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作 者:俞文凯[1,2,3] 姚旭日[1,2,3] 刘雪峰[1,2,3] 翟光杰[1,2] 赵清[4]
机构地区:[1]中国科学院空间科学与应用研究中心空间科学实验技术研究室,北京100190 [2]中国科学院国家空间科学中心空间科学实验技术研究室,北京100190 [3]中国科学院大学,北京100049 [4]北京理工大学物理学院,北京100081
出 处:《光学精密工程》2012年第10期2283-2292,共10页Optics and Precision Engineering
基 金:国家863高技术研究发展计划资助项目(No.2011AA120102)
摘 要:为解决灵敏度达到单光子水平的面阵探测器件其单位像素上灵敏度有限和测量数多等问题,研制了具有极高灵敏度的成像系统来实现欠采样的极弱光成像探测。该成像系统基于光子计数成像技术和压缩感知理论,利用数字微镜器件(DMD)完成随机空间光调制,通过单光子点探测器收集光子,以计数形式记录下光强值。然后,利用算法重建出极弱光照明下的图像。文中设计了相关实验,研究了测量数、光强极弱程度和测量时间对成像质量的影响。最后,引入了图像质量评价标准和系统信噪比,分析对比了实验数据。结果表明,当测量数高于信号总维度的19.5%时,系统能完美成像,信噪比可低至2.843 8dB,DMD单位像素上的平均光子数可低于1.106count/s,成像的关键在于信号的波动大于噪声的波动。该成像系统基本满足了极弱光成像探测在光强、灵敏度和采样数等方面的要求。Abstract. Since array detectors with sensitivity to single photon level were limited by sensitivity on each pixel and needed large number of measurements, an imaging system with high sensitivity was designed to realize under-sampling ultra-weak light imaging detection. This imaging system based on photon counting technique and compressed sensing theory employed a Digital Micromirror Device (DMD) to complete the random spatial light modulation, and used a single photon point detector to collect photons. The total light intensity was recorded by the form of photon counting. Then, the image of an object under ultra-weak light illumination could be reconstructed by an algorithm. The influences of the number of measurements, ultra-weak light intensity level and measurement time on the quality of imaging were investigated by experiments. Furthermore, the evaluation criterion of reconstructed image and the Signal to Noise Ratio (SNR) of the system were discussed to analyze the experimental data. The experimental results show that when the 19.5 percent of the dimension of data, it can acquire a good be even decreased to 2. 843 8 dB, and the average count of number of measurements is greater than reconstruction, the SNR of the system can photons on each pixel of the DMD can be lower than 1. 106 count/s. Experiments also prove that the key of imaging lies in the fact that the fluctuation of signal should be greater than the fluetuation of noise. It concludes that this imaging system meets the demand of ultra-weak light imaging detection for ultra-weak light intensity, high sensitivity and few measurements.
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