用于质球冷离子成像的两款薄膜滤光片的新型极紫外透射测量结果

IF 1.7 3区 工程技术 Q2 ENGINEERING, AEROSPACE Journal of Astronomical Telescopes Instruments and Systems Pub Date : 2024-03-01 DOI:10.1117/1.jatis.10.1.015003
Philippa Molyneux, Todd Veach, Michael Davis, Gregory Fletcher, Jerry Goldstein
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引用次数: 0

摘要

我们展示了两款薄膜滤光片的极紫外(EUV)透射测量结果,这两款滤光片的设计目的是获得更好的质球He+图像,以及致密氧环中O+/O++的首批全局图像。与之前使用铝滤光片的 He+ 30.4 nm 成像相比,我们发现铝+碳组合滤光片能更好地抑制来自中性氦(He I)的 58.4 nm 背景。我们的研究表明,铟滤光片既能满足 83.4 纳米波长的透射要求,又能充分抑制较亮的 He I(58.4 纳米波长)和 H I(121.6 纳米波长)背景发射。我们发现,58.4 nm 波长处的铟透射率比根据 λ<68 nm 处的内插光学常数预测的值低 ∼ 16 倍。我们表明,观测到的较低的 58.4 nm 波长透射率与以前实验室测量得出的其他光学常数是一致的。
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New extreme ultraviolet transmission measurements of two thin-film filters for imaging of plasmaspheric cold ions
We present extreme ultraviolet (EUV) transmission measurements of two thin-film filters designed to obtain improved images of plasmaspheric He+, and the first global images of O+/O++ in the dense oxygen torus. Compared to previous He+ 30.4 nm imaging that used an Al filter, we show that a combined Al+C filter achieves superior rejection of 58.4 nm background from neutral helium (He I). We show that an indium filter provides both the required transmission at 83.4 nm and adequate rejection of brighter He I (58.4 nm) and H I (121.6 nm) background emissions. We find that the In transmission at 58.4 nm is a factor of ∼16 lower than predicted based on optical constants that rely on interpolations at λ<68 nm. We show that the observed lower 58.4 nm transmission is consistent with alternative optical constants derived from previous lab measurements.
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来源期刊
CiteScore
4.40
自引率
13.00%
发文量
119
期刊介绍: The Journal of Astronomical Telescopes, Instruments, and Systems publishes peer-reviewed papers reporting on original research in the development, testing, and application of telescopes, instrumentation, techniques, and systems for ground- and space-based astronomy.
期刊最新文献
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