Modern UV detectors for small aperture space mission to study comets

IF 0.4 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Contributions of the Astronomical Observatory Skalnate Pleso Pub Date : 2021-12-01 DOI:10.31577/caosp.2021.51.3.257
A. Shugarov
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Abstract

A small dedicated UV telescope with a modern detector can obtain a lot of new information to study comets in the UV range, which is inaccessible for ground telescopes. We discuss the latest trends in UV-optimized CMOS and CCD detectors that can improve the efficiency of a small aperture (20 cm) space burn UV telescope. The improvements of classical CCD are moving toward improving quantum efficiency in UV, development of the new anti-reflection coatings and multilayer UV filters with enhanced red leak suppression. CMOS with a very small pixel (3-5μm) of more than 20 Mpixel format allows to improve sampling and to increase the price/performance ratio of a small aperture telescope.
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用于研究彗星的小孔径太空任务的现代紫外线探测器
配备现代探测器的小型专用紫外线望远镜可以获得许多新信息,用于研究紫外线范围内的彗星,而地面望远镜无法获得这些信息。我们讨论了紫外线优化CMOS和CCD探测器的最新趋势,这些探测器可以提高小孔径(20厘米)空间燃烧紫外线望远镜的效率。经典CCD的改进正在朝着提高紫外线量子效率、开发新型抗反射涂层和增强红色泄漏抑制的多层紫外线滤光片的方向发展。CMOS具有超过20M像素格式的非常小的像素(3-5μm),可以改进采样并提高小孔径望远镜的性价比。
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来源期刊
CiteScore
1.10
自引率
20.00%
发文量
4
审稿时长
>12 weeks
期刊介绍: Contributions of the Astronomical Observatory Skalnate Pleso" (CAOSP) is published by the Astronomical Institute of the Slovak Academy of Sciences (SAS). The journal publishes new results of astronomical and astrophysical research, preferentially covering the fields of Interplanetary Matter, Stellar Astrophysics and Solar Physics. We publish regular papers, expert comments and review contributions.
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