, INTA, and Bertin Technologies, within grant contracts financed by F4E. In the EP12, the in-vessel and ex-vessel components of the WAVS are at their final design phase. This article presents an overview of the opto-mechanical design of the WAVS in the EP12 presented at the final design review.

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Publication Details

Journal
Review of Scientific Instruments
Published
2024-11-01
DOI
https://doi.org/10.1063/5.0234380
Citations
3
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
0.99

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article

Design, justification, and prototyping of the visible and infrared wide angle viewing system diagnostic for ITER equatorial port 12

M. Medrano, J. Piqueras, S. Garitta, M.-H. Aumeunier et al.
3 citations
Review of Scientific Instruments
Ionosphere and magnetosphere dynamics
0.99
article

Design, justification, and prototyping of the visible and infrared wide angle viewing system diagnostic for ITER equatorial port 12

M. Medrano, J. Piqueras, S. Garitta, M.-H. Aumeunier, J. Grosy, Rebeca García-López, Nicolas Lefèvre, M. Fernández-Rodrı́guez, Y. Pénéliau, Marco Fabbri, Magdalena Zamora, X. Courtois, P. Testoni, C. Pastor, Vincent Martin, N. Lapcevic, F. Le Guern, J. Poissy, L. Letellier, R. L. Heredero, F. Mota, Bertrand Peluso, C. Guillon, Luís González, T. Belenguer, S. Vivès, G. Jouffroy
article en
3 citations

Abstract

The ITER equatorial visible and infrared Wide Angle Viewing System (WAVS) will play a major role in the protection of plasma facing components by providing surface temperature measurements of these components. It will also image the plasma emission in the visible range. The WAVS is composed of 15 lines of sight located in four Equatorial Ports (EPs) 3, 9, 12, and 17. Its development is being carried out by the Consortium constituted by CEA, CIEMAT, INTA, and Bertin Technologies, within grant contracts financed by F4E. In the EP12, the in-vessel and ex-vessel components of the WAVS are at their final design phase. This article presents an overview of the opto-mechanical design of the WAVS in the EP12 presented at the final design review.

Review of Scientific InstrumentsVol. 95(11)
CEA Cadarache (FR), Instituto Nacional de Técnica Aeroespacial (ES), Fusion for Energy (ES)
Fusion for Energy
Openalex Percentile: Top 23%
Ionosphere and magnetosphere dynamics
0.99
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