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Designing ultra-narrowband interference filters

机译:设计超窄带干涉过滤器

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To understand the factors involved in the cost and risk of manufacture of ultra-narrowband imaging filters in the near IR, we have carried out detailed design work for a range of different filter specifications. This work was essential to the success of the DAZLE near-IR imaging spectrograph, a project led by the Institute of Astronomy at the University of Cambridge. The necessity for very narrow passbands (approximately 1 nm), for observing in the windows between the OH emission lines in the near-IR bands, requires coatings of more than 200 layers and greater than 30 μm thickness. Broadband filters to block OH and thermal emission over wide near-IR spectral ranges (1.4-2.8 μm) also require many thin film layers in the filter coatings. In most cases, the large number of layers is the most significant factor in determining manufacturing cost, as such coatings require long periods of time for deposition (days to weeks), with a resultant high risk of failure during manufacture.
机译:要了解近IR中超窄带成像滤波器制造成本和风险的因素,我们对一系列不同的过滤器规格进行了详细的设计工作。这项工作对于剑桥大学天文学研究所的一个项目的成功是必不可少的。对于非常窄的通带(约1nm)的必要性,用于在近红外条带中的OH发射线之间观察,需要大于200层的涂层,厚度大于30μm。宽带滤波器以阻塞OH和宽近红外光谱范围(1.4-2.8μm)的热排放也需要在过滤涂层中需要多种薄膜层。在大多数情况下,大量层是确定制造成本中最重要的因素,因为这种涂层需要长时间的沉积(天至周),因此制造过程中具有高风险的失效。

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