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The effect of surface temperature on optical properties of molybdenum mirrors in the visible and near-infrared domains

机译:表面温度对可见光和近红外域中钼镜光学性能的影响

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Molybdenum mirrors will be used in several optical diagnostics to control the plasma in the ITER tokamak. In this harsh environment, mirrors can undergo transient temperature rises. Thus, the knowledge of the temperature dependence of optical properties of molybdenum is necessary for a good operation of optical systems in ITER. Molybdenum optical properties have been extensively studied at room temperature, but little has been done at high temperatures in the visible and near-infrared domains. We investigate the temperature dependence of molybdenum reflectivity from the ambient to high temperatures (<800 K) in the 500-1050nm spectral range. Experimental measurements of reflectivity, performed via a spectroscopic system coupled with laser remote heating, show a maximum increase of 2.5% at 800 K in the 850-900 nm wavelength range and a non-linear temperature dependency as a function of wavelength. We describe these dependencies through a Fresnel and a Lorentz-Drude model. The Fresnel model accurately reproduces the experimental curve at a given temperature by using a parabolic temperature dependency for the refractive index, n, and a linear dependency for the extinction coefficient, k. We develop a Lorentz-Drude model to describe the interaction of light with charge carriers in the solid. This model includes temperature dependency on both intraband (Drude) and interband (Lorentz) transitions. It is able to reproduce the experimental results quantitatively, highlighting a non-trivial dependency of interband transitions on temperature. Eventually, we use the Lorentz-Drude model to evaluate the total emissivity of molybdenum from 300 K to 2800 K, and we compare our experimental and theoretical findings with previous results.
机译:钼镜将用于多种光学诊断中,以控制ITER托卡马克中的等离子体。在这种恶劣的环境中,镜子可能会经历短暂的温度上升。因此,对于ITER中光学系统的良好操作,必须了解钼的光学性质与温度的关系。钼的光学性质已在室温下进行了广泛研究,但在高温下在可见光和近红外域中几乎没有做过任何事情。我们研究了钼反射率在500-1050nm光谱范围内从环境温度到高温(<800 K)的温度依赖性。通过光谱系统结合激光远程加热进行的反射率实验测量表明,在850-900 nm波长范围内,在800 K下最大增加了2.5%,并且非线性温度依赖性随波长变化。我们通过菲涅耳和洛伦兹-德鲁德模型来描述这些依赖关系。菲涅耳模型通过使用抛物线温度依赖性折射率n和消光系数k线性关系来精确再现给定温度下的实验曲线。我们开发了一个Lorentz-Drude模型来描述固体中光与电荷载体的相互作用。该模型包括对带内(Drude)和带间(Lorentz)过渡的温度依赖性。它能够定量地再现实验结果,突出显示了带间跃迁对温度的非平凡依赖性。最终,我们使用Lorentz-Drude模型评估了300 K至2800 K的钼的总发射率,并将我们的实验和理论发现与先前的结果进行了比较。

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