2008 International Workshop on Education Technology and Training &Amp; 2008 International Workshop on Geoscience and Remote Sen 2008
DOI: 10.1109/ettandgrs.2008.125
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Noise Analysis and Image Restoration for Optical Sparse Aperture Systems

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Cited by 8 publications
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“…In real observation condition, images collected by CCD are inevitably affected by noises. As far as synthetic aperture imaging system is concerned, there are three main sources of noises, namely the photon noise, dark current noise and readout noise 9,10 . The photon noise is defined as the number of optoelectronics generated by background radiation in the observations field while dark current noise is the number of photoelectrons generated by CCD heating, both of which collectively refer to background noise and follow Poisson distribution; readout noise generate in the procedure of reading the signal from the sensor, which occupies a major part in the signal-weak regions and can be considered to be under the Gaussian distribution.…”
Section: Noise Influence and Accuracy Analysismentioning
confidence: 99%
“…In real observation condition, images collected by CCD are inevitably affected by noises. As far as synthetic aperture imaging system is concerned, there are three main sources of noises, namely the photon noise, dark current noise and readout noise 9,10 . The photon noise is defined as the number of optoelectronics generated by background radiation in the observations field while dark current noise is the number of photoelectrons generated by CCD heating, both of which collectively refer to background noise and follow Poisson distribution; readout noise generate in the procedure of reading the signal from the sensor, which occupies a major part in the signal-weak regions and can be considered to be under the Gaussian distribution.…”
Section: Noise Influence and Accuracy Analysismentioning
confidence: 99%
“…One of the most common methods used to achieve image restoration is Wiener filter [2] [3]. However, during real imaging process, the precise estimation of transfer function and signal-to-noise ratio (SNR) cannot be obtained due to the influences of noises and phase errors, which restrains the capability of Wiener filter.…”
Section: Introductionmentioning
confidence: 99%
“…The noise affecting a given area of a homogeneous SAR image is classically supposed to be a multiplicative speckle noise with gamma or Weibull distribution [44]- [46]. Conversely, the noise affecting optical images has been considered as an additive Gaussian noise in many applications [47], [48]. The model considered in this study takes advantage of the relationships between the sensor responses to the objects contained in the observed scene, the physical properties of these objects and the statistical properties of the noise corrupting the images.…”
mentioning
confidence: 99%