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Polarizing and non-polarizing mirrors for the hydrogen Lyman-α radiation at 121.6 nm

机译:用于121.6 nm处的Lyman-α氢辐射的偏振镜和非偏振镜

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Efficient polarizing as well as non-polarizing mirrors for a wavelength of λ=121.6 nm (hydrogen Lyman-α radiation) are necessary to achieve an experimental determination of the magnetic field in the solar corona through the Hanle effect. We have designed, realized and characterized such mirrors. These consist of glass coated with a thin-film stack. The coatings use the most reflective (Al) and most transparent (fluorides) materials at this wavelength. Different coatings were explored which involve an increasing number of films in the coating stack. At the incident angle of maximum polarization where the p-polarized reflectivity R p is minimized, an s-polarized reflectivity R s as high as 69% is experimentally obtained with a coating made of a Fabry–Pérot resonator. To our knowledge, this value is the highest ever reported for a polarizing mirror at this wavelength. Additionally, efficient non-polarizing mirrors have been designed and realized by using a two-layer coating (MgF2/Al/glass). By optimizing the fluoride layer thickness, a mirror with non-polarizing properties in the whole range of incident angles was realized.
机译:为了通过Hanle效应对太阳日冕中的磁场进行实验确定,必须使用有效波长为λ= 121.6 nm的偏振镜和非偏振镜(氢Lyman-α辐射)。我们已经设计,实现并表征了此类镜子。这些由涂有薄膜叠层的玻璃组成。涂层在该波长下使用最具反射性的(Al)和最透明的(氟化物)材料。探索了不同的涂层,这些涂层涉及涂层堆叠中越来越多的膜。在最大偏振的入射角处,p偏振反射率R p 最小,通过镀膜实验获得了高达69%的s偏振反射率R s 由Fabry-Pérot谐振器制成。据我们所知,该值是该波长下偏振镜报道的最高值。此外,通过使用两层涂层(MgF 2 / Al /玻璃)设计并实现了有效的非偏振镜。通过优化氟化物层的厚度,实现了在整个入射角范围内具有非偏振特性的镜子。

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