共查询到20条相似文献,搜索用时 31 毫秒
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针对两点温度定标算法在应用过程中曝露的问题,提出了基于变积分时间的红外焦平面非均匀性校正算法.该算法先对图像进行非线性压缩,转换为线性图像,再利用红外焦平面阵列探测元的响应特性与积分时间之间的关系,采用改变积分时间的方法拟合红外焦平面探测器的平均响应特性曲线,进行两点校正,然后对结果进行取指数操作,即得到原图非均匀校正后的图像.分别利用两点温度定标法和变积分法对航拍红外图像进行校正效果验证,同时进行了不同校正算法的非均匀性适应性评价实验.实验结果表明新算法计算量小,校正准确度高,反应速度快,并在一定程度上解决了大动态范围下响应非线性对校正性能的影响,具有很好的工程应用价值. 相似文献
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红外焦平面阵列的非均匀性噪音是制约红外成像质量的主要因素,非均匀性校正是红外焦平面器件应用的一个关键技术.本文提出了一种基于焦平面归一化响应特性且易于实现的非均匀性校正算法,并基于像元分布的卡方直方图提出一种新的图像非均匀性评估方法,即校正比例.该方法的校正输出考虑了每个像元的观测值与焦平面的响应信号的平均值,校正参量通过将像元的输出与其理想校正结果之间的偏差用焦平面响应的平均值建立联系而计算得到.提出的校正比例兼顾考虑了焦平面响应的时间与空间特性,比现有的图像非均匀性评估方法更能合理衡量焦平面的非均匀性程度.多种非均匀性校正的评价数据以及实验结果表明,该算法的校正效果优于两点校正法与原值拟合二阶校正法,并对于响应异常的像元具有较强的校正能力.此外其校正准确度高,所需参量少,易于实时处理,具有较强的实用价值. 相似文献
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针对红外遥感图像非均匀性的定量评价问题,研究了基于场景的红外焦平面阵列响应非均匀性的定量评价方法。利用真实红外遥感图像序列量值分布的特点,针对小序列图像提出了基于序列排序和小波变换的标准图像构建算法;结合非均匀性评价指标,提出了利用构建标准图像的响应非均匀性对红外图像的非均匀性进行定量估计;分别利用黑体定标实验和统计方法对标准图像构建算法进行了验证,同时进行了不同校正算法的剩余非均匀性评价实验。结果表明,128frame序列构建得到的标准图像的非均匀性分别比同温黑体图像小0.92%,比统计标准图像大0.59%。该方法可用于定量估计红外遥感图像的非均匀性。 相似文献
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基于稳态卡尔曼滤波的红外焦平面阵列非均匀校正算法 总被引:3,自引:1,他引:2
传统的卡尔曼滤波算法利用批处理实现非均匀校正,这样不仅会带来较大的计算量和存储量,而且更重要的是该方法不能实时处理.为此,提出了一种基于稳态卡尔曼滤波的红外焦平面阵列非均匀校正算法,它可以根据固定图案噪声的特点离线计算出滤波器的增益矩阵,并且非均匀校正过程也采用了逐帧迭代方式,因此大大降低了计算复杂度和存储占用量.详细阐述了该算法的基本原理,并用仿真数据和真实红外数据对算法性能进行验证,实验结果表明:本方法平均校正一帧图像所需CPU时间和内存占用量分别为1.7188 s和131.25 KB,完全可以满足实时处理的要求. 相似文献
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基于低次插值的红外焦平面器件非均匀性多点校正算法 总被引:22,自引:5,他引:17
提出了分段线性插值和三次样条插值两种基于低次插值的红外焦平面阵列非均匀性多点校正算法,该算法能有效地克服工程上常用的一点和二点校正算法的不足,具有校正精度高、动态范围大、在线计算量小、易于实时实现等优点,并且能有效克服IRFPA各探测单元响应特性的非线性对校正精度的影响. 相似文献
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The spatial fixed-pattern noise (FPN) reduces the quality of the infrared image seriously, even makes infrared images inappropriate for some applications. In order to lower the FPN, some critical nonuniformity correction (NUC) algorithms such as NUC based on linear model, scene-based NUC and so on have been developed. But the algorithms have some drawbacks: restricted application in small dynamic range of objects temperature, low performance under the drift with the working time and complex calculations. In these cases, we develop a bivariate and quadratic model (bivariate is radiation and working time) of the FPA and the NUC technique based on the model. The proposed method is a true reflection of the infrared response and is a good solution for hardware implementation. It overcomes the drawbacks of the critical algorithm mentioned above. The last simulations and experiments show that the proposed algorithm exhibits a superior correction effect in both large objects temperature range and long working time of the thermal imager. 相似文献
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Chao Zuo Qian Chen Guohua Gu Xiubao Sui Jianle Ren 《Infrared Physics & Technology》2012,55(4):263-269
In this paper, an improved interframe registration based nonuniformity correction algorithm for focal plane arrays is proposed. The method simultaneously estimates detector parameters and carries out the nonuniformity correction by minimizing the mean square error between the two properly registered image frames. A new masked phase correlation algorithm is introduced to obtain reliable shift estimates in the presence of fixed pattern noise. The use of an outliers exclusion scheme, together with a variable step size strategy, could not only promote the correction precision considerably, but also eliminate ghosting artifacts effectively. The performance of the proposed algorithm is evaluated with clean infrared image sequences with simulated nonuniformity and real pattern noise. We also apply the method to a real-time imaging system to show how effective it is in reducing noise and the ghosting artifacts. 相似文献
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本文综述了星敏感器技术的研究现状和未来发展趋势。首先,总结了国内外星载星敏感器的发展历程。接着,根据星敏感器工作原理,分析讨论了星点质心定位算法、星图识别算法和姿态解算算法等星敏感器关键技术的发展现状。通过讨论星点质心定位精度对星敏感器测量精度影响,分析了星点质心定位算法以及对应误差补偿的研究现状;基于星座特征、字符模式和智能行为,介绍了星图识别算法并进行了对比分析;根据确定姿态解算算法和动态姿态解算算法分析了姿态解算算法的研究现状。最后,对星敏感器的未来发展进行了展望,讨论了航空机载星敏感器、微小型星敏感器和甚高精度星敏感器的发展趋势以及未来重点研究内容。 相似文献
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Zhifeng Zhang Zhangye Wang Guotu Sheng Changbo Wang Qunsheng Peng 《International Journal of Infrared and Millimeter Waves》2005,26(11):1627-1638
This paper proposes a new method to generate the dynamic infrared outer space scene in real time. In the paper, we first model
the dynamic infrared background of star sky based on the infrared star catalogue and temporal and spacial coordinate transformations.
We also present a new concept called infrared star magnitude for given infrared receiving wavebands to display the infrared
star sky effectively. Then we put forward an infrared image synthesis model for outer space targets based on the method of
divided elements and energy equilibrium. To generate the dynamic infrared outer space scene, several simplification and accelerating
techniques such as Billboard, Levels of Details and Occlusion Culling are hired to accelerate the generating speed of the
scene. Finally infrared images of targets, background of outer space scene at different infrared receiving wavebands are drawn
and the dynamic infrared outer space scene is successfully carried out in real time.
* Corresponding author 相似文献