S Vives, C Guillon, L Letellier, M H Aumeunier, X Courtois, S Garitta, J Grosy, N Lapcevic, N Lefevre, B Peluso, Y Peneliau, M Medrano, C Pastor, F Mota, V Martin, J Poissy, G Jouffroy, R Lopez Heredero, L M Gonzalez-Fernandez, M Fernandez-Rodríguez, R Garcia-Lopez, M J Zamora, T Belenguer, F Le Guern, J Piqueras, M Fabbri, P Testoni
{"title":"Design, justification, and prototyping of the visible and infrared wide angle viewing system diagnostic for ITER equatorial port 12.","authors":"S Vives, C Guillon, L Letellier, M H Aumeunier, X Courtois, S Garitta, J Grosy, N Lapcevic, N Lefevre, B Peluso, Y Peneliau, M Medrano, C Pastor, F Mota, V Martin, J Poissy, G Jouffroy, R Lopez Heredero, L M Gonzalez-Fernandez, M Fernandez-Rodríguez, R Garcia-Lopez, M J Zamora, T Belenguer, F Le Guern, J Piqueras, M Fabbri, P Testoni","doi":"10.1063/5.0234380","DOIUrl":null,"url":null,"abstract":"<p><p>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.</p>","PeriodicalId":21111,"journal":{"name":"Review of Scientific Instruments","volume":null,"pages":null},"PeriodicalIF":1.3000,"publicationDate":"2024-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Review of Scientific Instruments","FirstCategoryId":"5","ListUrlMain":"https://doi.org/10.1063/5.0234380","RegionNum":4,"RegionCategory":"工程技术","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"INSTRUMENTS & INSTRUMENTATION","Score":null,"Total":0}
引用次数: 0
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.
期刊介绍:
Review of Scientific Instruments, is committed to the publication of advances in scientific instruments, apparatuses, and techniques. RSI seeks to meet the needs of engineers and scientists in physics, chemistry, and the life sciences.