基于MTF识别的大气模糊图象复原(英文)  被引量:3

RSTORATION OF IMAGES BLURRED BY THE ATMOSPHERE,BASED ON MEAN MTF IDENTIFICATION

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作  者:陈书海[1] 朱国富[1] 陈华[1] 张平[1] 王宝慧[1] 杜占虎 安斌[1] 冯保红[1] 杜宏亮[1] 

机构地区:[1]西北核技术研究所

出  处:《光子学报》1998年第12期1091-1097,共7页Acta Photonica Sinica

摘  要:大气传递函数(MTF),H,所引起的图象畸变可看作两个成分的贡献之和:一个确定成分<H>和一个随机成分△H而<H>又是大气扰动的平均MTF和尘埃雾气微粒MTF的和实际大气的H是完全未知的,要通过实验测量确定D.Sadot等人提出了一种改进的滤波器,其中以确定成分<H>作为滤波器的传函,而把△H作为噪音成分对待,但传函<H>的获取要依赖于实时实验测量显然,伴随PSF实验测量的方法将难以履行某些应用场合(如卫星摄影测绘)的图象复原此外,经由该方法的复原结果已被表面噪音过重由于<H>的精确解析式已被Fried等人在总结前人研究的基础上给出,并被实验所证实,但解析式中的Fried参数r0(表征能见度)仍然是未知的,依然要通过实验测量给出如果能从模糊图象本身中识别出参数r0,则可解析求得平均扰动传函<H>所以关键是如何从识别r0本文提出一种大气畸变图象复原的新方法该技术的先进性在于避开昂贵且费时的实验测量,而直接从模糊图象中识别<H>我们开发的这种识别是基于以下物理事实:1)<H>包含尘雾微粒MTF和扰动MTF的平均效果,它在秒级照相曝光时间内是确定不变的;2)模糊图象可由具有Gaus传函Hg的?A new blind method of restoration of images distorted by atmosphere is presented in this paper.In imaging through the atmosphere,the system MTF can be decomposed into the sum of its mean <H>,and random component ΔH.The <H> have been studied by Fried 6 who derived analytical expressions.This technique deals with identification of Fried parameter r 0 in expression of <H>.The identification of r 0 is based on the facts:1)<H>,including average turbulence MTF and aerosol MTF,is determinate in a few second exposure times,and located at low frequency areas;2)A approximate restoration can be obtained by Wiener filter with Caussian H g;3)<H> has the same zero cross point as the H g and the image degraded by this <H>.It will be seen that a corrected r 0 can result in a good restoration result.This is due to the main contribution on blur is <H>,while the random MTF,ΔH,can be removed by Wiener filter.

关 键 词:图象复原 传递函数 大气扰动 功率谱 MTF 

分 类 号:TN919.8[电子电信—通信与信息系统]

 

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