首页> 外文会议>Sensors, Systems, and Next-Generation Satellites XI; Proceedings of SPIE-The International Society for Optical Engineering; vol.6744 >AlGaN-based focal plane arrays for selective UV imaging at 310nm and 280nm and route toward deep UV imaging
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AlGaN-based focal plane arrays for selective UV imaging at 310nm and 280nm and route toward deep UV imaging

机译:基于AlGaN的焦平面阵列,可在310nm和280nm处进行选择性UV成像并实现深紫外成像

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The fast development of nitrides has given the opportunity to investigate AlGaN as a material for ultraviolet detection. Such camera present an intrinsic spectral selectivity and an extremely low dark current at room temperature. It can compete with technologies based on photocathodes, MCP intensifiers, back thinned CCD or hybrid CMOS focal plane arrays (FPA) for low flux measurements. AlGaN based cameras allow UV imaging without filters or with simplified ones in harsh solar blind conditions. Few results on camera have been shown in the last years, but the ultimate performances of AlGaN photodiodes couldn't be achieved due to parasitic illumination of multiplexers, responsivity of p layers in p-i-n structures, or use of cooled readout circuit. Such issues have prevented up to now a large development of this technology. We present results on focal plane array of 320×256 pixels with a pitch of 30μm for which Schottky photodiodes are multiplexed with a readout circuit protected by black matrix at room temperature. Theses focal plane present a peak reponsivity around 280nm and 310nm with a rejection of visible light of four decades only limited by internal photoemission in contact. Then we will show the capability to outdoor measurements. The noise figure is due to readout noise of the multiplexer and we will investigate the ultimate capabilities of Schottky diodes or Metal-Semiconductor-Metal (MSM) technologies to detect extremely low signal. Furthermore, we will consider deep UV measurements on single pixels MSM from 32nm to 61nm in a front side illumination configuration. Finally, we will define technology process allowing backside illumination and deep UV imaging.
机译:氮化物的快速发展为研究AlGaN作为紫外线检测材料提供了机会。这种相机在室温下具有固有的光谱选择性和极低的暗电流。它可以与基于光电阴极,MCP增强器,背面薄型CCD或混合CMOS焦平面阵列(FPA)的技术竞争,以进行低通量测量。基于AlGaN的相机允许在没有滤光镜的情况下进行UV成像,或者在恶劣的阳光盲条件下使用简化的滤镜。过去几年中几乎没有在相机上显示出任何结果,但是由于多路复用器的寄生照明,p-i-n结构中p层的响应度或使用冷却的读出电路,无法实现AlGaN光电二极管的最终性能。迄今为止,这些问题阻止了该技术的大规模发展。我们在焦距为320×256像素,间距为30μm的焦平面阵列上呈现结果,为此,肖特基光电二极管与室温下受黑矩阵保护的读出电路多路复用。这些焦平面在280nm和310nm处呈现出峰值响应度,并且仅受接触内部光发射的限制,拒绝了四十年的可见光。然后,我们将展示户外测量的功能。噪声系数是由于多路复用器的读出噪声引起的,我们将研究肖特基二极管或金属半导体金属(MSM)技术检测极低信号的极限功能。此外,我们将考虑在正面照明配置中在32nm至61nm的单个像素MSM上进行深紫外测量。最后,我们将定义允许背面照明和深紫外成像的技术过程。

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