共查询到20条相似文献,搜索用时 15 毫秒
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帧转移型CCD传感器在拍摄星空背景图像时,视场中高亮度恒星会产生Smear现象,从而对目标检测有严重影响.为了消除Smear现象,提出了一种星图中基于小波变换的Smear消除方法.首先根据Smear产生机理及星空图像特性,建立星图Smear问题的模型|然后使用多层二维Haar小波分解,把Smear亮线分离到低频分量及高频垂直分量中分别进行Smear消除处理|最后重构出消除Smear的图像.实验结果表明:该方法能有效去除Smear,最大限度保留图像原有信息,并可增强Smear区域弱小目标信噪比. 相似文献
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为了实现对星空观测图像中高亮目标产生的拖尾现象进行自动消除,建立了目标拖尾自动消除系统,对该系统所采用的图像背景高斯噪声分布参数估计、目标拖尾检测以及图像灰度值校正等算法进行研究。利用直方图最小二乘曲线拟合估计星空观测图像背景高斯噪声的分布参数;利用观测图像中目标拖尾现象的特征提出一种基于统计信息的拖尾检测算法;在确定目标拖尾位置的基础上对被污染的像素进行灰度值校正;利用Visual Studio 2005开发出一套星空观测图像目标拖尾自动消除系统。实验结果表明:针对16 bit,1 0241 024的星空观测图像,单帧图像处理时间约为300 ms,拖尾现象得到消除,恒星和目标等有用信息未被破坏。本文算法基本满足后续观测图像中弱小目标检测稳定、可靠、精度高等要求。 相似文献
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在用532nm连续激光辐照TCD-1200D型线阵CCD的过程中,发现了光斑的全饱和单侧拖尾现象。为了分析这种现象的特性,实验测量了拖尾长度随激光功率、CCD积分时间和CCD驱动频率的关系,发现拖尾长度随着激光功率和积分时间的增加而增加,但在一定范围内与CCD驱动频率无关。通过理论计算和实验数据分析拟合发现,拖尾长度和激光功率密度和积分时间的乘积有关,并根据激光辐照下CCD器件光生电荷量的产生过程,推导出了拖尾长度与CCD势阱光生电荷量的关系,得到了拖尾长度随光生电荷量的变化曲线,为全饱和单侧拖尾现象机理分析提供了数据支持。 相似文献
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利用532 nm连续激光辐照以东芝TCD1200D型线阵CCD为图像传感器的扫描相机进行实验,在相机输出视频中发现了光斑拖尾的现象,拖尾有限长、全饱和并且仅在光斑一侧。分析排除了光分布造成拖尾的可能原因。其单侧、有限长的特点不符合像素溢出或漏光造成的拖尾,而与转移损失造成的拖尾一致。但其全饱和的特点,不符合目前转移损失率的常数模型。针对当前体沟道CCD的内部结构和工作原理,提出了一种转移损失率随电荷量变化的模型,对新发现的全饱和单侧拖尾进行了解释。 相似文献
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将分子成像技术和高光谱技术相结合,研制了基于AOTF(Acousto-optic Tunable Filters)的分子高光谱成像系统。系统由显微镜、分光仪、CCD镜头、图像数据采集卡和计算机等几部分组成。在综合考虑各功能部件的性能及相互的制约关系的基础上,分析了系统的性能指标,系统的光谱范围从550~1 000 nm,可采集200个波段,空间分辨率可达0.061 5 μm,光谱分辨率可达2 nm,当CCD工作在积分模式下采集速度可达到2.612 5 s·B-1,当CCD工作在非积分模式下可达到约0.11 μs·B-1。由于受系统光源和光路中透镜及传感器性能的影响,采集到的图像数据需要进行预处理,文中提出一种空间维和光谱维联合校正的灰度校正系数算法,并给出算法的具体实现。以白血病的血液作样本,通过对比校正前后的单波段图像、伪彩色图像和光谱曲线,说明校正算法的有效性,为后续的光谱图像数据分析提供了有效的数据。 相似文献
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In the photoelectric tracking system, the detection of space multi-target is crucial for target localization and tracking. The difficulties include the interferences from CCD smear and strong noise, the few characteristics of spot-like targets and the challenge of multiple targets. In this paper, we propose a hybrid algorithm of joint decision and Naive Bayes (JD-NB) learning, and present the duty ratio feature to discriminate the target and smear blocks. Firstly, we extract the proper features and train the parameters of the Naive Bayes classifier. Secondly, target blocks are preliminarily estimated with the Naive Bayes. Lastly, the 4-adjacent blocks of the candidate target blocks are jointed to analyze the distribution pattern and the true target blocks are secondarily extracted by the method of pattern matching. Experimental results indicate that the proposed JD-NB algorithm not only possesses a high recognition rate of better than 90% for the target block, but also effectively overcomes the disturbance of the smear block. Moreover, it performs well in the detection of small and faint targets when the SNR of the block is higher than about 0.014. 相似文献
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When the speeds of objects in a scene exceed the temporal resolution of the camera shutter, motion blurs will occur. Since objects are often moving in different directions at different speeds, the degradation of a CCD image is often characterized by space-variant motion blurs. Image restoration algorithms for space-variant motion blurs are available for progressive scan CCD images, but not for interlaced scan images. To address the space-variant image restoration for interlaced scan images, a novel three-step image restoration scheme is proposed. Firstly, one interlaced scan image is divided into odd field and even field images. Secondly, these two field images are further segmented into rectangular blocks and the motion vectors are computed based on these rectangular blocks using an efficient block matching algorithm. Thirdly, image restoration is performed using a blind deconvolution algorithm in the odd or even field image. The final restored image is obtained by combining the restored odd and even field images. The scheme is illustrated by restoring a space-variant blurred moving vehicle image and a synthetic blurred image. 相似文献
