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Near Ultraviolet Spectrograph for Balloon Platform

机译:气球平台用近紫外光谱仪

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Small and compact scientific payloads may be easily designed constructed and flown on high altitude balloons. Despite the fact that large orbital observatories provide accurate observations and statistical studies of remote and/or faint space sources, small telescopes on board balloons or rockets are still attractive because of their low cost and rapid response time. We describe here a near ultraviolet (NUV) spectrograph designed to be flown on a high-altitude balloon platform. Our basic optical design is a modified Czerny-Turner system using off the shelf optics. We compare different methods of aberration corrections in such a system. We intend the system to be portable and scalable to different telescopes. The use of reflecting optics reduces the transmission loss in UV. We plan on using an image intensified CMOS sensor operating in photon counting mode as the detector of choice.
机译:小型紧凑的科学有效载荷可以轻松设计并在高空气球上飞行。尽管大型轨道天文台提供了对遥远和/或微弱空间源的准确观测和统计研究,但气球或火箭上的小型望远镜仍然具有吸引力,因为它们的成本低且响应时间短。我们在这里介绍一种设计用于在高空气球平台上飞行的近紫外(NUV)光谱仪。我们的基本光学设计是使用现成的光学器件的改进的Czerny-Turner系统。我们比较了这种系统中像差校正的不同方法。我们希望该系统具有可移植性,并且可以扩展到不同的望远镜。使用反射光学器件可减少紫外线的透射损耗。我们计划使用以光子计数模式运行的图像增强型CMOS传感器作为首选检测器。

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