Image Restoration for Multiplicative Noise with Unknown Parameters

碩士 === 國立中山大學 === 電機工程學系研究所 === 94 === First, we study a Poisson model a polluted random screen. In this model, the defects on random screen are assumed Poisson-distribution and overlapped. The transmittance effects of overlapping defects are multiplicative. We can compute the autocorrelation functi...

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Bibliographic Details
Main Authors: Ren-Chi Chen, 陳仁吉
Other Authors: B.S Chow
Format: Others
Language:zh-TW
Published: 2006
Online Access:http://ndltd.ncl.edu.tw/handle/90897725447248530115
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spelling ndltd-TW-094NSYS54420932016-05-27T04:18:10Z http://ndltd.ncl.edu.tw/handle/90897725447248530115 Image Restoration for Multiplicative Noise with Unknown Parameters 乘積雜訊下容許未知參數的影像還原 Ren-Chi Chen 陳仁吉 碩士 國立中山大學 電機工程學系研究所 94 First, we study a Poisson model a polluted random screen. In this model, the defects on random screen are assumed Poisson-distribution and overlapped. The transmittance effects of overlapping defects are multiplicative. We can compute the autocorrelation function of the screen is obtained by defects'' density, radius, and transmittance. Using the autocorrelation function, we then restore the telescope astronomy images. These image signals are generally degraded by their propagation through the random scattering in atmosphere. To restore the images, we estimate the three key parameters by three methods. They are expectation- maximization (EM) method and two Maximum-Entropy (ME) methods according to two different definitions. The restoration are successful and demonstrated in this thesis. B.S Chow 周本生 2006 學位論文 ; thesis 75 zh-TW
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language zh-TW
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sources NDLTD
description 碩士 === 國立中山大學 === 電機工程學系研究所 === 94 === First, we study a Poisson model a polluted random screen. In this model, the defects on random screen are assumed Poisson-distribution and overlapped. The transmittance effects of overlapping defects are multiplicative. We can compute the autocorrelation function of the screen is obtained by defects'' density, radius, and transmittance. Using the autocorrelation function, we then restore the telescope astronomy images. These image signals are generally degraded by their propagation through the random scattering in atmosphere. To restore the images, we estimate the three key parameters by three methods. They are expectation- maximization (EM) method and two Maximum-Entropy (ME) methods according to two different definitions. The restoration are successful and demonstrated in this thesis.
author2 B.S Chow
author_facet B.S Chow
Ren-Chi Chen
陳仁吉
author Ren-Chi Chen
陳仁吉
spellingShingle Ren-Chi Chen
陳仁吉
Image Restoration for Multiplicative Noise with Unknown Parameters
author_sort Ren-Chi Chen
title Image Restoration for Multiplicative Noise with Unknown Parameters
title_short Image Restoration for Multiplicative Noise with Unknown Parameters
title_full Image Restoration for Multiplicative Noise with Unknown Parameters
title_fullStr Image Restoration for Multiplicative Noise with Unknown Parameters
title_full_unstemmed Image Restoration for Multiplicative Noise with Unknown Parameters
title_sort image restoration for multiplicative noise with unknown parameters
publishDate 2006
url http://ndltd.ncl.edu.tw/handle/90897725447248530115
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