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针对CCD图像输出时间长影响其帧频率的问题,提出了一种基于普通CCD实现超高帧频成像的方法.采用掩膜覆盖CCD的光敏区,建立图像的片上存储空间,消除CCD电荷转移输出占用过多时间的影响,可以使普通CCD的帧频达到每秒百万帧频以上.介绍了不同掩膜实现方案的优缺点,讨论了掩膜图像的恢复方法,采用条状孔掩膜方式建立了基于普通CCD的每秒百万帧高帧频成像系统样机,利用氙灯对样机性能进行验证,获得了14幅79×79像素的氙灯发光过程图像,样机帧频率达到了每秒200万帧的超高速度. 相似文献
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A new 3D-PTV technique has been developed using GA (Genetic Algorithm). The measurement system consists of three CCD cameras,
Ar-ion laser, an image grabber and a host computer. One-to-one correspondences are made by taking advantage of the combinatorial
optimization of the genetic algorithm for the whole particles of the two images during the time interval of image frames.
Two fitness functions are introduced in order to enhance the correspondences of the particles. One is based on the concept
of continuum theory and the other one is based on the minimum error of threedimensional distance. Performance of the developed
algorithm is tested using a set of virtual images constructed by the use of LES data set on an impinging jet. The developed
3D-PTV system is successfully applied to the measurement of flow characteristics of the wake of a circular cylinder. 相似文献
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Motion blur is caused by camera shakes or object motions during exposure when the shutter speed is relatively slow. As for the object motion blur, the degradation of a CCD image is often characterized by space-variant motion blurs, since objects are often moving in different directions at different speeds. But most image restorations for space-variant motion blurs are addressed only for progressive scan CCD images. To address the space-variant image restorations for interlaced scan images, we propose a novel image restoration scheme. First, one interlaced scan image frame is required, which is divided into the odd field and the even field images. These two field images are further segmented into rectangular blocks. The motion vectors are computed in these rectangular blocks using an efficient block matching algorithm. Second, image restoration is performed in these rectangular blocks using a constrained least square algorithm in the odd or even field image, which can both preserve edge structures and remove noises. Our novel scheme is illustrated by restoring a space-variant blurred moving boat image and a synthetic blurred image. 相似文献
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The Space multi-band Variable Object Monitor (SVOM) is a proposed Chinese astronomical satellite, dedicated to the detection, localization and measurement of gamma-ray bursts (GRBs) on a cosmological scale. An efficient algorithm is developed for the purpose of onboard star extraction from the CCD images obtained with the Visible Telescope (VT) onboard the SVOM. The CCD pixel coordinates of the reference stars will be used to refine the astronomical position of the satellite, which will facilitate triggering rapid ground-based follow-up observations of the GRBs. In this algorithm, the image is divided into a number of grid cells and the “global” pixel-value maximum within each cell is taken as the first-guess position of a “bright” star. The correct center position of a star is then computed using a simple iterative method. Applying two additional strategies, i.e., scanning the image only by even (or odd) lines or in a black-white chess board mode, we propose to further reduce the time to extract the stars. To examine the efficiency of the above algorithms, we applied them to the experimental images obtained with a ground-based telescope. We find that the accuracy of the astronomical positioning achieved by our method is comparable to that derived by using the conventional star-extraction method, while the former needs about 25 times less CPU time than the latter. This will significantly improve the performance of the SVOM VT mission. 相似文献