钨的光学性质:表征粗糙度、表面成分和温度作用的参数化研究

3区 物理与天体物理 Q1 Materials Science
Federica Pappalardo, Francisco Romero Romero Lairado, C. L. D. Louis de Canonville, C. Martin, G. Giacometti, Guillaume Serin, E. Salomon, T. Angot, L. Gallais, R. Bisson, M. Minissale
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引用次数: 0

摘要

钨(W)是国际核聚变实验ITER引流器排气选用的材料。在这种恶劣的环境下,热载荷和离子通量与W的相互作用会导致光学性质的暂时或永久演变。在等离子体操作过程中,对这种演变的不了解可能导致光学诊断进行温度测量时出现错误。因此,表征W光学性质可能发生的变化是至关重要的。在这项工作中,我们研究了形貌和温度对W光学响应的影响。在激光退火(25-800℃)期间,测量了5种不同粗糙度值(20-100 nm)的W样品在可见光和近红外域(500-1100 nm)的反射率。我们观察到退火后反射率的增加,我们证明这是由于表面化学成分的变化,特别是天然氧化物的减少。此外,我们表明粗糙度在所研究的温度范围内没有明显变化。通过强调粗糙度和表面杂质(例如氧化物)所起的作用,我们提供了W光学性质如何在托卡马克中演变的见解,在托卡马克中,高离子通量、热负荷和杂质可以诱导W的形态和表面组成的演变。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Optical Properties of Tungsten: A Parametric Study to Characterize the Role of Roughness, Surface Composition and Temperature
Tungsten (W) is the material selected for the divertor exhaust of the international nuclear fusion experiment ITER. In this harsh environment, the interactions of heat loads and ion fluxes with W can induce temporary or permanent evolution in the optical properties. Poor knowledge of such evolution during a plasma operation can lead to errors in temperature measurements performed by optical diagnostics. Therefore, it is of fundamental importance to characterize possible changes in W optical properties. In this work, we studied the role of morphology and temperature on the optical response of W. The reflectivities of five W samples with different roughness values (20–100 nm) were measured during laser annealing (25–800 °C) in the visible and near-infrared domains (500–1100 nm). We observed an increase in reflectivity after annealing and we demonstrated that it was due to a change in the chemical composition of the surface, in particular a reduction in the amount of native oxide. Moreover, we show that roughness does not sensibly vary in the investigated temperature range. By highlighting the role played by roughness and surface impurities (e.g., oxide), we provide insight in how W optical properties can evolve in tokamaks where high ion fluxes, heat loads, and impurities can induce the evolution of both the morphology and surface composition of W.
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来源期刊
Progress in Optics
Progress in Optics 物理-光学
CiteScore
4.50
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0.00%
发文量
8
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