数字成像仪中的单事件干扰和热像素

G. Chapman, Rahul Thomas, Rohan Thomas, Klinsmann J. Coelho Silva Meneses, Tommy Q. Yang, I. Koren, Z. Koren
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引用次数: 6

摘要

通过对数码成像仪缺陷的广泛研究,我们发现永久性的“热像素”是数码相机主要的长期缺陷,它是由高能宇宙射线粒子引起的。显然,与其他微电子集成电路一样,大多数粒子不会造成永久性损坏,而是注入短期电荷,可能导致瞬态故障,即所谓的单事件扰动(SEU)。与标准数字集成电路不同,数字成像传感器中的像素几乎可以在任何期望的频率下进行监测。由于单亮度单位表现为在暗图像中显示一个或多个更亮的像素,因此通过在不同曝光时间和不同频率下拍摄暗场图像,可以以相当高的精度测量单亮度单位的速率。在本文中,我们描述了一种实验方法来测量seu的发生率和产生的特性。我们在数字成像仪上观察到的SEU速率为每30秒约4 SEU,远远高于之前报道的普通ic。对于相同的成像仪,永久热像素的频率为每12.6天1次,而seu的频率为14.5万倍。据报道,普通IC的SEU率约为永久故障率的100倍。此外,我们发现数字成像仪中的一些seu不会像热像素那样影响单个像素,但会产生一条注入电荷线,在暗图像中显示为一条亮线。
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Single Event Upsets and Hot Pixels in digital imagers
From extensive study of digital imager defects, we found that permanent “Hot Pixels” are the main long term digital camera defects, and are caused by high energy cosmic ray particles. Clearly, as in other microelectronic integrated circuits, most of the particles do not induce permanent damage but instead, inject a short term charge that may cause a transient fault, known as a Single Event Upset (SEU). Unlike standard digital ICs, pixels in a digital imaging sensor can be monitored at almost any desirable frequency. Since an SEU manifests itself as one or more brighter pixels in an otherwise dark image, the rate of SEUs can be measured at a considerably higher accuracy by taking dark-field pictures at different exposure times and different frequencies. In this paper we describe an experimental approach to measuring the occurrence rate and resulting characteristics of SEUs. The SEU rate that we have observed for digital imagers, of about 4 SEUs for every 30 seconds, is considerably higher than was previously reported for ordinary ICs. For the same imager, permanent hot pixels have a rate of 1 every 12.6 days, while SEUs occur 145,000 times more often. Ordinary IC SEU rates have been reported to be about 100× of permanent fault rates. In addition, we found that some SEUs in digital imagers do not impact a single pixel, as do hot pixels, but can create a line of injected charges which appears as a bright line in the dark image.
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