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Development of sensitive long-wave infrared detector arrays for passively cooled space missions

机译:敏感长波红外探测器阵列的研制   被动冷却的太空任务

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摘要

The near-earth object camera (NEOCam) is a proposed infrared space missiondesigned to discover and characterize most of the potentially hazardousasteroids larger than 140 m in diameter that orbit near the Earth. NASA hasfunded technology development for NEOCam, including the development of longwavelength infrared detector arrays that will have excellent zodiacalbackground emission-limited performance at passively cooled focal planetemperatures. Teledyne Imaging Sensors has developed and delivered for test atthe University of Rochester the first set of approximately 10 micron cutoff,1024 x 1024 pixel HgCdTe detector arrays. Measurements of these arrays show thedevelopment to be extremely promising: noise, dark current, quantum efficiency,and well depth goals have been met by this technology at focal planetemperatures of 35 to 40 K, readily attainable with passive cooling. The nextset of arrays to be developed will address changes suggested by the first setof deliverables.
机译:近地天体摄像机(NEOCam)是一项拟议的红外太空任务,旨在发现和表征绕地球运行的直径大于140 m的大多数潜在危险小行星。美国国家航空航天局(NASA)已资助NEOCam的技术开发,包括开发长波长红外探测器阵列,该阵列将在被动冷却焦平面温度下具有出色的黄道背景发射限制性能。 Teledyne Imaging Sensors已开发并交付了第一批约10微米截止波长,1024 x 1024像素的HgCdTe检测器阵列,并在罗切斯特大学进行了测试。对这些阵列的测量表明,该技术的发展非常有希望:在35至40 K的焦平面温度下,通过被动冷却即可轻松达到该技术的噪声,暗电流,量子效率和阱深度目标。下一组要开发的阵列将解决第一组可交付成果建议的更改。

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